0s autopkgtest [00:59:23]: starting date and time: 2024-04-19 00:59:23+0000 0s autopkgtest [00:59:23]: git checkout: 43bc6cdf gitlab-ci: do not include the salsa pipeline 0s autopkgtest [00:59:23]: host juju-7f2275-prod-proposed-migration-environment-4; command line: /home/ubuntu/autopkgtest/runner/autopkgtest --output-dir /tmp/autopkgtest-work.cgcjak3g/out --timeout-copy=6000 --setup-commands 'dhclient || true; ln -s /dev/null /etc/systemd/system/bluetooth.service; printf "http_proxy=http://squid.internal:3128\nhttps_proxy=http://squid.internal:3128\nno_proxy=127.0.0.1,127.0.1.1,login.ubuntu.com,localhost,localdomain,novalocal,internal,archive.ubuntu.com,ports.ubuntu.com,security.ubuntu.com,ddebs.ubuntu.com,changelogs.ubuntu.com,launchpadlibrarian.net,launchpadcontent.net,launchpad.net,10.24.0.0/24,keystone.ps5.canonical.com,objectstorage.prodstack5.canonical.com\n" >> /etc/environment' --apt-pocket=proposed=src:gsl --apt-upgrade cpl-plugin-fors --timeout-short=300 --timeout-copy=20000 --timeout-build=20000 --env=ADT_TEST_TRIGGERS=gsl/2.7.1+dfsg-6ubuntu2 -- lxd -r lxd-armhf-10.145.243.182 lxd-armhf-10.145.243.182:autopkgtest/ubuntu/noble/armhf 28s autopkgtest [00:59:51]: testbed dpkg architecture: armhf 30s autopkgtest [00:59:53]: testbed apt version: 2.7.14build2 30s autopkgtest [00:59:53]: @@@@@@@@@@@@@@@@@@@@ test bed setup 38s Get:1 http://ftpmaster.internal/ubuntu noble-proposed InRelease [117 kB] 38s Get:2 http://ftpmaster.internal/ubuntu noble-proposed/universe Sources [376 kB] 38s Get:3 http://ftpmaster.internal/ubuntu noble-proposed/main Sources [54.2 kB] 38s Get:4 http://ftpmaster.internal/ubuntu noble-proposed/multiverse Sources [2340 B] 38s Get:5 http://ftpmaster.internal/ubuntu noble-proposed/restricted Sources [12.2 kB] 38s Get:6 http://ftpmaster.internal/ubuntu noble-proposed/main armhf Packages [82.2 kB] 38s Get:7 http://ftpmaster.internal/ubuntu noble-proposed/main armhf c-n-f Metadata [2492 B] 38s Get:8 http://ftpmaster.internal/ubuntu noble-proposed/restricted armhf Packages [976 B] 38s Get:9 http://ftpmaster.internal/ubuntu noble-proposed/restricted armhf c-n-f Metadata [116 B] 38s Get:10 http://ftpmaster.internal/ubuntu noble-proposed/universe armhf Packages [459 kB] 40s Get:11 http://ftpmaster.internal/ubuntu noble-proposed/universe armhf c-n-f Metadata [7776 B] 40s Get:12 http://ftpmaster.internal/ubuntu noble-proposed/multiverse armhf c-n-f Metadata [116 B] 40s Fetched 1114 kB in 1s (974 kB/s) 40s Reading package lists... 56s sh: 1: dhclient: not found 58s tee: /proc/self/fd/2: Permission denied 90s Hit:1 http://ftpmaster.internal/ubuntu noble-proposed InRelease 90s Hit:2 http://ftpmaster.internal/ubuntu noble InRelease 90s Hit:3 http://ftpmaster.internal/ubuntu noble-updates InRelease 90s Hit:4 http://ftpmaster.internal/ubuntu noble-security InRelease 91s Reading package lists... 91s Reading package lists... 92s Building dependency tree... 92s Reading state information... 92s Calculating upgrade... 93s The following packages will be upgraded: 93s apport apport-core-dump-handler apport-symptoms base-passwd bcache-tools 93s bind9-dnsutils bind9-host bind9-libs bzip2 cloud-init cpio cryptsetup-bin 93s dbus dbus-bin dbus-daemon dbus-session-bus-common dbus-system-bus-common 93s dbus-user-session diffutils dmidecode dracut-install e2fsprogs 93s e2fsprogs-l10n eatmydata ethtool findutils ftp gcc-13-base gcc-14-base 93s gettext-base grep gzip hdparm hostname htop iptables iputils-ping 93s iputils-tracepath kmod libacl1 libargon2-1 libassuan0 libatasmart4 libattr1 93s libbytesize-common libbytesize1 libbz2-1.0 libcap2 libcap2-bin libcom-err2 93s libcrypt1 libcryptsetup12 libdb5.3t64 libdbus-1-3 libdrm-common libdrm2 93s libeatmydata1 libedit2 libestr0 libevdev2 libext2fs2t64 libfastjson4 libffi8 93s libfido2-1 libflashrom1 libfribidi0 libgcc-s1 libgcrypt20 libgmp10 93s libgpg-error-l10n libgpg-error0 libicu74 libidn2-0 libinih1 libip4tc2 93s libip6tc2 libjson-c5 libkeyutils1 libkmod2 liblmdb0 liblz4-1 liblzo2-2 93s libmaxminddb0 libmd0 libmnl0 libmpfr6 libncurses6 libncursesw6 93s libnetfilter-conntrack3 libnfnetlink0 libnftables1 libnftnl11 libnghttp2-14 93s libnl-3-200 libnl-genl-3-200 libnl-route-3-200 libnspr4 libnss3 libnuma1 93s libonig5 libp11-kit0 libpam-cap libpam-modules libpam-modules-bin 93s libpam-runtime libpam0g libpci3 libpcre2-8-0 libpopt0 libpython3-stdlib 93s libpython3.12-minimal libpython3.12-stdlib libsepol2 libsgutils2-1.46-2 93s libsigsegv2 libss2 libstdc++6 libtasn1-6 libtinfo6 libuchardet0 93s libunistring5 libutempter0 libx11-6 libx11-data libxau6 libxdmcp6 libxext6 93s libxkbcommon0 libxmlb2 libxtables12 libxxhash0 libyaml-0-2 libzstd1 login 93s logrotate logsave make man-db mawk nano ncurses-base ncurses-bin 93s ncurses-term netcat-openbsd nftables numactl openssh-client openssh-server 93s openssh-sftp-server passwd patch pci.ids pciutils python-apt-common python3 93s python3-apport python3-apt python3-cffi-backend python3-gdbm python3-minimal 93s python3-netifaces python3-problem-report python3-systemd python3.12 93s python3.12-minimal rsync rsyslog screen sed sg3-utils sg3-utils-udev sudo 93s sysstat sysvinit-utils tar tcpdump time tnftp tzdata ufw usb.ids usbutils 93s xauth xdg-user-dirs xkb-data zstd 93s 186 upgraded, 0 newly installed, 0 to remove and 0 not upgraded. 93s Need to get 43.7 MB of archives. 93s After this operation, 585 kB disk space will be freed. 93s Get:1 http://ftpmaster.internal/ubuntu noble/main armhf diffutils armhf 1:3.10-1build1 [167 kB] 93s Get:2 http://ftpmaster.internal/ubuntu noble/main armhf findutils armhf 4.9.0-5build1 [293 kB] 93s Get:3 http://ftpmaster.internal/ubuntu noble/main armhf grep armhf 3.11-4build1 [157 kB] 93s Get:4 http://ftpmaster.internal/ubuntu noble/main armhf gzip armhf 1.12-1ubuntu3 [95.8 kB] 93s Get:5 http://ftpmaster.internal/ubuntu noble/main armhf hostname armhf 3.23+nmu2ubuntu2 [10.4 kB] 93s Get:6 http://ftpmaster.internal/ubuntu noble/main armhf login armhf 1:4.13+dfsg1-4ubuntu3 [200 kB] 93s Get:7 http://ftpmaster.internal/ubuntu noble/main armhf ncurses-bin armhf 6.4+20240113-1ubuntu2 [178 kB] 93s Get:8 http://ftpmaster.internal/ubuntu noble/main armhf sed armhf 4.9-2build1 [190 kB] 93s Get:9 http://ftpmaster.internal/ubuntu noble/main armhf tar armhf 1.35+dfsg-3build1 [236 kB] 93s Get:10 http://ftpmaster.internal/ubuntu noble/main armhf base-passwd armhf 3.6.3build1 [50.9 kB] 93s Get:11 http://ftpmaster.internal/ubuntu noble/main armhf ncurses-base all 6.4+20240113-1ubuntu2 [25.5 kB] 93s Get:12 http://ftpmaster.internal/ubuntu noble/main armhf ncurses-term all 6.4+20240113-1ubuntu2 [275 kB] 94s Get:13 http://ftpmaster.internal/ubuntu noble/main armhf sysvinit-utils armhf 3.08-6ubuntu3 [33.8 kB] 94s Get:14 http://ftpmaster.internal/ubuntu noble/main armhf libcrypt1 armhf 1:4.4.36-4build1 [92.6 kB] 94s Get:15 http://ftpmaster.internal/ubuntu noble/main armhf libpam0g armhf 1.5.3-5ubuntu5 [62.1 kB] 94s Get:16 http://ftpmaster.internal/ubuntu noble/main armhf libpam-modules-bin armhf 1.5.3-5ubuntu5 [47.0 kB] 94s Get:17 http://ftpmaster.internal/ubuntu noble/main armhf libpam-modules armhf 1.5.3-5ubuntu5 [260 kB] 94s Get:18 http://ftpmaster.internal/ubuntu noble/main armhf e2fsprogs-l10n all 1.47.0-2.4~exp1ubuntu4 [5998 B] 94s Get:19 http://ftpmaster.internal/ubuntu noble/main armhf logsave armhf 1.47.0-2.4~exp1ubuntu4 [22.0 kB] 94s Get:20 http://ftpmaster.internal/ubuntu noble/main armhf libext2fs2t64 armhf 1.47.0-2.4~exp1ubuntu4 [202 kB] 94s Get:21 http://ftpmaster.internal/ubuntu noble/main armhf e2fsprogs armhf 1.47.0-2.4~exp1ubuntu4 [571 kB] 94s Get:22 http://ftpmaster.internal/ubuntu noble/main armhf tzdata all 2024a-2ubuntu1 [273 kB] 94s Get:23 http://ftpmaster.internal/ubuntu noble/main armhf python3.12 armhf 3.12.3-1 [651 kB] 94s Get:24 http://ftpmaster.internal/ubuntu noble/main armhf bzip2 armhf 1.0.8-5.1 [33.5 kB] 94s Get:25 http://ftpmaster.internal/ubuntu noble/main armhf libbz2-1.0 armhf 1.0.8-5.1 [31.1 kB] 94s Get:26 http://ftpmaster.internal/ubuntu noble/main armhf libdb5.3t64 armhf 5.3.28+dfsg2-7 [662 kB] 94s Get:27 http://ftpmaster.internal/ubuntu noble/main armhf gcc-14-base armhf 14-20240412-0ubuntu1 [47.6 kB] 94s Get:28 http://ftpmaster.internal/ubuntu noble/main armhf libgcc-s1 armhf 14-20240412-0ubuntu1 [41.5 kB] 94s Get:29 http://ftpmaster.internal/ubuntu noble/main armhf libstdc++6 armhf 14-20240412-0ubuntu1 [714 kB] 94s Get:30 http://ftpmaster.internal/ubuntu noble/main armhf libffi8 armhf 3.4.6-1build1 [21.2 kB] 94s Get:31 http://ftpmaster.internal/ubuntu noble/main armhf libncurses6 armhf 6.4+20240113-1ubuntu2 [88.1 kB] 94s Get:32 http://ftpmaster.internal/ubuntu noble/main armhf libncursesw6 armhf 6.4+20240113-1ubuntu2 [119 kB] 94s Get:33 http://ftpmaster.internal/ubuntu noble/main armhf libtinfo6 armhf 6.4+20240113-1ubuntu2 [90.8 kB] 94s Get:34 http://ftpmaster.internal/ubuntu noble/main armhf libpython3.12-stdlib armhf 3.12.3-1 [1925 kB] 94s Get:35 http://ftpmaster.internal/ubuntu noble/main armhf python3.12-minimal armhf 3.12.3-1 [2023 kB] 95s Get:36 http://ftpmaster.internal/ubuntu noble/main armhf libpython3.12-minimal armhf 3.12.3-1 [817 kB] 95s Get:37 http://ftpmaster.internal/ubuntu noble/main armhf python3-minimal armhf 3.12.3-0ubuntu1 [27.2 kB] 95s Get:38 http://ftpmaster.internal/ubuntu noble/main armhf python3 armhf 3.12.3-0ubuntu1 [24.1 kB] 95s Get:39 http://ftpmaster.internal/ubuntu noble/main armhf libpython3-stdlib armhf 3.12.3-0ubuntu1 [9896 B] 95s Get:40 http://ftpmaster.internal/ubuntu noble/main armhf libacl1 armhf 2.3.2-1build1 [15.1 kB] 95s Get:41 http://ftpmaster.internal/ubuntu noble/main armhf liblz4-1 armhf 1.9.4-1build1 [58.0 kB] 95s Get:42 http://ftpmaster.internal/ubuntu noble/main armhf libpopt0 armhf 1.19+dfsg-1build1 [25.0 kB] 95s Get:43 http://ftpmaster.internal/ubuntu noble/main armhf libxxhash0 armhf 0.8.2-2build1 [31.5 kB] 95s Get:44 http://ftpmaster.internal/ubuntu noble/main armhf libzstd1 armhf 1.5.5+dfsg2-2build1 [265 kB] 95s Get:45 http://ftpmaster.internal/ubuntu noble/main armhf rsync armhf 3.2.7-1ubuntu1 [413 kB] 95s Get:46 http://ftpmaster.internal/ubuntu noble/main armhf python-apt-common all 2.7.7ubuntu1 [20.1 kB] 95s Get:47 http://ftpmaster.internal/ubuntu noble/main armhf python3-apt armhf 2.7.7ubuntu1 [162 kB] 95s Get:48 http://ftpmaster.internal/ubuntu noble/main armhf python3-problem-report all 2.28.1-0ubuntu1 [23.8 kB] 95s Get:49 http://ftpmaster.internal/ubuntu noble/main armhf python3-apport all 2.28.1-0ubuntu1 [92.1 kB] 95s Get:50 http://ftpmaster.internal/ubuntu noble/main armhf apport-core-dump-handler all 2.28.1-0ubuntu1 [16.8 kB] 95s Get:51 http://ftpmaster.internal/ubuntu noble/main armhf apport all 2.28.1-0ubuntu1 [83.5 kB] 95s Get:52 http://ftpmaster.internal/ubuntu noble/main armhf passwd armhf 1:4.13+dfsg1-4ubuntu3 [817 kB] 95s Get:53 http://ftpmaster.internal/ubuntu noble/main armhf libedit2 armhf 3.1-20230828-1build1 [78.7 kB] 95s Get:54 http://ftpmaster.internal/ubuntu noble/main armhf libfido2-1 armhf 1.14.0-1build3 [75.8 kB] 95s Get:55 http://ftpmaster.internal/ubuntu noble/main armhf openssh-sftp-server armhf 1:9.6p1-3ubuntu13 [35.5 kB] 95s Get:56 http://ftpmaster.internal/ubuntu noble/main armhf openssh-server armhf 1:9.6p1-3ubuntu13 [504 kB] 95s Get:57 http://ftpmaster.internal/ubuntu noble/main armhf openssh-client armhf 1:9.6p1-3ubuntu13 [890 kB] 95s Get:58 http://ftpmaster.internal/ubuntu noble/main armhf libpam-runtime all 1.5.3-5ubuntu5 [40.8 kB] 95s Get:59 http://ftpmaster.internal/ubuntu noble/main armhf libcom-err2 armhf 1.47.0-2.4~exp1ubuntu4 [21.9 kB] 95s Get:60 http://ftpmaster.internal/ubuntu noble/main armhf libattr1 armhf 1:2.5.2-1build1 [10.2 kB] 95s Get:61 http://ftpmaster.internal/ubuntu noble/main armhf libcap2 armhf 1:2.66-5ubuntu2 [25.8 kB] 95s Get:62 http://ftpmaster.internal/ubuntu noble/main armhf libgpg-error-l10n all 1.47-3build2 [8064 B] 95s Get:63 http://ftpmaster.internal/ubuntu noble/main armhf libgpg-error0 armhf 1.47-3build2 [61.6 kB] 95s Get:64 http://ftpmaster.internal/ubuntu noble/main armhf libgcrypt20 armhf 1.10.3-2build1 [454 kB] 95s Get:65 http://ftpmaster.internal/ubuntu noble/main armhf libgmp10 armhf 2:6.3.0+dfsg-2ubuntu6 [207 kB] 95s Get:66 http://ftpmaster.internal/ubuntu noble/main armhf libmd0 armhf 1.1.0-2build1 [23.0 kB] 95s Get:67 http://ftpmaster.internal/ubuntu noble/main armhf libpcre2-8-0 armhf 10.42-4ubuntu2 [198 kB] 95s Get:68 http://ftpmaster.internal/ubuntu noble/main armhf libsepol2 armhf 3.5-2build1 [263 kB] 95s Get:69 http://ftpmaster.internal/ubuntu noble/main armhf libunistring5 armhf 1.1-2build1 [513 kB] 95s Get:70 http://ftpmaster.internal/ubuntu noble/main armhf libidn2-0 armhf 2.3.7-2build1 [96.2 kB] 95s Get:71 http://ftpmaster.internal/ubuntu noble/main armhf libp11-kit0 armhf 0.25.3-4ubuntu2 [258 kB] 95s Get:72 http://ftpmaster.internal/ubuntu noble/main armhf libtasn1-6 armhf 4.19.0-3build1 [37.2 kB] 95s Get:73 http://ftpmaster.internal/ubuntu noble/main armhf libassuan0 armhf 2.5.6-1build1 [31.3 kB] 95s Get:74 http://ftpmaster.internal/ubuntu noble/main armhf libss2 armhf 1.47.0-2.4~exp1ubuntu4 [14.7 kB] 95s Get:75 http://ftpmaster.internal/ubuntu noble/main armhf mawk armhf 1.3.4.20240123-1build1 [115 kB] 95s Get:76 http://ftpmaster.internal/ubuntu noble/main armhf dbus-system-bus-common all 1.14.10-4ubuntu4 [81.6 kB] 95s Get:77 http://ftpmaster.internal/ubuntu noble/main armhf dbus-session-bus-common all 1.14.10-4ubuntu4 [80.4 kB] 95s Get:78 http://ftpmaster.internal/ubuntu noble/main armhf dbus-user-session armhf 1.14.10-4ubuntu4 [9960 B] 95s Get:79 http://ftpmaster.internal/ubuntu noble/main armhf dbus-daemon armhf 1.14.10-4ubuntu4 [109 kB] 95s Get:80 http://ftpmaster.internal/ubuntu noble/main armhf dbus-bin armhf 1.14.10-4ubuntu4 [37.1 kB] 95s Get:81 http://ftpmaster.internal/ubuntu noble/main armhf dbus armhf 1.14.10-4ubuntu4 [28.1 kB] 95s Get:82 http://ftpmaster.internal/ubuntu noble/main armhf libdbus-1-3 armhf 1.14.10-4ubuntu4 [190 kB] 95s Get:83 http://ftpmaster.internal/ubuntu noble/main armhf libpam-cap armhf 1:2.66-5ubuntu2 [11.6 kB] 95s Get:84 http://ftpmaster.internal/ubuntu noble/main armhf libcap2-bin armhf 1:2.66-5ubuntu2 [32.3 kB] 95s Get:85 http://ftpmaster.internal/ubuntu noble/main armhf iputils-ping armhf 3:20240117-1build1 [43.1 kB] 95s Get:86 http://ftpmaster.internal/ubuntu noble/main armhf kmod armhf 31+20240202-2ubuntu6 [91.8 kB] 95s Get:87 http://ftpmaster.internal/ubuntu noble/main armhf libkmod2 armhf 31+20240202-2ubuntu6 [45.0 kB] 95s Get:88 http://ftpmaster.internal/ubuntu noble/main armhf libargon2-1 armhf 0~20190702+dfsg-4build1 [22.6 kB] 95s Get:89 http://ftpmaster.internal/ubuntu noble/main armhf libjson-c5 armhf 0.17-1build1 [31.3 kB] 95s Get:90 http://ftpmaster.internal/ubuntu noble/main armhf libcryptsetup12 armhf 2:2.7.0-1ubuntu4 [238 kB] 95s Get:91 http://ftpmaster.internal/ubuntu noble/main armhf libestr0 armhf 0.1.11-1build1 [6770 B] 95s Get:92 http://ftpmaster.internal/ubuntu noble/main armhf libfastjson4 armhf 1.2304.0-1build1 [20.1 kB] 95s Get:93 http://ftpmaster.internal/ubuntu noble/main armhf libfribidi0 armhf 1.0.13-3build1 [23.9 kB] 95s Get:94 http://ftpmaster.internal/ubuntu noble/main armhf libicu74 armhf 74.2-1ubuntu3 [10.5 MB] 96s Get:95 http://ftpmaster.internal/ubuntu noble/main armhf libkeyutils1 armhf 1.6.3-3build1 [8236 B] 96s Get:96 http://ftpmaster.internal/ubuntu noble/main armhf libmnl0 armhf 1.0.5-2build1 [10.5 kB] 96s Get:97 http://ftpmaster.internal/ubuntu noble/main armhf iptables armhf 1.8.10-3ubuntu2 [338 kB] 96s Get:98 http://ftpmaster.internal/ubuntu noble/main armhf libip4tc2 armhf 1.8.10-3ubuntu2 [21.3 kB] 96s Get:99 http://ftpmaster.internal/ubuntu noble/main armhf libip6tc2 armhf 1.8.10-3ubuntu2 [21.7 kB] 96s Get:100 http://ftpmaster.internal/ubuntu noble/main armhf libnfnetlink0 armhf 1.0.2-2build1 [12.9 kB] 96s Get:101 http://ftpmaster.internal/ubuntu noble/main armhf libnetfilter-conntrack3 armhf 1.0.9-6build1 [37.5 kB] 96s Get:102 http://ftpmaster.internal/ubuntu noble/main armhf libnftnl11 armhf 1.2.6-2build1 [52.5 kB] 96s Get:103 http://ftpmaster.internal/ubuntu noble/main armhf libxtables12 armhf 1.8.10-3ubuntu2 [32.4 kB] 96s Get:104 http://ftpmaster.internal/ubuntu noble/main armhf libyaml-0-2 armhf 0.2.5-1build1 [45.2 kB] 96s Get:105 http://ftpmaster.internal/ubuntu noble/main armhf logrotate armhf 3.21.0-2build1 [50.3 kB] 96s Get:106 http://ftpmaster.internal/ubuntu noble/main armhf netcat-openbsd armhf 1.226-1ubuntu2 [42.8 kB] 96s Get:107 http://ftpmaster.internal/ubuntu noble/main armhf python3-cffi-backend armhf 1.16.0-2build1 [68.0 kB] 96s Get:108 http://ftpmaster.internal/ubuntu noble/main armhf python3-netifaces armhf 0.11.0-2build3 [17.2 kB] 96s Get:109 http://ftpmaster.internal/ubuntu noble/main armhf rsyslog armhf 8.2312.0-3ubuntu9 [460 kB] 97s Get:110 http://ftpmaster.internal/ubuntu noble/main armhf sudo armhf 1.9.15p5-3ubuntu5 [936 kB] 97s Get:111 http://ftpmaster.internal/ubuntu noble/main armhf xdg-user-dirs armhf 0.18-1build1 [17.3 kB] 97s Get:112 http://ftpmaster.internal/ubuntu noble/main armhf xkb-data all 2.41-2ubuntu1 [395 kB] 97s Get:113 http://ftpmaster.internal/ubuntu noble/main armhf liblmdb0 armhf 0.9.31-1build1 [39.9 kB] 97s Get:114 http://ftpmaster.internal/ubuntu noble/main armhf libmaxminddb0 armhf 1.9.1-1build1 [23.2 kB] 97s Get:115 http://ftpmaster.internal/ubuntu noble/main armhf libnghttp2-14 armhf 1.59.0-1build4 [68.2 kB] 97s Get:116 http://ftpmaster.internal/ubuntu noble/main armhf bind9-dnsutils armhf 1:9.18.24-0ubuntu5 [149 kB] 97s Get:117 http://ftpmaster.internal/ubuntu noble/main armhf bind9-host armhf 1:9.18.24-0ubuntu5 [47.4 kB] 97s Get:118 http://ftpmaster.internal/ubuntu noble/main armhf bind9-libs armhf 1:9.18.24-0ubuntu5 [1148 kB] 97s Get:119 http://ftpmaster.internal/ubuntu noble/main armhf cpio armhf 2.15+dfsg-1ubuntu2 [81.8 kB] 97s Get:120 http://ftpmaster.internal/ubuntu noble/main armhf dmidecode armhf 3.5-3build1 [58.6 kB] 97s Get:121 http://ftpmaster.internal/ubuntu noble/main armhf tnftp armhf 20230507-2build3 [98.7 kB] 97s Get:122 http://ftpmaster.internal/ubuntu noble/main armhf ftp all 20230507-2build3 [4728 B] 97s Get:123 http://ftpmaster.internal/ubuntu noble/main armhf gettext-base armhf 0.21-14ubuntu2 [38.1 kB] 97s Get:124 http://ftpmaster.internal/ubuntu noble/main armhf hdparm armhf 9.65+ds-1build1 [96.7 kB] 97s Get:125 http://ftpmaster.internal/ubuntu noble/main armhf iputils-tracepath armhf 3:20240117-1build1 [12.8 kB] 97s Get:126 http://ftpmaster.internal/ubuntu noble/main armhf libdrm-common all 2.4.120-2build1 [8096 B] 97s Get:127 http://ftpmaster.internal/ubuntu noble/main armhf libdrm2 armhf 2.4.120-2build1 [36.6 kB] 97s Get:128 http://ftpmaster.internal/ubuntu noble/main armhf nftables armhf 1.0.9-1build1 [69.5 kB] 97s Get:129 http://ftpmaster.internal/ubuntu noble/main armhf libnftables1 armhf 1.0.9-1build1 [309 kB] 97s Get:130 http://ftpmaster.internal/ubuntu noble/main armhf libnuma1 armhf 2.0.18-1build1 [19.8 kB] 97s Get:131 http://ftpmaster.internal/ubuntu noble/main armhf pci.ids all 0.0~2024.03.31-1 [275 kB] 97s Get:132 http://ftpmaster.internal/ubuntu noble/main armhf pciutils armhf 1:3.10.0-2build1 [64.4 kB] 97s Get:133 http://ftpmaster.internal/ubuntu noble/main armhf libpci3 armhf 1:3.10.0-2build1 [29.5 kB] 97s Get:134 http://ftpmaster.internal/ubuntu noble/main armhf libuchardet0 armhf 0.0.8-1build1 [73.9 kB] 97s Get:135 http://ftpmaster.internal/ubuntu noble/main armhf libx11-data all 2:1.8.7-1build1 [115 kB] 97s Get:136 http://ftpmaster.internal/ubuntu noble/main armhf libx11-6 armhf 2:1.8.7-1build1 [583 kB] 97s Get:137 http://ftpmaster.internal/ubuntu noble/main armhf libxau6 armhf 1:1.0.9-1build6 [6312 B] 97s Get:138 http://ftpmaster.internal/ubuntu noble/main armhf libxdmcp6 armhf 1:1.1.3-0ubuntu6 [8738 B] 97s Get:139 http://ftpmaster.internal/ubuntu noble/main armhf libxext6 armhf 2:1.3.4-1build2 [25.3 kB] 97s Get:140 http://ftpmaster.internal/ubuntu noble/main armhf man-db armhf 2.12.0-4build2 [1202 kB] 97s Get:141 http://ftpmaster.internal/ubuntu noble/main armhf nano armhf 7.2-2build1 [269 kB] 97s Get:142 http://ftpmaster.internal/ubuntu noble/main armhf python3-gdbm armhf 3.12.3-0ubuntu1 [15.2 kB] 97s Get:143 http://ftpmaster.internal/ubuntu noble/main armhf tcpdump armhf 4.99.4-3ubuntu4 [425 kB] 97s Get:144 http://ftpmaster.internal/ubuntu noble/main armhf time armhf 1.9-0.2build1 [45.8 kB] 97s Get:145 http://ftpmaster.internal/ubuntu noble/main armhf ufw all 0.36.2-6 [169 kB] 97s Get:146 http://ftpmaster.internal/ubuntu noble/main armhf usb.ids all 2024.03.18-1 [223 kB] 97s Get:147 http://ftpmaster.internal/ubuntu noble/main armhf usbutils armhf 1:017-3build1 [75.6 kB] 97s Get:148 http://ftpmaster.internal/ubuntu noble/main armhf xauth armhf 1:1.1.2-1build1 [22.7 kB] 97s Get:149 http://ftpmaster.internal/ubuntu noble/main armhf apport-symptoms all 0.25 [13.1 kB] 97s Get:150 http://ftpmaster.internal/ubuntu noble/main armhf bcache-tools armhf 1.0.8-5build1 [20.2 kB] 97s Get:151 http://ftpmaster.internal/ubuntu noble/main armhf cryptsetup-bin armhf 2:2.7.0-1ubuntu4 [214 kB] 97s Get:152 http://ftpmaster.internal/ubuntu noble/main armhf dracut-install armhf 060+5-1ubuntu3 [34.1 kB] 97s Get:153 http://ftpmaster.internal/ubuntu noble/main armhf libeatmydata1 armhf 131-1ubuntu1 [7188 B] 97s Get:154 http://ftpmaster.internal/ubuntu noble/main armhf eatmydata all 131-1ubuntu1 [5584 B] 97s Get:155 http://ftpmaster.internal/ubuntu noble/main armhf ethtool armhf 1:6.7-1build1 [218 kB] 97s Get:156 http://ftpmaster.internal/ubuntu noble/main armhf gcc-13-base armhf 13.2.0-23ubuntu4 [48.9 kB] 97s Get:157 http://ftpmaster.internal/ubuntu noble/main armhf libnl-genl-3-200 armhf 3.7.0-0.3build1 [10.3 kB] 97s Get:158 http://ftpmaster.internal/ubuntu noble/main armhf libnl-route-3-200 armhf 3.7.0-0.3build1 [162 kB] 97s Get:159 http://ftpmaster.internal/ubuntu noble/main armhf libnl-3-200 armhf 3.7.0-0.3build1 [49.0 kB] 97s Get:160 http://ftpmaster.internal/ubuntu noble/main armhf htop armhf 3.3.0-4build1 [139 kB] 97s Get:161 http://ftpmaster.internal/ubuntu noble/main armhf libatasmart4 armhf 0.19-5build3 [24.0 kB] 97s Get:162 http://ftpmaster.internal/ubuntu noble/main armhf libmpfr6 armhf 4.2.1-1build1 [229 kB] 97s Get:163 http://ftpmaster.internal/ubuntu noble/main armhf libbytesize1 armhf 2.10-1ubuntu2 [11.7 kB] 97s Get:164 http://ftpmaster.internal/ubuntu noble/main armhf libbytesize-common all 2.10-1ubuntu2 [3396 B] 97s Get:165 http://ftpmaster.internal/ubuntu noble/main armhf libflashrom1 armhf 1.3.0-2.1ubuntu2 [138 kB] 97s Get:166 http://ftpmaster.internal/ubuntu noble/main armhf libinih1 armhf 55-1ubuntu2 [6506 B] 97s Get:167 http://ftpmaster.internal/ubuntu noble/main armhf liblzo2-2 armhf 2.10-2build4 [46.1 kB] 97s Get:168 http://ftpmaster.internal/ubuntu noble/main armhf libnspr4 armhf 2:4.35-1.1build1 [93.0 kB] 97s Get:169 http://ftpmaster.internal/ubuntu noble/main armhf libnss3 armhf 2:3.98-1build1 [1288 kB] 98s Get:170 http://ftpmaster.internal/ubuntu noble/main armhf libonig5 armhf 6.9.9-1build1 [148 kB] 98s Get:171 http://ftpmaster.internal/ubuntu noble/main armhf libsgutils2-1.46-2 armhf 1.46-3ubuntu4 [82.7 kB] 98s Get:172 http://ftpmaster.internal/ubuntu noble/main armhf libsigsegv2 armhf 2.14-1ubuntu2 [14.2 kB] 98s Get:173 http://ftpmaster.internal/ubuntu noble/main armhf libutempter0 armhf 1.2.1-3build1 [8862 B] 98s Get:174 http://ftpmaster.internal/ubuntu noble/main armhf libxkbcommon0 armhf 1.6.0-1build1 [108 kB] 98s Get:175 http://ftpmaster.internal/ubuntu noble/main armhf libxmlb2 armhf 0.3.18-1 [56.9 kB] 98s Get:176 http://ftpmaster.internal/ubuntu noble/main armhf make armhf 4.3-4.1build2 [162 kB] 98s Get:177 http://ftpmaster.internal/ubuntu noble/main armhf numactl armhf 2.0.18-1build1 [38.2 kB] 98s Get:178 http://ftpmaster.internal/ubuntu noble/main armhf patch armhf 2.7.6-7build3 [110 kB] 98s Get:179 http://ftpmaster.internal/ubuntu noble/main armhf python3-systemd armhf 235-1build4 [39.7 kB] 98s Get:180 http://ftpmaster.internal/ubuntu noble/main armhf screen armhf 4.9.1-1build1 [638 kB] 98s Get:181 http://ftpmaster.internal/ubuntu noble/main armhf sg3-utils armhf 1.46-3ubuntu4 [816 kB] 98s Get:182 http://ftpmaster.internal/ubuntu noble/main armhf sg3-utils-udev all 1.46-3ubuntu4 [5922 B] 98s Get:183 http://ftpmaster.internal/ubuntu noble/main armhf sysstat armhf 12.6.1-2 [479 kB] 98s Get:184 http://ftpmaster.internal/ubuntu noble/main armhf zstd armhf 1.5.5+dfsg2-2build1 [683 kB] 98s Get:185 http://ftpmaster.internal/ubuntu noble/main armhf cloud-init all 24.1.3-0ubuntu3 [598 kB] 98s Get:186 http://ftpmaster.internal/ubuntu noble/main armhf libevdev2 armhf 1.13.1+dfsg-1build1 [29.8 kB] 99s Preconfiguring packages ... 99s Fetched 43.7 MB in 5s (8445 kB/s) 99s (Reading database ... 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(Reading database ... 5% (Reading database ... 10% (Reading database ... 15% (Reading database ... 20% (Reading database ... 25% (Reading database ... 30% (Reading database ... 35% (Reading database ... 40% (Reading database ... 45% (Reading database ... 50% (Reading database ... 55% (Reading database ... 60% (Reading database ... 65% (Reading database ... 70% (Reading database ... 75% (Reading database ... 80% (Reading database ... 85% (Reading database ... 90% (Reading database ... 95% (Reading database ... 100% (Reading database ... 58471 files and directories currently installed.) 100s Preparing to unpack .../ncurses-bin_6.4+20240113-1ubuntu2_armhf.deb ... 100s Unpacking ncurses-bin (6.4+20240113-1ubuntu2) over (6.4+20240113-1ubuntu1) ... 100s Setting up ncurses-bin (6.4+20240113-1ubuntu2) ... 100s (Reading database ... (Reading database ... 5% (Reading database ... 10% (Reading database ... 15% (Reading database ... 20% (Reading database ... 25% (Reading database ... 30% (Reading database ... 35% (Reading database ... 40% (Reading database ... 45% (Reading database ... 50% (Reading database ... 55% (Reading database ... 60% (Reading database ... 65% (Reading database ... 70% (Reading database ... 75% (Reading database ... 80% (Reading database ... 85% (Reading database ... 90% (Reading database ... 95% (Reading database ... 100% (Reading database ... 58471 files and directories currently installed.) 100s Preparing to unpack .../sed_4.9-2build1_armhf.deb ... 100s Unpacking sed (4.9-2build1) over (4.9-2) ... 100s Setting up sed (4.9-2build1) ... 100s (Reading database ... (Reading database ... 5% (Reading database ... 10% (Reading database ... 15% (Reading database ... 20% (Reading database ... 25% (Reading database ... 30% (Reading database ... 35% (Reading database ... 40% (Reading database ... 45% (Reading database ... 50% (Reading database ... 55% (Reading database ... 60% (Reading database ... 65% (Reading database ... 70% (Reading database ... 75% (Reading database ... 80% (Reading database ... 85% (Reading database ... 90% (Reading database ... 95% (Reading database ... 100% (Reading database ... 58471 files and directories currently installed.) 100s Preparing to unpack .../tar_1.35+dfsg-3build1_armhf.deb ... 100s Unpacking tar (1.35+dfsg-3build1) over (1.35+dfsg-3) ... 100s Setting up tar (1.35+dfsg-3build1) ... 100s (Reading database ... (Reading database ... 5% (Reading database ... 10% (Reading database ... 15% (Reading database ... 20% (Reading database ... 25% (Reading database ... 30% (Reading database ... 35% (Reading database ... 40% (Reading database ... 45% (Reading database ... 50% (Reading database ... 55% (Reading database ... 60% (Reading database ... 65% (Reading database ... 70% (Reading database ... 75% (Reading database ... 80% (Reading database ... 85% (Reading database ... 90% (Reading database ... 95% (Reading database ... 100% (Reading database ... 58471 files and directories currently installed.) 100s Preparing to unpack .../base-passwd_3.6.3build1_armhf.deb ... 100s Unpacking base-passwd (3.6.3build1) over (3.6.3) ... 100s Setting up base-passwd (3.6.3build1) ... 100s (Reading database ... (Reading database ... 5% (Reading database ... 10% (Reading database ... 15% (Reading database ... 20% (Reading database ... 25% (Reading database ... 30% (Reading database ... 35% (Reading database ... 40% (Reading database ... 45% (Reading database ... 50% (Reading database ... 55% (Reading database ... 60% (Reading database ... 65% (Reading database ... 70% (Reading database ... 75% (Reading database ... 80% (Reading database ... 85% (Reading database ... 90% (Reading database ... 95% (Reading database ... 100% (Reading database ... 58471 files and directories currently installed.) 100s Preparing to unpack .../ncurses-base_6.4+20240113-1ubuntu2_all.deb ... 100s Unpacking ncurses-base (6.4+20240113-1ubuntu2) over (6.4+20240113-1ubuntu1) ... 100s Setting up ncurses-base (6.4+20240113-1ubuntu2) ... 100s (Reading database ... (Reading database ... 5% (Reading database ... 10% (Reading database ... 15% (Reading database ... 20% (Reading database ... 25% (Reading database ... 30% (Reading database ... 35% (Reading database ... 40% (Reading database ... 45% (Reading database ... 50% (Reading database ... 55% (Reading database ... 60% (Reading database ... 65% (Reading database ... 70% (Reading database ... 75% (Reading database ... 80% (Reading database ... 85% (Reading database ... 90% (Reading database ... 95% (Reading database ... 100% (Reading database ... 58471 files and directories currently installed.) 100s Preparing to unpack .../ncurses-term_6.4+20240113-1ubuntu2_all.deb ... 100s Unpacking ncurses-term (6.4+20240113-1ubuntu2) over (6.4+20240113-1ubuntu1) ... 101s Preparing to unpack .../sysvinit-utils_3.08-6ubuntu3_armhf.deb ... 101s Unpacking sysvinit-utils (3.08-6ubuntu3) over (3.08-6ubuntu2) ... 101s Setting up sysvinit-utils (3.08-6ubuntu3) ... 101s (Reading database ... (Reading database ... 5% (Reading database ... 10% (Reading database ... 15% (Reading database ... 20% (Reading database ... 25% (Reading database ... 30% (Reading database ... 35% (Reading database ... 40% (Reading database ... 45% (Reading database ... 50% (Reading database ... 55% (Reading database ... 60% (Reading database ... 65% (Reading database ... 70% (Reading database ... 75% (Reading database ... 80% (Reading database ... 85% (Reading database ... 90% (Reading database ... 95% (Reading database ... 100% (Reading database ... 58471 files and directories currently installed.) 101s Preparing to unpack .../libcrypt1_1%3a4.4.36-4build1_armhf.deb ... 101s Unpacking libcrypt1:armhf (1:4.4.36-4build1) over (1:4.4.36-4) ... 101s Setting up libcrypt1:armhf (1:4.4.36-4build1) ... 101s (Reading database ... (Reading database ... 5% (Reading database ... 10% (Reading database ... 15% (Reading database ... 20% (Reading database ... 25% (Reading database ... 30% (Reading database ... 35% (Reading database ... 40% (Reading database ... 45% (Reading database ... 50% (Reading database ... 55% (Reading database ... 60% (Reading database ... 65% (Reading database ... 70% (Reading database ... 75% (Reading database ... 80% (Reading database ... 85% (Reading database ... 90% (Reading database ... 95% (Reading database ... 100% (Reading database ... 58471 files and directories currently installed.) 101s Preparing to unpack .../libpam0g_1.5.3-5ubuntu5_armhf.deb ... 101s Unpacking libpam0g:armhf (1.5.3-5ubuntu5) over (1.5.3-5ubuntu4) ... 101s Setting up libpam0g:armhf (1.5.3-5ubuntu5) ... 101s (Reading database ... (Reading database ... 5% (Reading database ... 10% (Reading database ... 15% (Reading database ... 20% (Reading database ... 25% (Reading database ... 30% (Reading database ... 35% (Reading database ... 40% (Reading database ... 45% (Reading database ... 50% (Reading database ... 55% (Reading database ... 60% (Reading database ... 65% (Reading database ... 70% (Reading database ... 75% (Reading database ... 80% (Reading database ... 85% (Reading database ... 90% (Reading database ... 95% (Reading database ... 100% (Reading database ... 58471 files and directories currently installed.) 101s Preparing to unpack .../libpam-modules-bin_1.5.3-5ubuntu5_armhf.deb ... 101s Unpacking libpam-modules-bin (1.5.3-5ubuntu5) over (1.5.3-5ubuntu4) ... 101s Setting up libpam-modules-bin (1.5.3-5ubuntu5) ... 102s pam_namespace.service is a disabled or a static unit not running, not starting it. 102s (Reading database ... (Reading database ... 5% (Reading database ... 10% (Reading database ... 15% (Reading database ... 20% (Reading database ... 25% (Reading database ... 30% (Reading database ... 35% (Reading database ... 40% (Reading database ... 45% (Reading database ... 50% (Reading database ... 55% (Reading database ... 60% (Reading database ... 65% (Reading database ... 70% (Reading database ... 75% (Reading database ... 80% (Reading database ... 85% (Reading database ... 90% (Reading database ... 95% (Reading database ... 100% (Reading database ... 58471 files and directories currently installed.) 102s Preparing to unpack .../libpam-modules_1.5.3-5ubuntu5_armhf.deb ... 102s Unpacking libpam-modules:armhf (1.5.3-5ubuntu5) over (1.5.3-5ubuntu4) ... 102s Setting up libpam-modules:armhf (1.5.3-5ubuntu5) ... 102s (Reading database ... (Reading database ... 5% (Reading database ... 10% (Reading database ... 15% (Reading database ... 20% (Reading database ... 25% (Reading database ... 30% (Reading database ... 35% (Reading database ... 40% (Reading database ... 45% (Reading database ... 50% (Reading database ... 55% (Reading database ... 60% (Reading database ... 65% (Reading database ... 70% (Reading database ... 75% (Reading database ... 80% (Reading database ... 85% (Reading database ... 90% (Reading database ... 95% (Reading database ... 100% (Reading database ... 58471 files and directories currently installed.) 102s Preparing to unpack .../e2fsprogs-l10n_1.47.0-2.4~exp1ubuntu4_all.deb ... 102s Unpacking e2fsprogs-l10n (1.47.0-2.4~exp1ubuntu4) over (1.47.0-2.4~exp1ubuntu3) ... 102s Preparing to unpack .../logsave_1.47.0-2.4~exp1ubuntu4_armhf.deb ... 102s Unpacking logsave (1.47.0-2.4~exp1ubuntu4) over (1.47.0-2.4~exp1ubuntu3) ... 102s Preparing to unpack .../libext2fs2t64_1.47.0-2.4~exp1ubuntu4_armhf.deb ... 102s Leaving 'diversion of /lib/arm-linux-gnueabihf/libe2p.so.2 to /lib/arm-linux-gnueabihf/libe2p.so.2.usr-is-merged by libext2fs2t64' 102s Leaving 'diversion of /lib/arm-linux-gnueabihf/libe2p.so.2.3 to /lib/arm-linux-gnueabihf/libe2p.so.2.3.usr-is-merged by libext2fs2t64' 102s Leaving 'diversion of /lib/arm-linux-gnueabihf/libext2fs.so.2 to /lib/arm-linux-gnueabihf/libext2fs.so.2.usr-is-merged by libext2fs2t64' 102s Leaving 'diversion of /lib/arm-linux-gnueabihf/libext2fs.so.2.4 to /lib/arm-linux-gnueabihf/libext2fs.so.2.4.usr-is-merged by libext2fs2t64' 102s Unpacking libext2fs2t64:armhf (1.47.0-2.4~exp1ubuntu4) over (1.47.0-2.4~exp1ubuntu3) ... 102s Setting up libext2fs2t64:armhf (1.47.0-2.4~exp1ubuntu4) ... 102s (Reading database ... (Reading database ... 5% (Reading database ... 10% (Reading database ... 15% (Reading database ... 20% (Reading database ... 25% (Reading database ... 30% (Reading database ... 35% (Reading database ... 40% (Reading database ... 45% (Reading database ... 50% (Reading database ... 55% (Reading database ... 60% (Reading database ... 65% (Reading database ... 70% (Reading database ... 75% (Reading database ... 80% (Reading database ... 85% (Reading database ... 90% (Reading database ... 95% (Reading database ... 100% (Reading database ... 58471 files and directories currently installed.) 102s Preparing to unpack .../e2fsprogs_1.47.0-2.4~exp1ubuntu4_armhf.deb ... 102s Unpacking e2fsprogs (1.47.0-2.4~exp1ubuntu4) over (1.47.0-2.4~exp1ubuntu3) ... 102s Preparing to unpack .../tzdata_2024a-2ubuntu1_all.deb ... 102s Unpacking tzdata (2024a-2ubuntu1) over (2024a-1ubuntu1) ... 102s Preparing to unpack .../python3.12_3.12.3-1_armhf.deb ... 102s Unpacking python3.12 (3.12.3-1) over (3.12.2-5ubuntu3) ... 102s Preparing to unpack .../bzip2_1.0.8-5.1_armhf.deb ... 102s Unpacking bzip2 (1.0.8-5.1) over (1.0.8-5ubuntu1) ... 102s Preparing to unpack .../libbz2-1.0_1.0.8-5.1_armhf.deb ... 102s Unpacking libbz2-1.0:armhf (1.0.8-5.1) over (1.0.8-5ubuntu1) ... 102s Setting up libbz2-1.0:armhf (1.0.8-5.1) ... 103s (Reading database ... (Reading database ... 5% (Reading database ... 10% (Reading database ... 15% (Reading database ... 20% (Reading database ... 25% (Reading database ... 30% (Reading database ... 35% (Reading database ... 40% (Reading database ... 45% (Reading database ... 50% (Reading database ... 55% (Reading database ... 60% (Reading database ... 65% (Reading database ... 70% (Reading database ... 75% (Reading database ... 80% (Reading database ... 85% (Reading database ... 90% (Reading database ... 95% (Reading database ... 100% (Reading database ... 58470 files and directories currently installed.) 103s Preparing to unpack .../libdb5.3t64_5.3.28+dfsg2-7_armhf.deb ... 103s Unpacking libdb5.3t64:armhf (5.3.28+dfsg2-7) over (5.3.28+dfsg2-6build1) ... 103s Preparing to unpack .../gcc-14-base_14-20240412-0ubuntu1_armhf.deb ... 103s Unpacking gcc-14-base:armhf (14-20240412-0ubuntu1) over (14-20240330-1ubuntu2) ... 103s Setting up gcc-14-base:armhf (14-20240412-0ubuntu1) ... 103s (Reading database ... (Reading database ... 5% (Reading database ... 10% (Reading database ... 15% (Reading database ... 20% (Reading database ... 25% (Reading database ... 30% (Reading database ... 35% (Reading database ... 40% (Reading database ... 45% (Reading database ... 50% (Reading database ... 55% (Reading database ... 60% (Reading database ... 65% (Reading database ... 70% (Reading database ... 75% (Reading database ... 80% (Reading database ... 85% (Reading database ... 90% (Reading database ... 95% (Reading database ... 100% (Reading database ... 58470 files and directories currently installed.) 103s Preparing to unpack .../libgcc-s1_14-20240412-0ubuntu1_armhf.deb ... 103s Unpacking libgcc-s1:armhf (14-20240412-0ubuntu1) over (14-20240330-1ubuntu2) ... 103s Setting up libgcc-s1:armhf (14-20240412-0ubuntu1) ... 103s (Reading database ... (Reading database ... 5% (Reading database ... 10% (Reading database ... 15% (Reading database ... 20% (Reading database ... 25% (Reading database ... 30% (Reading database ... 35% (Reading database ... 40% (Reading database ... 45% (Reading database ... 50% (Reading database ... 55% (Reading database ... 60% (Reading database ... 65% (Reading database ... 70% (Reading database ... 75% (Reading database ... 80% (Reading database ... 85% (Reading database ... 90% (Reading database ... 95% (Reading database ... 100% (Reading database ... 58470 files and directories currently installed.) 103s Preparing to unpack .../libstdc++6_14-20240412-0ubuntu1_armhf.deb ... 103s Unpacking libstdc++6:armhf (14-20240412-0ubuntu1) over (14-20240330-1ubuntu2) ... 103s Setting up libstdc++6:armhf (14-20240412-0ubuntu1) ... 103s (Reading database ... (Reading database ... 5% (Reading database ... 10% (Reading database ... 15% (Reading database ... 20% (Reading database ... 25% (Reading database ... 30% (Reading database ... 35% (Reading database ... 40% (Reading database ... 45% (Reading database ... 50% (Reading database ... 55% (Reading database ... 60% (Reading database ... 65% (Reading database ... 70% (Reading database ... 75% (Reading database ... 80% (Reading database ... 85% (Reading database ... 90% (Reading database ... 95% (Reading database ... 100% (Reading database ... 58470 files and directories currently installed.) 103s Preparing to unpack .../libffi8_3.4.6-1build1_armhf.deb ... 103s Unpacking libffi8:armhf (3.4.6-1build1) over (3.4.6-1) ... 103s Setting up libffi8:armhf (3.4.6-1build1) ... 103s (Reading database ... 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You need policy admin privileges to manage profiles. 114s 114s Setting up libxau6:armhf (1:1.0.9-1build6) ... 114s Setting up libxdmcp6:armhf (1:1.1.3-0ubuntu6) ... 114s Setting up time (1.9-0.2build1) ... 114s Setting up libkeyutils1:armhf (1.6.3-3build1) ... 114s Setting up pci.ids (0.0~2024.03.31-1) ... 114s Setting up xdg-user-dirs (0.18-1build1) ... 114s Setting up libyaml-0-2:armhf (0.2.5-1build1) ... 114s Setting up libip6tc2:armhf (1.8.10-3ubuntu2) ... 114s Setting up libestr0:armhf (0.1.11-1build1) ... 114s Setting up libfastjson4:armhf (1.2304.0-1build1) ... 114s Setting up libinih1:armhf (55-1ubuntu2) ... 114s Setting up libmaxminddb0:armhf (1.9.1-1build1) ... 114s Setting up libargon2-1:armhf (0~20190702+dfsg-4build1) ... 114s Setting up libxmlb2:armhf (0.3.18-1) ... 114s Setting up libedit2:armhf (3.1-20230828-1build1) ... 114s Setting up rsyslog (8.2312.0-3ubuntu9) ... 114s info: The user `syslog' is already a member of `adm'. 115s apparmor_parser: Unable to replace "rsyslogd". apparmor_parser: Access denied. You need policy admin privileges to manage profiles. 115s 116s Setting up netcat-openbsd (1.226-1ubuntu2) ... 116s Setting up libnghttp2-14:armhf (1.59.0-1build4) ... 116s Setting up libsgutils2-1.46-2:armhf (1.46-3ubuntu4) ... 116s Setting up gettext-base (0.21-14ubuntu2) ... 116s Setting up xkb-data (2.41-2ubuntu1) ... 116s Setting up liblzo2-2:armhf (2.10-2build4) ... 116s Setting up hdparm (9.65+ds-1build1) ... 116s Setting up libcom-err2:armhf (1.47.0-2.4~exp1ubuntu4) ... 116s Setting up bzip2 (1.0.8-5.1) ... 116s Setting up man-db (2.12.0-4build2) ... 116s Updating database of manual pages ... 117s apparmor_parser: Unable to replace "/usr/bin/man". apparmor_parser: Access denied. You need policy admin privileges to manage profiles. 117s 118s man-db.service is a disabled or a static unit not running, not starting it. 118s Setting up apport-symptoms (0.25) ... 118s Setting up usbutils (1:017-3build1) ... 118s Setting up tzdata (2024a-2ubuntu1) ... 118s 118s Current default time zone: 'Etc/UTC' 118s Local time is now: Fri Apr 19 01:01:21 UTC 2024. 118s Universal Time is now: Fri Apr 19 01:01:21 UTC 2024. 118s Run 'dpkg-reconfigure tzdata' if you wish to change it. 118s 118s Setting up libcap2-bin (1:2.66-5ubuntu2) ... 118s Setting up gcc-13-base:armhf (13.2.0-23ubuntu4) ... 118s Setting up libatasmart4:armhf (0.19-5build3) ... 118s Setting up libx11-data (2:1.8.7-1build1) ... 118s Setting up make (4.3-4.1build2) ... 118s Setting up libmpfr6:armhf (4.2.1-1build1) ... 118s Setting up libnspr4:armhf (2:4.35-1.1build1) ... 118s Setting up libncurses6:armhf (6.4+20240113-1ubuntu2) ... 118s Setting up libdbus-1-3:armhf (1.14.10-4ubuntu4) ... 118s Setting up libsigsegv2:armhf (2.14-1ubuntu2) ... 118s Setting up libfribidi0:armhf (1.0.13-3build1) ... 118s Setting up libbytesize-common (2.10-1ubuntu2) ... 118s Setting up libmnl0:armhf (1.0.5-2build1) ... 118s Setting up patch (2.7.6-7build3) ... 118s Setting up libss2:armhf (1.47.0-2.4~exp1ubuntu4) ... 118s Setting up usb.ids (2024.03.18-1) ... 118s Setting up sudo (1.9.15p5-3ubuntu5) ... 118s Setting up libncursesw6:armhf (6.4+20240113-1ubuntu2) ... 118s Setting up libxtables12:armhf (1.8.10-3ubuntu2) ... 118s Setting up logsave (1.47.0-2.4~exp1ubuntu4) ... 118s Setting up libdb5.3t64:armhf (5.3.28+dfsg2-7) ... 118s Setting up libutempter0:armhf (1.2.1-3build1) ... 118s Setting up libicu74:armhf (74.2-1ubuntu3) ... 118s Setting up nano (7.2-2build1) ... 118s Setting up libpci3:armhf (1:3.10.0-2build1) ... 118s Setting up libnuma1:armhf (2.0.18-1build1) ... 118s Setting up python-apt-common (2.7.7ubuntu1) ... 118s Setting up libnfnetlink0:armhf (1.0.2-2build1) ... 118s Setting up dbus-session-bus-common (1.14.10-4ubuntu4) ... 118s Setting up libuchardet0:armhf (0.0.8-1build1) ... 118s Setting up libeatmydata1:armhf (131-1ubuntu1) ... 118s Setting up libnl-3-200:armhf (3.7.0-0.3build1) ... 118s Setting up libx11-6:armhf (2:1.8.7-1build1) ... 118s Setting up mawk (1.3.4.20240123-1build1) ... 118s Setting up libbytesize1:armhf (2.10-1ubuntu2) ... 118s Setting up tnftp (20230507-2build3) ... 118s Setting up dmidecode (3.5-3build1) ... 118s Setting up dbus-system-bus-common (1.14.10-4ubuntu4) ... 118s Setting up libfido2-1:armhf (1.14.0-1build3) ... 118s Setting up libgpg-error-l10n (1.47-3build2) ... 118s Setting up libdrm-common (2.4.120-2build1) ... 118s Setting up libpam-cap:armhf (1:2.66-5ubuntu2) ... 118s Setting up iputils-ping (3:20240117-1build1) ... 118s Setting up libjson-c5:armhf (0.17-1build1) ... 118s Setting up libevdev2:armhf (1.13.1+dfsg-1build1) ... 118s Setting up sysstat (12.6.1-2) ... 121s Setting up zstd (1.5.5+dfsg2-2build1) ... 121s Setting up dbus-bin (1.14.10-4ubuntu4) ... 121s Setting up libonig5:armhf (6.9.9-1build1) ... 121s Setting up iputils-tracepath (3:20240117-1build1) ... 121s Setting up libkmod2:armhf (31+20240202-2ubuntu6) ... 121s Setting up libpopt0:armhf (1.19+dfsg-1build1) ... 121s Setting up ethtool (1:6.7-1build1) ... 121s Setting up sg3-utils (1.46-3ubuntu4) ... 121s Setting up ncurses-term (6.4+20240113-1ubuntu2) ... 121s Setting up libxkbcommon0:armhf (1.6.0-1build1) ... 121s Setting up logrotate (3.21.0-2build1) ... 121s logrotate.service is a disabled or a static unit not running, not starting it. 121s Setting up eatmydata (131-1ubuntu1) ... 121s Setting up libpython3.12-stdlib:armhf (3.12.3-1) ... 121s Setting up numactl (2.0.18-1build1) ... 121s Setting up bind9-libs:armhf (1:9.18.24-0ubuntu5) ... 121s Setting up openssh-client (1:9.6p1-3ubuntu13) ... 121s Setting up python3.12 (3.12.3-1) ... 123s Setting up libxext6:armhf (2:1.3.4-1build2) ... 123s Setting up screen (4.9.1-1build1) ... 123s Setting up libnftnl11:armhf (1.2.6-2build1) ... 123s Setting up e2fsprogs (1.47.0-2.4~exp1ubuntu4) ... 123s update-initramfs: deferring update (trigger activated) 124s e2scrub_all.service is a disabled or a static unit not running, not starting it. 124s Setting up libnss3:armhf (2:3.98-1build1) ... 124s Setting up dbus-daemon (1.14.10-4ubuntu4) ... 124s Setting up kmod (31+20240202-2ubuntu6) ... 124s Setting up sg3-utils-udev (1.46-3ubuntu4) ... 124s update-initramfs: deferring update (trigger activated) 124s Setting up libnl-route-3-200:armhf (3.7.0-0.3build1) ... 124s Setting up dbus-user-session (1.14.10-4ubuntu4) ... 124s Setting up libflashrom1:armhf (1.3.0-2.1ubuntu2) ... 124s Setting up dbus (1.14.10-4ubuntu4) ... 124s A reboot is required to replace the running dbus-daemon. 124s Please reboot the system when convenient. 125s Setting up ftp (20230507-2build3) ... 125s Setting up pciutils (1:3.10.0-2build1) ... 125s Setting up libdrm2:armhf (2.4.120-2build1) ... 125s Setting up dracut-install (060+5-1ubuntu3) ... 125s Setting up xauth (1:1.1.2-1build1) ... 125s Setting up libnetfilter-conntrack3:armhf (1.0.9-6build1) ... 125s Setting up libnl-genl-3-200:armhf (3.7.0-0.3build1) ... 125s Setting up libcryptsetup12:armhf (2:2.7.0-1ubuntu4) ... 125s Setting up bind9-host (1:9.18.24-0ubuntu5) ... 125s Setting up rsync (3.2.7-1ubuntu1) ... 125s rsync.service is a disabled or a static unit not running, not starting it. 125s Setting up libpython3-stdlib:armhf (3.12.3-0ubuntu1) ... 125s Setting up cryptsetup-bin (2:2.7.0-1ubuntu4) ... 125s Setting up openssh-sftp-server (1:9.6p1-3ubuntu13) ... 125s Setting up libnftables1:armhf (1.0.9-1build1) ... 125s Setting up nftables (1.0.9-1build1) ... 126s Setting up openssh-server (1:9.6p1-3ubuntu13) ... 127s Setting up e2fsprogs-l10n (1.47.0-2.4~exp1ubuntu4) ... 127s Setting up iptables (1.8.10-3ubuntu2) ... 127s Setting up htop (3.3.0-4build1) ... 127s Setting up python3 (3.12.3-0ubuntu1) ... 127s Setting up python3-netifaces:armhf (0.11.0-2build3) ... 127s Setting up bind9-dnsutils (1:9.18.24-0ubuntu5) ... 127s Setting up python3-systemd (235-1build4) ... 128s Setting up python3-cffi-backend:armhf (1.16.0-2build1) ... 128s Setting up cloud-init (24.1.3-0ubuntu3) ... 129s Setting up python3-gdbm:armhf (3.12.3-0ubuntu1) ... 129s Setting up python3-problem-report (2.28.1-0ubuntu1) ... 129s Setting up python3-apt (2.7.7ubuntu1) ... 130s Setting up ufw (0.36.2-6) ... 131s Setting up python3-apport (2.28.1-0ubuntu1) ... 131s Setting up apport-core-dump-handler (2.28.1-0ubuntu1) ... 132s Setting up apport (2.28.1-0ubuntu1) ... 132s Installing new version of config file /etc/apport/crashdb.conf ... 132s apport-autoreport.service is a disabled or a static unit not running, not starting it. 133s Processing triggers for debianutils (5.17build1) ... 133s Processing triggers for install-info (7.1-3build2) ... 133s Processing triggers for initramfs-tools (0.142ubuntu24) ... 133s Processing triggers for libc-bin (2.39-0ubuntu8) ... 133s Processing triggers for systemd (255.4-1ubuntu7) ... 133s Reading package lists... 134s Building dependency tree... 134s Reading state information... 134s 0 upgraded, 0 newly installed, 0 to remove and 0 not upgraded. 137s autopkgtest [01:01:40]: rebooting testbed after setup commands that affected boot 179s autopkgtest [01:02:22]: testbed running kernel: Linux 5.4.0-174-generic #193-Ubuntu SMP Thu Mar 7 15:13:37 UTC 2024 207s autopkgtest [01:02:50]: @@@@@@@@@@@@@@@@@@@@ apt-source cpl-plugin-fors 226s Get:1 http://ftpmaster.internal/ubuntu noble/universe cpl-plugin-fors 5.5.7+dfsg-2build1 (dsc) [2571 B] 226s Get:2 http://ftpmaster.internal/ubuntu noble/universe cpl-plugin-fors 5.5.7+dfsg-2build1 (tar) [1299 kB] 226s Get:3 http://ftpmaster.internal/ubuntu noble/universe cpl-plugin-fors 5.5.7+dfsg-2build1 (diff) [13.3 kB] 227s gpgv: Signature made Tue Dec 7 17:25:56 2021 UTC 227s gpgv: using RSA key AC483F68DE728F43F2202FCA568D30F321B2133D 227s gpgv: issuer "steve.langasek@ubuntu.com" 227s gpgv: Can't check signature: No public key 227s dpkg-source: warning: cannot verify inline signature for ./cpl-plugin-fors_5.5.7+dfsg-2build1.dsc: no acceptable signature found 227s autopkgtest [01:03:10]: testing package cpl-plugin-fors version 5.5.7+dfsg-2build1 229s autopkgtest [01:03:12]: build not needed 283s autopkgtest [01:04:06]: test test-recipe.py: preparing testbed 293s Reading package lists... 293s Building dependency tree... 293s Reading state information... 294s Starting pkgProblemResolver with broken count: 0 294s Starting 2 pkgProblemResolver with broken count: 0 294s Done 295s The following additional packages will be installed: 295s cpl-plugin-fors libblas3 libcext0 libcfitsio10t64 libcplcore26 libcpldfs26 295s libcpldrs26 libcplui26 liberfa1 libfftw3-double3 libfftw3-single3 295s libgfortran5 libgomp1 libgsl27 libgslcblas0 libjs-jquery 295s libjs-jquery-hotkeys libjs-jquery-isonscreen libjs-jquery-metadata 295s libjs-jquery-tablesorter libjs-jquery-throttle-debounce libjs-sphinxdoc 295s libjs-underscore liblapack3 libwcs8 python3-astropy 295s python3-astropy-iers-data python3-coverage python3-cpl python3-dateutil 295s python3-erfa python3-hypothesis python3-iniconfig python3-numpy 295s python3-packaging python3-pluggy python3-ply python3-pytest 295s python3-pytest-arraydiff python3-pytest-astropy 295s python3-pytest-astropy-header python3-pytest-cov python3-pytest-doctestplus 295s python3-pytest-filter-subpackage python3-pytest-mock 295s python3-pytest-remotedata python3-sortedcontainers 295s Suggested packages: 295s cpl-plugin-fors-calib cpl-plugin-fors-doc libfftw3-bin libfftw3-dev 295s gsl-ref-psdoc | gsl-doc-pdf | gsl-doc-info | gsl-ref-html libxml2-utils 295s python-astropy-doc python3-astropy-affiliated python3-bs4 python3-h5py 295s python3-matplotlib python3-pandas python-coverage-doc gdb 295s python-hypothesis-doc gcc gfortran python3-dev python-ply-doc 295s python-pytest-mock-doc python-sortedcontainers-doc 295s Recommended packages: 295s source-extractor javascript-common libjs-jquery-datatables python3-scipy 295s python3-click 295s The following NEW packages will be installed: 295s autopkgtest-satdep cpl-plugin-fors libblas3 libcext0 libcfitsio10t64 295s libcplcore26 libcpldfs26 libcpldrs26 libcplui26 liberfa1 libfftw3-double3 295s libfftw3-single3 libgfortran5 libgomp1 libgsl27 libgslcblas0 libjs-jquery 295s libjs-jquery-hotkeys libjs-jquery-isonscreen libjs-jquery-metadata 295s libjs-jquery-tablesorter libjs-jquery-throttle-debounce libjs-sphinxdoc 295s libjs-underscore liblapack3 libwcs8 python3-astropy 295s python3-astropy-iers-data python3-coverage python3-cpl python3-dateutil 295s python3-erfa python3-hypothesis python3-iniconfig python3-numpy 295s python3-packaging python3-pluggy python3-ply python3-pytest 295s python3-pytest-arraydiff python3-pytest-astropy 295s python3-pytest-astropy-header python3-pytest-cov python3-pytest-doctestplus 295s python3-pytest-filter-subpackage python3-pytest-mock 295s python3-pytest-remotedata python3-sortedcontainers 296s 0 upgraded, 48 newly installed, 0 to remove and 0 not upgraded. 296s Need to get 18.5 MB/18.5 MB of archives. 296s After this operation, 80.8 MB of additional disk space will be used. 296s Get:1 /tmp/autopkgtest.8HxwY7/1-autopkgtest-satdep.deb autopkgtest-satdep armhf 0 [724 B] 296s Get:2 http://ftpmaster.internal/ubuntu noble/main armhf libjs-jquery all 3.6.1+dfsg+~3.5.14-1 [328 kB] 296s Get:3 http://ftpmaster.internal/ubuntu noble/universe armhf libjs-jquery-hotkeys all 0~20130707+git2d51e3a9+dfsg-2ubuntu2 [11.5 kB] 296s Get:4 http://ftpmaster.internal/ubuntu noble/universe armhf libcext0 armhf 7.3.2+ds-1build3 [24.9 kB] 296s Get:5 http://ftpmaster.internal/ubuntu noble/universe armhf libcfitsio10t64 armhf 4.3.1-1.1build2 [504 kB] 296s Get:6 http://ftpmaster.internal/ubuntu noble/main armhf libgomp1 armhf 14-20240412-0ubuntu1 [125 kB] 296s Get:7 http://ftpmaster.internal/ubuntu noble/main armhf libfftw3-double3 armhf 3.3.10-1ubuntu3 [369 kB] 297s Get:8 http://ftpmaster.internal/ubuntu noble/main armhf libfftw3-single3 armhf 3.3.10-1ubuntu3 [376 kB] 297s Get:9 http://ftpmaster.internal/ubuntu noble/universe armhf libcplcore26 armhf 7.3.2+ds-1build3 [498 kB] 297s Get:10 http://ftpmaster.internal/ubuntu noble/universe armhf libcplui26 armhf 7.3.2+ds-1build3 [34.5 kB] 297s Get:11 http://ftpmaster.internal/ubuntu noble/universe armhf libcpldfs26 armhf 7.3.2+ds-1build3 [39.4 kB] 297s Get:12 http://ftpmaster.internal/ubuntu noble/universe armhf libwcs8 armhf 8.2.2+ds-3build2 [235 kB] 297s Get:13 http://ftpmaster.internal/ubuntu noble/universe armhf libcpldrs26 armhf 7.3.2+ds-1build3 [68.7 kB] 297s Get:14 http://ftpmaster.internal/ubuntu noble-proposed/universe armhf libgslcblas0 armhf 2.7.1+dfsg-6ubuntu2 [77.8 kB] 297s Get:15 http://ftpmaster.internal/ubuntu noble-proposed/universe armhf libgsl27 armhf 2.7.1+dfsg-6ubuntu2 [827 kB] 297s Get:16 http://ftpmaster.internal/ubuntu noble/universe armhf cpl-plugin-fors armhf 5.5.7+dfsg-2build1 [1101 kB] 297s Get:17 http://ftpmaster.internal/ubuntu noble/main armhf libblas3 armhf 3.12.0-3build1 [123 kB] 297s Get:18 http://ftpmaster.internal/ubuntu noble/main armhf libgfortran5 armhf 14-20240412-0ubuntu1 [316 kB] 297s Get:19 http://ftpmaster.internal/ubuntu noble/universe armhf libjs-jquery-metadata all 12-4 [6582 B] 297s Get:20 http://ftpmaster.internal/ubuntu noble/universe armhf libjs-jquery-tablesorter all 1:2.31.3+dfsg1-3 [193 kB] 297s Get:21 http://ftpmaster.internal/ubuntu noble/universe armhf libjs-jquery-throttle-debounce all 1.1+dfsg.1-2 [12.5 kB] 297s Get:22 http://ftpmaster.internal/ubuntu noble/main armhf libjs-underscore all 1.13.4~dfsg+~1.11.4-3 [118 kB] 297s Get:23 http://ftpmaster.internal/ubuntu noble/main armhf libjs-sphinxdoc all 7.2.6-6 [149 kB] 297s Get:24 http://ftpmaster.internal/ubuntu noble/main armhf liblapack3 armhf 3.12.0-3build1 [2085 kB] 298s Get:25 http://ftpmaster.internal/ubuntu noble/universe armhf python3-iniconfig all 1.1.1-2 [6024 B] 298s Get:26 http://ftpmaster.internal/ubuntu noble/main armhf python3-packaging all 24.0-1 [41.1 kB] 298s Get:27 http://ftpmaster.internal/ubuntu noble/universe armhf python3-pluggy all 1.4.0-1 [20.4 kB] 298s Get:28 http://ftpmaster.internal/ubuntu noble/universe armhf python3-pytest all 7.4.4-1 [305 kB] 298s Get:29 http://ftpmaster.internal/ubuntu noble/main armhf python3-dateutil all 2.8.2-3ubuntu1 [79.4 kB] 298s Get:30 http://ftpmaster.internal/ubuntu noble/main armhf python3-sortedcontainers all 2.4.0-2 [27.6 kB] 298s Get:31 http://ftpmaster.internal/ubuntu noble/universe armhf python3-hypothesis all 6.98.15-1 [311 kB] 298s Get:32 http://ftpmaster.internal/ubuntu noble/main armhf python3-numpy armhf 1:1.26.4+ds-6ubuntu1 [3541 kB] 298s Get:33 http://ftpmaster.internal/ubuntu noble/universe armhf python3-pytest-arraydiff all 0.6.1-2 [10.2 kB] 298s Get:34 http://ftpmaster.internal/ubuntu noble/universe armhf python3-pytest-astropy-header all 0.2.2-1 [8190 B] 298s Get:35 http://ftpmaster.internal/ubuntu noble/universe armhf python3-coverage armhf 7.4.4+dfsg1-0ubuntu2 [146 kB] 298s Get:36 http://ftpmaster.internal/ubuntu noble/universe armhf libjs-jquery-isonscreen all 1.2.0-1.1 [3244 B] 298s Get:37 http://ftpmaster.internal/ubuntu noble/universe armhf python3-pytest-cov all 4.1.0-1 [21.5 kB] 298s Get:38 http://ftpmaster.internal/ubuntu noble/universe armhf python3-pytest-doctestplus all 1.2.0-1 [23.1 kB] 298s Get:39 http://ftpmaster.internal/ubuntu noble/universe armhf python3-pytest-filter-subpackage all 0.2.0-1 [6094 B] 298s Get:40 http://ftpmaster.internal/ubuntu noble/universe armhf python3-pytest-mock all 3.12.0-1.1 [11.3 kB] 298s Get:41 http://ftpmaster.internal/ubuntu noble/universe armhf python3-pytest-remotedata all 0.4.1-1 [8650 B] 298s Get:42 http://ftpmaster.internal/ubuntu noble/universe armhf python3-pytest-astropy all 0.11.0-1 [5902 B] 298s Get:43 http://ftpmaster.internal/ubuntu noble/main armhf python3-ply all 3.11-6 [46.5 kB] 298s Get:44 http://ftpmaster.internal/ubuntu noble/universe armhf python3-astropy-iers-data all 0.2024.01.01.00.33.39-1 [2046 kB] 298s Get:45 http://ftpmaster.internal/ubuntu noble/universe armhf liberfa1 armhf 2.0.1-1 [130 kB] 298s Get:46 http://ftpmaster.internal/ubuntu noble/universe armhf python3-erfa armhf 2.0.1.1+ds-3 [309 kB] 298s Get:47 http://ftpmaster.internal/ubuntu noble/universe armhf python3-astropy armhf 6.0.0-1ubuntu2 [3771 kB] 299s Get:48 http://ftpmaster.internal/ubuntu noble/universe armhf python3-cpl armhf 0.7.4-2build10 [33.5 kB] 299s Fetched 18.5 MB in 3s (6033 kB/s) 299s Selecting previously unselected package libjs-jquery. 299s (Reading database ... (Reading database ... 5% (Reading database ... 10% (Reading database ... 15% (Reading database ... 20% (Reading database ... 25% (Reading database ... 30% (Reading database ... 35% (Reading database ... 40% (Reading database ... 45% (Reading database ... 50% (Reading database ... 55% (Reading database ... 60% (Reading database ... 65% (Reading database ... 70% (Reading database ... 75% (Reading database ... 80% (Reading database ... 85% (Reading database ... 90% (Reading database ... 95% (Reading database ... 100% (Reading database ... 58461 files and directories currently installed.) 299s Preparing to unpack .../00-libjs-jquery_3.6.1+dfsg+~3.5.14-1_all.deb ... 299s Unpacking libjs-jquery (3.6.1+dfsg+~3.5.14-1) ... 299s Selecting previously unselected package libjs-jquery-hotkeys. 299s Preparing to unpack .../01-libjs-jquery-hotkeys_0~20130707+git2d51e3a9+dfsg-2ubuntu2_all.deb ... 299s Unpacking libjs-jquery-hotkeys (0~20130707+git2d51e3a9+dfsg-2ubuntu2) ... 299s Selecting previously unselected package libcext0:armhf. 299s Preparing to unpack .../02-libcext0_7.3.2+ds-1build3_armhf.deb ... 299s Unpacking libcext0:armhf (7.3.2+ds-1build3) ... 300s Selecting previously unselected package libcfitsio10t64:armhf. 300s Preparing to unpack .../03-libcfitsio10t64_4.3.1-1.1build2_armhf.deb ... 300s Unpacking libcfitsio10t64:armhf (4.3.1-1.1build2) ... 300s Selecting previously unselected package libgomp1:armhf. 300s Preparing to unpack .../04-libgomp1_14-20240412-0ubuntu1_armhf.deb ... 300s Unpacking libgomp1:armhf (14-20240412-0ubuntu1) ... 300s Selecting previously unselected package libfftw3-double3:armhf. 300s Preparing to unpack .../05-libfftw3-double3_3.3.10-1ubuntu3_armhf.deb ... 300s Unpacking libfftw3-double3:armhf (3.3.10-1ubuntu3) ... 300s Selecting previously unselected package libfftw3-single3:armhf. 300s Preparing to unpack .../06-libfftw3-single3_3.3.10-1ubuntu3_armhf.deb ... 300s Unpacking libfftw3-single3:armhf (3.3.10-1ubuntu3) ... 300s Selecting previously unselected package libcplcore26:armhf. 300s Preparing to unpack .../07-libcplcore26_7.3.2+ds-1build3_armhf.deb ... 300s Unpacking libcplcore26:armhf (7.3.2+ds-1build3) ... 300s Selecting previously unselected package libcplui26:armhf. 300s Preparing to unpack .../08-libcplui26_7.3.2+ds-1build3_armhf.deb ... 300s Unpacking libcplui26:armhf (7.3.2+ds-1build3) ... 300s Selecting previously unselected package libcpldfs26:armhf. 300s Preparing to unpack .../09-libcpldfs26_7.3.2+ds-1build3_armhf.deb ... 300s Unpacking libcpldfs26:armhf (7.3.2+ds-1build3) ... 300s Selecting previously unselected package libwcs8:armhf. 300s Preparing to unpack .../10-libwcs8_8.2.2+ds-3build2_armhf.deb ... 300s Unpacking libwcs8:armhf (8.2.2+ds-3build2) ... 300s Selecting previously unselected package libcpldrs26:armhf. 300s Preparing to unpack .../11-libcpldrs26_7.3.2+ds-1build3_armhf.deb ... 300s Unpacking libcpldrs26:armhf (7.3.2+ds-1build3) ... 300s Selecting previously unselected package 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up python3-cpl (0.7.4-2build10) ... 312s Setting up autopkgtest-satdep (0) ... 312s Processing triggers for man-db (2.12.0-4build2) ... 313s Processing triggers for libc-bin (2.39-0ubuntu8) ... 331s (Reading database ... 62385 files and directories currently installed.) 331s Removing autopkgtest-satdep (0) ... 337s autopkgtest [01:05:00]: test test-recipe.py: [----------------------- 339s Recipe fors_align_sky: 339s version 5.5.7 339s Parameters: {'dispersion': 0.0, 'startwavelength': 0.0, 'endwavelength': 0.0, 'skyalign': 0, 'wcolumn': 'WLEN'} 339s Docstring: Upgrade wavelength solution using sky lines 339s 339s This recipe is used to align the wavelength solution based on the arc 339s lamp exposure on a set of sky lines observed on a scientific exposure. 339s The input rectified frames are produced by the recipe 339s fors_extract_slits. An input catalog of sky lines can be specified, 339s otherwise an internal one is used. This recipe should be applied to 339s multi-slit MOS/MXU data: for LSS or long-slit like data (MOS/MXU with 339s all slits at the same offset) use recipe fors_align_sky_lss instead. 339s Please refer to the FORS Pipeline User's Manual for more details. In 339s the table below the MXU acronym can be alternatively read as MOS, and 339s SCI as STD. Input files: DO category: Type: 339s Explanation: Required: RECTIFIED_ALL_SCI_MXU or 339s RECTIFIED_SKY_SCI_MXU Calib Frame with sky lines Y 339s SPATIAL_MAP_MXU Calib Spatial coordinate map Y 339s CURV_COEFF_MXU Calib Spectral curvature Y 339s SLIT_LOCATION_MXU Calib Slit location on CCD Y 339s DISP_COEFF_MXU Calib Dispersion solution Y 339s MASTER_SKYLINECAT Calib Catalog of sky lines . 339s GRISM_TABLE Calib Grism table . 339s Output files: DO category: Data type: Explanation: 339s SKY_SHIFTS_SLIT_SCI_MXU FITS table Observed sky lines offsets 339s WAVELENGTH_MAP_SCI_MXU FITS image Wavelength mapped on CCD 339s DISP_COEFF_SCI_MXU FITS image Upgraded dispersion solution 339s 339s Parameters: 339s dispersion: Expected spectral dispersion (Angstrom/pixel) 339s (float; default: 0.0) 339s startwavelength: Start wavelength in spectral extraction (float; 339s default: 0.0) 339s endwavelength: End wavelength in spectral extraction (float; 339s default: 0.0) 339s skyalign: Polynomial order for sky lines alignment (int; 339s default: 0) 339s wcolumn: Name of sky line catalog table column with 339s wavelengths (str; default: 'WLEN') 339s Author: Carlo Izzo 339s 339s 339s Recipe fors_align_sky_lss: 339s version 5.5.7 339s Parameters: {'dispersion': 0.0, 'startwavelength': 0.0, 'endwavelength': 0.0, 'skyalign': 0, 'wcolumn': 'WLEN'} 339s Docstring: Upgrade wavelength solution using sky lines 339s 339s This recipe is used to align the wavelength solution based on the arc 339s lamp exposure on a set of sky lines observed on a scientific exposure. 339s The input scientific frames are produced by the recipes 339s fors_remove_bias and fors_flatfield. An input catalog of sky lines can 339s be specified, or an internal one is used. This recipe should be 339s applied to LSS or long-slit like data (MOS/MXU with all slits at the 339s same offset). For multi-slit MOS/MXU data use recipe fors_align_sky 339s instead. Please refer to the FORS PIpeline User's Manual for more 339s details. In the table below the MXU acronym can be alternatively read 339s as MOS and LSS, and SCI as STD. Input files: DO category: 339s Type: Explanation: Required: SCIENCE_UNBIAS_MXU or 339s SCIENCE_UNFLAT_MXU or STANDARD_UNBIAS_MXU or STANDARD_UNFLAT_MXU 339s Calib Frame with sky lines Y DISP_COEFF_MXU 339s Calib Dispersion solution Y SLIT_LOCATION_MXU 339s Calib Slit location on CCD Y MASTER_SKYLINECAT 339s Calib Catalog of sky lines . GRISM_TABLE 339s Calib Grism table . Output files: DO category: 339s Data type: Explanation: SKY_SHIFTS_LONG_SCI_MXU FITS table 339s Observed sky lines offsets WAVELENGTH_MAP_SCI_MXU FITS image 339s Wavelength mapped on CCD DISP_COEFF_SCI_MXU FITS image 339s Upgraded dispersion solution 339s 339s Parameters: 339s dispersion: Expected spectral dispersion (Angstrom/pixel) 339s (float; default: 0.0) 339s startwavelength: Start wavelength in spectral extraction (float; 339s default: 0.0) 339s endwavelength: End wavelength in spectral extraction (float; 339s default: 0.0) 339s skyalign: Polynomial order for sky lines alignment (int; 339s default: 0) 339s wcolumn: Name of sky line catalog table column with 339s wavelengths (str; default: 'WLEN') 339s Author: Carlo Izzo 339s 339s 339s Recipe fors_bias: 339s version 5.5.7 339s Parameters: {'stack_method': 'minmax', 'minrejection': 1, 'maxrejection': 1, 'klow': 3.0, 'khigh': 3.0, 'kiter': 999} 339s Docstring: Compute the master bias frame 339s 339s This recipe is used to combine input raw BIAS frames into a master 339s bias frame. The overscan regions, if present, are removed from the 339s result. Input files: DO category: Type: 339s Explanation: Required: BIAS Raw 339s Bias frame Y Output files: DO category: 339s Data type: Explanation: MASTER_BIAS FITS image 339s Master bias frame 339s 339s Parameters: 339s stack_method: Frames combination method (str; default: 'minmax') 339s minrejection: Number of lowest values to be rejected (int; default: 339s 1) 339s maxrejection: Number of highest values to be rejected (int; default: 339s 1) 339s klow: Low threshold in ksigma method (float; default: 3.0) 339s khigh: High threshold in ksigma method (float; default: 3.0) 339s kiter: Max number of iterations in ksigma method (int; 339s default: 999) 339s Author: Jonas M. Larsen, Carlo Izzo 339s 339s 339s Recipe fors_calib: 339s version 5.5.7 339s Parameters: {'dispersion': 0.0, 'peakdetection': 0.0, 'wdegree': 0, 'wradius': 4, 'wreject': 0.7, 'wmode': 2, 'wmosmode': 0, 'ignore_lines': '', 'used_linesets': 'standard', 'cdegree': -1, 'cmode': 1, 'startwavelength': 0.0, 'endwavelength': 0.0, 'slit_ident': False, 'stack_method': 'sum', 'ksigma': '-3.0,3.0', 'kiter': 999, 's_degree': -1, 'sradius': -1, 'd_nknots': -1, 'dradius': 10, 'dradius_aver': -1, 'fit_threshold': 0.01, 'nonlinear_level': 60000.0, 'max_nonlinear_ratio': 0.2} 339s Docstring: Determination of the extraction mask 339s 339s This recipe is used to identify reference lines on LSS, MOS and MXU 339s arc lamp exposures, and trace the spectral edges on the corresponding 339s flat field exposures. This information is used to determine the 339s spectral extraction mask to be applied in the scientific data 339s reduction, performed with the recipe fors_science. This recipe accepts 339s both FORS1 and FORS2 frames. The input arc lamp and flat field 339s exposures are assumed to be obtained quasi-simultaneously, so that 339s they would be described by exactly the same instrument distortions. A 339s line catalog must be specified, containing the wavelengths of the 339s reference arc lamp lines used for the wavelength calibration. A grism 339s table (typically depending on the instrument mode, and in particular 339s on the grism used) may also be specified: this table contains a 339s default recipe parameter setting to control the way spectra are 339s extracted for a specific instrument mode, as it is used for automatic 339s run of the pipeline on Paranal and in Garching. If this table is 339s specified, it will modify the default recipe parameter setting, with 339s the exception of those parameters which have been explicitly modified 339s on the command line. If a grism table is not specified, the input 339s recipe parameters values will always be read from the command line, or 339s from an esorex configuration file if present, or from their generic 339s default values (that are rarely meaningful). Finally a master bias 339s frame must be input to this recipe. In the table below the MXU acronym 339s can be read alternatively as MOS and LSS, with the exception of 339s CURV_COEFF_LSS, CURV_TRACES_LSS, SPATIAL_MAP_LSS, 339s SPECTRA_DETECTION_LSS, and and SLIT_MAP_LSS, which are never created. 339s The products SPECTRA_DETECTION_MXU, SLIT_MAP_MXU, and 339s DISP_RESIDUALS_MXU, are just created if the --check parameter is set 339s to true. The product GLOBAL_DISTORTION_TABLE is just created if more 339s than 12 separate spectra are found in the CCD. Input files: DO 339s category: Type: Explanation: Required: 339s SCREEN_FLAT_MXU Raw Flat field exposures Y 339s LAMP_MXU Raw Arc lamp exposure Y 339s MASTER_BIAS Calib Master Bias frame Y 339s MASTER_LINECAT Calib Line catalog Y 339s GRISM_TABLE Calib Grism table . Output 339s files: DO category: Data type: Explanation: 339s MASTER_SCREEN_FLAT_MXU FITS image Combined (sum) flat field 339s MASTER_NORM_FLAT_MXU FITS image Normalised flat field 339s MAPPED_SCREEN_FLAT_MXU FITS image Wavelength calibrated flat field 339s MAPPED_NORM_FLAT_MXU FITS image Wavelength calibrated normalised 339s flat REDUCED_LAMP_MXU FITS image Wavelength calibrated arc 339s spectrum DISP_COEFF_MXU FITS table Inverse dispersion 339s coefficients DISP_RESIDUALS_MXU FITS image Residuals in 339s wavelength calibration DISP_RESIDUALS_TABLE_MXU FITS table 339s Residuals in wavelength calibration DELTA_IMAGE_MXU FITS 339s image Offset vs linear wavelength calib WAVELENGTH_MAP_MXU 339s FITS image Wavelength for each pixel on CCD SPECTRA_DETECTION_MXU 339s FITS image Check for preliminary detection SLIT_MAP_MXU 339s FITS image Map of central wavelength on CCD CURV_TRACES_MXU 339s FITS table Spectral curvature traces CURV_COEFF_MXU FITS 339s table Spectral curvature coefficients SPATIAL_MAP_MXU FITS 339s image Spatial position along slit on CCD SPECTRAL_RESOLUTION_MXU 339s FITS table Resolution at reference arc lines DETECTED_LINES_MXU 339s FITS table All the lines detected in the arc ARC_RECTIFIED_MXU 339s FITS image The spatial rectified arc SLIT_LOCATION_MXU FITS 339s table Slits on product frames and CCD GLOBAL_DISTORTION_TABLE FITS 339s table Global distortions table FLAT_SED_LSS FITS image 339s Average SED for each of the slitsi 339s 339s Parameters: 339s dispersion: Expected spectral dispersion (Angstrom/pixel) 339s (float; default: 0.0) 339s peakdetection: Initial peak detection threshold (ADU) (float; 339s default: 0.0) 339s wdegree: Degree of wavelength calibration polynomial 339s (int; default: 0) 339s wradius: Search radius if iterating pattern-matching with 339s first-guess method (int; default: 4) 339s wreject: Rejection threshold in dispersion relation fit 339s (pixel) (float; default: 0.7) 339s wmode: Interpolation mode of wavelength solution 339s applicable to LSS-like data (0 = no 339s interpolation, 1 = fill gaps, 2 = global model) 339s (int; default: 2) 339s wmosmode: Interpolation mode of wavelength solution (0 = 339s no interpolation, 1 = local (slit) solution, 2 = 339s global model) (int; default: 0) 339s ignore_lines: Catalog lines nearest to wavelengths in this 339s list will be ignored for wavelength calibration 339s (str; default: '') 339s used_linesets: Linesets to use. Valid are 'standard' 339s and'extended' (see column LINE_SET in the line 339s catalogue) (str; default: 'standard') 339s cdegree: Degree of spectral curvature polynomial (int; 339s default: -1) 339s cmode: Interpolation mode of curvature solution 339s applicable to MOS-like data (0 = no 339s interpolation, 1 = fill gaps, 2 = global model) 339s (int; default: 1) 339s startwavelength: Start wavelength in spectral extraction (float; 339s default: 0.0) 339s endwavelength: End wavelength in spectral extraction (float; 339s default: 0.0) 339s slit_ident: Attempt slit identification for MOS or MXU 339s (bool; default: False) 339s stack_method: Frames combination method (str; default: 'sum') 339s ksigma: Low and high threshold in ksigma method (str; 339s default: '-3.0,3.0') 339s kiter: Max number of iterations in ksigma method (int; 339s default: 999) 339s s_degree: Polynomial degree for the flat field fitting 339s along spatial direction (int; default: -1) 339s sradius: Smooth box radius for flat field along spatial 339s direction (int; default: -1) 339s d_nknots: Number of knots in flat field fitting splines 339s along dispersion direction (int; default: -1) 339s dradius: Smooth box radius (median) for flat field along 339s dispersion direction (int; default: 10) 339s dradius_aver: Smooth box radius (average) for flat field along 339s dispersion direction (performed after median 339s smoothing) (int; default: -1) 339s fit_threshold: Threshold percentage for flat spline fittingwith 339s respect to the maximum (float; default: 0.01) 339s nonlinear_level: Level above which the detector is not linear 339s (float; default: 60000.0) 339s max_nonlinear_ratio: Maximum allowed ratio of non-linear pixels per 339s slit (float; default: 0.2) 339s Author: Carlo Izzo 339s 339s 339s Recipe fors_config: 339s version 5.5.7 339s Parameters: {'dispersion': 0.0, 'peakdetection': 250.0, 'wdegree': 4, 'cdegree': 4, 'startwavelength': 0.0, 'endwavelength': 0.0, 'instrument': '0', 'grism': '0', 'grism_id': '0', 'filter': '0', 'filter_id': '0'} 339s Docstring: Creation of FORS recipes configuration tables 339s 339s This recipe is used to create the so-called GRISM_TABLE, containing 339s all the FORS spectral pipeline configuration parameters related to a 339s specific grism. This is a way to provide for each specific instrument 339s mode a set of appropriate defaults for the recipe parameters. The 339s values assigned to each input parameter of fors_config are simply 339s copied to a FITS table consisting of one row, and as many columns as 339s the input parameter: each column will have the same name and type of 339s each parameter. Only the three parameters "instrument", "grism", and 339s "id" are not written to the table columns, but to the descriptor 339s header keywords INSTRUME, ESO INS GRIS1 NAME, and ESO INS GRIS1 ID, 339s that will be used by the automatic pipeline for appropriate data 339s association. Input files: none DO category: Type: 339s Explanation: Required: Output files: DO category: 339s Data type: Explanation: GRISM_TABLE FITS table 339s Recipe configuration parameters 339s 339s Parameters: 339s dispersion: Expected spectral dispersion (Angstrom/pixel) 339s (float; default: 0.0) 339s peakdetection: Peak detection threshold (ADU) (float; default: 339s 250.0) 339s wdegree: Degree of wavelength calibration polynomial (int; 339s default: 4) 339s cdegree: Degree of spectral curvature polynomial (int; 339s default: 4) 339s startwavelength: Start wavelength in spectral extraction (float; 339s default: 0.0) 339s endwavelength: End wavelength in spectral extraction (float; 339s default: 0.0) 339s instrument: Name of instrument (str; default: '0') 339s grism: Name of grism (str; default: '0') 339s grism_id: Grism ID (str; default: '0') 339s filter: Name of filter (str; default: '0') 339s filter_id: Filter ID (str; default: '0') 339s Author: Carlo Izzo 339s 339s 339s Recipe fors_dark: 339s version 5.5.7 339s Parameters: {'stack_method': 'median', 'minrejection': 1, 'maxrejection': 1, 'klow': 3.0, 'khigh': 3.0, 'kiter': 999} 339s Docstring: Compute master dark frame 339s 339s This recipe is used to combine input raw DARK frames into a master 339s dark frame by subtracing the master bias and using the given stacking 339s method. The overscan regions, if present, are removed from the result. 339s Input files: DO category: Type: Explanation: 339s Required: DARK Raw Dark frame 339s Y MASTER_BIAS FITS image Master bias Y 339s Output files: DO category: Data type: Explanation: 339s MASTER_DARK FITS image Master dark frame 339s 339s Parameters: 339s stack_method: Frames combination method (str; default: 'median') 339s minrejection: Number of lowest values to be rejected (int; default: 339s 1) 339s maxrejection: Number of highest values to be rejected (int; default: 339s 1) 339s klow: Low threshold in ksigma method (float; default: 3.0) 339s khigh: High threshold in ksigma method (float; default: 3.0) 339s kiter: Max number of iterations in ksigma method (int; 339s default: 999) 339s Author: Jonas M. Larsen 339s 339s 339s Recipe fors_detect_objects: 339s version 5.5.7 339s Parameters: {'slit_margin': 3, 'ext_radius': 6, 'cont_radius': 0} 339s Docstring: Detect objects in slit spectra 339s 339s This recipe is used to detect scientific objects spectra on a 339s resampled image produced with recipe fors_resample. Please refer to 339s the FORS Pipeline User's Manual for more details on object detection. 339s In the table below the MXU acronym can be alternatively read as MOS 339s and LSS, and SCI as STD. Input files: DO category: 339s Type: Explanation: Required: MAPPED_SCI_MXU 339s Calib Resampled slit spectra Y SLIT_LOCATION_MXU 339s Calib Slit location on image Y Output files: DO category: 339s Data type: Explanation: OBJECT_TABLE_SCI_MXU FITS table 339s Object positions in slit spectra 339s 339s Parameters: 339s slit_margin: Number of pixels to exclude at each slit in object 339s detection and extraction (int; default: 3) 339s ext_radius: Maximum extraction radius for detected objects (pixel) 339s (int; default: 6) 339s cont_radius: Minimum distance at which two objects of equal 339s luminosity do not contaminate each other (pixel) (int; 339s default: 0) 339s Author: Carlo Izzo 339s 339s 339s Recipe fors_detect_spectra: 339s version 5.5.7 339s Parameters: {'dispersion': 0.0, 'peakdetection': 0.0, 'wdegree': 0, 'wradius': 4, 'wreject': 0.7, 'wcolumn': 'WLEN', 'startwavelength': 0.0, 'endwavelength': 0.0, 'slit_ident': True} 339s Docstring: Detect MOS/MXU spectra on CCD 339s 339s This recipe is used to detect and locate MOS/MXU slit spectra on the 339s CCD, applying a pattern-matching algorithm. The input spectral 339s exposure must contain spectra with the dispersion direction 339s approximately horizontal, with blue on the left and red on the right. 339s Use recipe fors_wave_calib_lss for LSS data, or for MOS/MXU data where 339s all slits have the same offset. The rows of the input spectral 339s exposure are processed separately, one by one. First, the background 339s continuum is removed. Second, a list of positions of reference lines 339s candidates is created. Only peaks above a given threshold (specified 339s by the parameter --peakdetection) are selected. Third, the pattern- 339s matching task selects from the found peaks the ones corresponding to 339s the reference lines, listed in the input line catalog, associating 339s them to the appropriate wavelengths. The ensuing polynomial fit is 339s used to locate the central wavelength of the applied grism along each 339s image row. The contributions from all rows form an image of the 339s location of all spectra, that can be used as a starting point for the 339s proper modeling of the optical and spectral distortions. For more 339s details on this reduction strategy please refer to the FORS Pipeline 339s User's Manual. Note that specifying an input GRISM_TABLE will set 339s some of the recipe configuration parameters to default values valid 339s for a particular grism. Again, see the pipeline manual for more 339s details. In the table below the MXU acronym can be alternatively read 339s as MOS. Input files: DO category: Type: 339s Explanation: Required: LAMP_UNBIAS_MXU Calib 339s Bias subtracted arc Y MASTER_LINECAT Calib 339s Line catalog Y GRISM_TABLE Calib 339s Grism table . Output files: DO category: 339s Data type: Explanation: SLIT_MAP_MXU FITS image Map 339s of central wavelength on CCD SLIT_LOCATION_DETECT_MXU FITS table 339s Slits positions on CCD SPECTRA_DETECTION_MXU FITS image Check 339s of preliminary detection 339s 339s Parameters: 339s dispersion: Expected spectral dispersion (Angstrom/pixel) 339s (float; default: 0.0) 339s peakdetection: Initial peak detection threshold (ADU) (float; 339s default: 0.0) 339s wdegree: Degree of wavelength calibration polynomial (int; 339s default: 0) 339s wradius: Search radius if iterating pattern-matching with 339s first-guess method (int; default: 4) 339s wreject: Rejection threshold in dispersion relation fit 339s (pixel) (float; default: 0.7) 339s wcolumn: Name of line catalog table column with wavelengths 339s (str; default: 'WLEN') 339s startwavelength: Start wavelength in spectral extraction (float; 339s default: 0.0) 339s endwavelength: End wavelength in spectral extraction (float; 339s default: 0.0) 339s slit_ident: Attempt slit identification for MOS or MXU (bool; 339s default: True) 339s Author: Carlo Izzo 339s 339s 339s Recipe fors_extract: 339s version 5.5.7 339s Parameters: {'dispersion': 0.0, 'skyalign': 0, 'wcolumn': 'WLEN', 'startwavelength': 0.0, 'endwavelength': 0.0, 'flux': True, 'flatfield': False, 'skyglobal': False, 'skymedian': False, 'skylocal': True, 'cosmics': False, 'slit_margin': 3, 'ext_radius': 6, 'cont_radius': 0, 'ext_mode': 1, 'time_normalise': True} 339s Docstring: Extraction of scientific spectra 339s 339s This recipe is used to reduce scientific spectra using the global 339s distortion table created by the recipe fors_calib. The spectra are 339s bias subtracted, flat fielded (if a normalised flat field is 339s specified) and remapped eliminating the optical distortions. The 339s wavelength calibration can be optionally upgraded using a number of 339s sky lines: if no sky lines catalog of wavelengths is specified, an 339s internal one is used instead. If the alignment to the sky lines is 339s performed, the applied dispersion coefficient table is upgraded and 339s saved to disk, and a new CCD wavelengths map is created. This recipe 339s accepts both FORS1 and FORS2 frames. A grism table (typically 339s depending on the instrument mode, and in particular on the grism used) 339s may also be specified: this table contains a default recipe parameter 339s setting to control the way spectra are extracted for a specific 339s instrument mode, as it is used for automatic run of the pipeline on 339s Paranal and in Garching. If this table is specified, it will modify 339s the default recipe parameter setting, with the exception of those 339s parameters which have been explicitly modifyed on the command line. If 339s a grism table is not specified, the input recipe parameters values 339s will always be read from the command line, or from an esorex 339s configuration file if present, or from their generic default values 339s (that are rarely meaningful). In the table below the MXU acronym can 339s be read alternatively as MOS and LSS, depending on the instrument mode 339s of the input data. Either a scientific or a standard star exposure can 339s be specified in input (not both). Input files: DO category: 339s Type: Explanation: Required: SCIENCE_MXU 339s Raw Scientific exposure Y or STANDARD_MXU Raw 339s Standard star exposure Y MASTER_BIAS Calib 339s Master bias Y GRISM_TABLE Calib 339s Grism table . MASTER_SKYLINECAT Calib Sky 339s lines catalog . MASTER_NORM_FLAT_MXU Calib 339s Normalised flat field . MASTER_DISTORTION_TABLE Calib 339s Global distortion model . or, in case of LSS-like MOS/MXU data, 339s MASTER_NORM_FLAT_LONG_MXU Calib Normalised flat field . 339s Output files: DO category: Data type: Explanation: 339s REDUCED_SCI_MXU FITS image Extracted scientific spectra 339s REDUCED_SKY_SCI_MXU FITS image Extracted sky spectra 339s REDUCED_ERROR_SCI_MXU FITS image Errors on extracted spectra 339s UNMAPPED_SCI_MXU FITS image Sky subtracted scientific 339s spectra MAPPED_SCI_MXU FITS image Rectified scientific 339s spectra MAPPED_ALL_SCI_MXU FITS image Rectified science 339s spectra with sky MAPPED_SKY_SCI_MXU FITS image Rectified 339s sky spectra UNMAPPED_SKY_SCI_MXU FITS image Sky on CCD 339s GLOBAL_SKY_SPECTRUM_MXU FITS table Global sky spectrum 339s OBJECT_TABLE_SCI_MXU FITS table Positions of detected objects 339s Only if the sky-alignment of the wavelength solution is requested: 339s SKY_SHIFTS_LONG_SCI_MXU FITS table Sky lines offsets (LSS-like 339s data) or SKY_SHIFTS_SLIT_SCI_MXU FITS table Sky lines offsets (MOS- 339s like data) DISP_COEFF_SCI_MXU FITS table Upgraded 339s dispersion coefficients WAVELENGTH_MAP_SCI_MXU FITS image 339s Upgraded wavelength map 339s 339s Parameters: 339s dispersion: Resampling step (Angstrom/pixel) (float; default: 339s 0.0) 339s skyalign: Polynomial order for sky lines alignment, or -1 to 339s avoid alignment (int; default: 0) 339s wcolumn: Name of sky line catalog table column with 339s wavelengths (str; default: 'WLEN') 339s startwavelength: Start wavelength in spectral extraction (float; 339s default: 0.0) 339s endwavelength: End wavelength in spectral extraction (float; 339s default: 0.0) 339s flux: Apply flux conservation (bool; default: True) 339s flatfield: Apply flat field (bool; default: False) 339s skyglobal: Subtract global sky spectrum from CCD (bool; 339s default: False) 339s skymedian: Sky subtraction from extracted slit spectra (bool; 339s default: False) 339s skylocal: Sky subtraction from CCD slit spectra (bool; 339s default: True) 339s cosmics: Eliminate cosmic rays hits (only if global sky 339s subtraction is also requested) (bool; default: 339s False) 339s slit_margin: Number of pixels to exclude at each slit in object 339s detection and extraction (int; default: 3) 339s ext_radius: Maximum extraction radius for detected objects 339s (pixel) (int; default: 6) 339s cont_radius: Minimum distance at which two objects of equal 339s luminosity do not contaminate each other (pixel) 339s (int; default: 0) 339s ext_mode: Object extraction method: 0 = aperture, 1 = Horne 339s optimal extraction (int; default: 1) 339s time_normalise: Normalise output spectra by the exposure time (bool; 339s default: True) 339s Author: Carlo Izzo 339s 339s 339s Recipe fors_extract_objects: 339s version 5.5.7 339s Parameters: {'ext_mode': 1} 339s Docstring: Extract objects in slit spectra 339s 339s This recipe is used to extract scientific objects spectra on a 339s resampled image produced with recipe fors_resample, at the positions 339s listed in the object table produced by recipe fors_detect_objects. 339s Please refer to the FORS Pipeline User's Manual for more details on 339s object extraction. In the table below the MXU acronym can be 339s alternatively read as MOS and LSS, and SCI as STD. Input files: DO 339s category: Type: Explanation: Required: 339s MAPPED_SCI_MXU Calib Resampled slit spectra Y 339s MAPPED_SKY_SCI_MXU Calib Resampled sky spectra Y 339s OBJECT_TABLE_SCI_MXU Calib Object table Y 339s Output files: DO category: Data type: Explanation: 339s REDUCED_SCI_MXU FITS image Extracted object spectra 339s REDUCED_SKY_SCI_MXU FITS image Extracted sky spectra 339s REDUCED_ERROR_SCI_MXU FITS image Error on extracted spectra 339s 339s Parameters: 339s ext_mode: Object extraction method: 0 = aperture, 1 = Horne optimal 339s extraction (int; default: 1) 339s Author: Carlo Izzo 339s 339s 339s Recipe fors_extract_slits: 339s version 5.5.7 339s Parameters: {'dispersion': 0.0, 'startwavelength': 0.0, 'endwavelength': 0.0, 'flux': True} 339s Docstring: Spatial rectification of spectral image 339s 339s This recipe is used to extract MOS/MXU slit spectra, following their 339s curvature, and to remap them into a spatially rectified image. Please 339s refer to the FORS Pipeline User's Manual for details about the spectra 339s remapping technique. Note however that the interpolation is done 339s exclusively along the spatial direction, and therefore the output 339s rectified image will have the same x size of the input spectral image. 339s In the table below the MXU acronym can be alternatively read as MOS. 339s Input files: DO category: Type: Explanation: 339s Required: LAMP_UNBIAS_MXU or SCIENCE_UNBIAS_MXU or 339s SCIENCE_UNFLAT_MXU or STANDARD_UNBIAS_MXU or STANDARD_UNFLAT_MXU 339s or UNMAPPED_SCI_MXU or UNMAPPED_STD_MXU or UNMAPPED_SKY_SCI_MXU 339s or UNMAPPED_SKY_STD_MXU Calib Spectral frame Y 339s SLIT_LOCATION_DETECT_MXU or SLIT_LOCATION_MXU Calib 339s Master flat frame Y CURV_COEFF_MXU Calib 339s Spectral curvature Y GRISM_TABLE Calib 339s Grism table . Output files: DO category: 339s Data type: Explanation: RECTIFIED_LAMP_MXU or 339s RECTIFIED_ALL_SCI_MXU or RECTIFIED_ALL_STD_MXU or 339s RECTIFIED_SCI_MXU or RECTIFIED_STD_MXU or RECTIFIED_SKY_SCI_MXU 339s or RECTIFIED_SKY_STD_MXU FITS image Rectified slit spectra 339s 339s Parameters: 339s dispersion: Expected spectral dispersion (Angstrom/pixel) 339s (float; default: 0.0) 339s startwavelength: Start wavelength in spectral extraction (float; 339s default: 0.0) 339s endwavelength: End wavelength in spectral extraction (float; 339s default: 0.0) 339s flux: Apply flux conservation (bool; default: True) 339s Author: Carlo Izzo 339s 339s 339s Recipe fors_flatfield: 339s version 5.5.7 339s Parameters: {} 339s Docstring: Flat field correction of input frame 339s 339s This recipe is used to divide the input frame by the normalised flat 339s field frame produced by recipe fors_normalise_flat. The input frame 339s must be already bias subtracted (e.g., by recipe fors_remove_bias). In 339s the table below the MXU acronym can be alternatively read as MOS and 339s LSS. Input files: DO category: Type: 339s Explanation: Required: SCIENCE_UNBIAS_MXU or 339s STANDARD_UNBIAS_MXU Raw Bias subtracted frame Y 339s MASTER_NORM_FLAT_MXU Calib Normalised flat frame Y 339s Output files: DO category: Data type: Explanation: 339s SCIENCE_UNFLAT_MXU or STANDARD_UNFLAT_MXU FITS image Flat field 339s corrected frame 339s 339s No parameters 339s Author: Carlo Izzo 339s 339s 339s Recipe fors_img_science: 339s version 5.5.7 339s Parameters: {'magsyserr': 0.01, 'sex_exe': '/usr/bin/source-extractor', 'sex_config': '/usr/share/cpl-plugins/fors-5.5.7/config/fors.sex', 'sex_mag': 'MAG_APER', 'sex_magerr': 'MAGERR_APER', 'sex_radius': 64, 'idp_generate': False, 'idp_weights_threshold': 0.5} 339s Docstring: Reduce imaging scientific exposure 339s 339s Input files: DO category: Type: Explanation: 339s Number: SCIENCE_IMG Raw Science image 339s 1 MASTER_BIAS FITS image Master bias 339s 1 MASTER_SKY_FLAT_IMG FITS image Master sky flat field 339s 1 PHOT_COEFF_TABLE FITS table Observed extinction 339s coefficients 0+ EXTINCTION_PER_NIGHT FITS table 339s Extinction per night 0+ 339s STATIC_PHOT_COEFF_TABLE FITS table Static filters photometry 339s coefficients 0+ DETECTOR_ILLUMINATED_REGION FITS table 339s Table with detector illuminated regions 0+ Output files: DO 339s category: Data type: Explanation: SCIENCE_REDUCED_IMG 339s FITS image Reduced science image PHOT_BACKGROUND_SCI_IMG FITS 339s image Reduced science image background SOURCES_SCI_IMG 339s FITS image Unfiltered SExtractor output OBJECT_TABLE_SCI_IMG 339s FITS table Extracted sources properties SCIENCE_REDUCED_IMG_IDP 339s FITS image Reduced science image in IDP-compliant format 339s SCIENCE_REDUCED_WEIGHT_IDP FITS image Ancillary file with the weights 339s for IDP the image SCIENCE_REDUCED_ERR_IDP FITS image Ancillary 339s file with the errors for IDP the image 339s 339s Parameters: 339s magsyserr: Systematic error in magnitude (float; default: 339s 0.01) 339s sex_exe: SExtractor executable (str; default: 339s '/usr/bin/source-extractor') 339s sex_config: SExtractor configuration file (str; default: 339s '/usr/share/cpl- 339s plugins/fors-5.5.7/config/fors.sex') 339s sex_mag: SExtractor magnitude (str; default: 339s 'MAG_APER') 339s sex_magerr: SExtractor magnitude error (str; default: 339s 'MAGERR_APER') 339s sex_radius: Background error map median filter radius 339s (unbinned pixels) (int; default: 64) 339s idp_generate: If TRUE compliant IDP science products are 339s generated (bool; default: False) 339s idp_weights_threshold: Every pixel in the MASTER_SKY_FLAT_IMG below 339s the threshold will be put to 0 in the weight- 339s map, 1 otherwise. Ignored if IDP generation is 339s not requested (float; default: 0.5) 339s Author: ESO PPS Group 339s 339s 339s Recipe fors_img_screen_flat: 339s version 5.5.7 339s Parameters: {'stack_method': 'average', 'minrejection': 1, 'maxrejection': 1, 'klow': 3.0, 'khigh': 3.0, 'kiter': 999, 'xradius': 50, 'yradius': 50, 'degree': -1, 'sampling': 100} 339s Docstring: Compute master screen flat frame 339s 339s After bias subtraction, the input flat field frames are combined using 339s the given stack method. The combined frame is finally normalised 339s dividing it by its large scale illumination trend. The large scale 339s trend is obtained by applying a median filter with a large kernel. To 339s avoid boundary effects, the median filter is applied only to the 339s specified region. The overscan regions, if present, are removed from 339s the result. Input files: DO category: Type: 339s Explanation: Required: SCREEN_FLAT_IMG Raw 339s Screen flat field Y MASTER_BIAS Raw Master 339s bias Y Output files: DO category: Data 339s type: Explanation: MASTER_SCREEN_FLAT_IMG FITS image Master 339s screen flat field 339s 339s Parameters: 339s stack_method: Frames combination method (str; default: 'average') 339s minrejection: Number of lowest values to be rejected (int; default: 339s 1) 339s maxrejection: Number of highest values to be rejected (int; default: 339s 1) 339s klow: Low threshold in ksigma method (float; default: 3.0) 339s khigh: High threshold in ksigma method (float; default: 3.0) 339s kiter: Max number of iterations in ksigma method (int; 339s default: 999) 339s xradius: Median filter x radius (unbinned pixels) (int; default: 339s 50) 339s yradius: Median filter y radius (unbinned pixels) (int; default: 339s 50) 339s degree: Degree of fitting polynomial (int; default: -1) 339s sampling: Sampling interval for fitting (int; default: 100) 339s Author: Jonas M. Larsen 339s 339s 339s Recipe fors_img_sky_flat: 339s version 5.5.7 339s Parameters: {'stack_method': 'median', 'minrejection': 1, 'maxrejection': 1, 'klow': 3.0, 'khigh': 3.0, 'kiter': 999} 339s Docstring: Compute master img_sky_flat frame 339s 339s Input files: DO category: Type: Explanation: 339s Number: SKY_FLAT_IMG Raw Jittered sky flat 339s fields 1+ MASTER_BIAS FITS image Master bias 339s 1 Output files: DO category: Data type: Explanation: 339s MASTER_SKY_FLAT_IMG FITS image Master sky flat field 339s 339s Parameters: 339s stack_method: Frames combination method (str; default: 'median') 339s minrejection: Number of lowest values to be rejected (int; default: 339s 1) 339s maxrejection: Number of highest values to be rejected (int; default: 339s 1) 339s klow: Low threshold in ksigma method (float; default: 3.0) 339s khigh: High threshold in ksigma method (float; default: 3.0) 339s kiter: Max number of iterations in ksigma method (int; 339s default: 999) 339s Author: Jonas M. Larsen 339s 339s 339s Recipe fors_normalise_flat: 339s version 5.5.7 339s Parameters: {'dispersion': 0.0, 'startwavelength': 0.0, 'endwavelength': 0.0, 'spa_polydegree': -1, 'sradius': 10, 'disp_nknots': -1, 'dradius': 10, 'dradius_aver': 10, 'splfit_threshold': 0.01} 339s Docstring: Normalise master flat spectrum 339s 339s This recipe is used to normalise a master flat field frame dividing it 339s by its large scale illumination trend. This recipe can be applied both 339s to generic multi-slit (MOS/MXU) and to long slit exposures (either 339s LSS, or LSS-like MOS/MXU), even if different normalisation methods are 339s applied in such different cases. The input master flat field image is 339s the product of the recipe fors_flat. The input spectral curvature 339s table, product of the recipe fors_detect_spectra, is only required in 339s the case of multi-slit data. In the case of multi-slit data, the flat 339s field spectra are spatially rectified, heavily smoothed, and then 339s mapped back on the CCD. Then the master flat image is divided by its 339s smoothed counterpart. The smoothing may be obtained either by applying 339s a running median filter of specified sizes, or by polynomial fitting 339s along the dispersion direction performed independently for each row of 339s the spatially remapped spectra. In the case of long-slit data, the 339s smoothing can still be obtained either by applying a running median 339s filter or by polynomial fitting, but the polynomial fitting will be 339s performed along the spatial direction, for each column of the 339s spectrum. In the table below the MXU acronym can be alternatively 339s read as MOS or LSS. Input files: DO category: Type: 339s Explanation: Required: MASTER_SCREEN_FLAT_MXU Calib 339s Master flat frame Y DISP_COEFF_MXU Calib 339s Wavelength calibration Y CURV_COEFF_MXU Calib 339s Spectral curvature . SLIT_LOCATION_MXU Calib 339s Slit detection . GRISM_TABLE Calib 339s Grism table Y Output files: DO category: 339s Data type: Explanation: MASTER_NORM_FLAT_MXU FITS image 339s Normalised flat field 339s 339s Parameters: 339s dispersion: Expected spectral dispersion (Angstrom/pixel) 339s (float; default: 0.0) 339s startwavelength: Start wavelength in spectral extraction (float; 339s default: 0.0) 339s endwavelength: End wavelength in spectral extraction (float; 339s default: 0.0) 339s spa_polydegree: Polynomial degree for the flat field fitting along 339s spatial direction (int; default: -1) 339s sradius: Smooth box radius for flat field along spatial 339s direction (int; default: 10) 339s disp_nknots: Number of knots in flat field fitting splines along 339s dispersion direction (int; default: -1) 339s dradius: Smooth box radius (median) for flat field along 339s dispersion direction (int; default: 10) 339s dradius_aver: Smooth box radius (average) for flat field along 339s dispersion direction (performed after median 339s smoothing) (int; default: 10) 339s splfit_threshold: Threshold percentage for flat spline fittingwith 339s respect to the maximum (float; default: 0.01) 339s Author: Carlo Izzo 339s 339s 339s Recipe fors_photometry: 339s version 5.5.7 339s Parameters: {'fitz': True, 'fit_all_mag': False, 'fite': 'pernight', 'fitc': False, 'use_all_stars': False, 'degreef1': 0, 'degreef2': -1, 'degreep': 0, 'mjd_obs_target': -1.0} 339s Docstring: Compute corrected flatfield 339s 339s Input files: DO category: Type: Explanation: 339s Number: PHOT_TABLE FITS table Expected extinction 339s params 1 ALIGNED_PHOT FITS table Photometry 339s 1+ MASTER_SKY_FLAT_IMG FITS image Master flat field 339s 1 Output files: DO category: Data type: Explanation: 339s PHOT_COEFF_TABLE FITS image Observed extinction 339s coefficients CORRECTION_MAP FITS image Correction map 339s (magnitude) CORRECTION_FACTOR FITS image Correction map 339s (flux) MASTER_FLAT_IMG FITS image Corrected master flat 339s field 339s 339s Parameters: 339s fitz: Fit zeropoint (bool; default: True) 339s fit_all_mag: Always fit star magnitudes (bool; default: False) 339s fite: Fit atmospheric extinctions (str; default: 339s 'pernight') 339s fitc: Fit color correction term (bool; default: False) 339s use_all_stars: Use also non-standard stars to fit polynomial f 339s (bool; default: False) 339s degreef1: FLatfield correction map polynomial degree (x) (int; 339s default: 0) 339s degreef2: Flatfield correction map polynomial degree (y), or 339s negative for triangular coefficient matrix (int; 339s default: -1) 339s degreep: Extinction/color coupling degree (int; default: 0) 339s mjd_obs_target: MJD-OBS used to match the raw frame from which 339s EXTINCTION_PER_NIGHT and PHOT_COEFF inherit MJD-OBS. 339s If negative theMJD-OBS of the first raw frame isused 339s (float; default: -1.0) 339s Author: Jonas M. Larsen 339s 339s 339s Recipe fors_pmos_calib: 339s version 5.5.7 339s Parameters: {'dispersion': 0.0, 'peakdetection': 0.0, 'wdegree': 0, 'wradius': 4, 'wreject': 0.7, 'wcolumn': 'WLEN', 'cdegree': 0, 'cmode': 1, 'startwavelength': 0.0, 'endwavelength': 0.0, 'stack_method': 'average', 'minrejection': 1, 'maxrejection': 1, 'klow': 3.0, 'khigh': 3.0, 'kiter': 999, 'ddegree': -1, 'dradius': 10, 'qc': True, 'check': False} 339s Docstring: Determination of the extraction mask 339s 339s This recipe is used to identify reference lines on PMOS arc lamp 339s exposures, and trace the spectral edges on the corresponding flat 339s field exposures. This information is used to determine the spectral 339s extraction mask to be applied in the scientific data reduction, 339s performed with the recipe fors_science. This recipe accepts both FORS1 339s and FORS2 frames. The input arc lamps and flat field exposures are 339s assumed to be obtained quasi-simultaneously, so that they would be 339s described by exactly the same instrument distortions. A line catalog 339s must be specified, containing the wavelengths of the reference arc 339s lamp lines used for the wavelength calibration. A grism table 339s (typically depending on the instrument mode, and in particular on the 339s grism used) may also be specified: this table contains a default 339s recipe parameter setting to control the way spectra are extracted for 339s a specific instrument mode, as it is used for automatic run of the 339s pipeline on Paranal and in Garching. If this table is specified, it 339s will modify the default recipe parameter setting, with the exception 339s of those parameters which have been explicitly modifyed on the command 339s line. If a grism table is not specified, the input recipe parameters 339s values will always be read from the command line, or from an esorex 339s configuration file if present, or from their generic default values 339s (that are rarely meaningful). Finally a master bias frame must be 339s input to this recipe. The products SPECTRA_DETECTION_PMOS, 339s SLIT_MAP_PMOS, and DISP_RESIDUALS_PMOS, are just created if the 339s --check parameter is set to true. The MASTER_DISTORTION_TABLE is 339s marked as required, but it is not so if all slits have different 339s offsets, and in the case of FORS1 observations made with the old 339s TK2048EB4-1 1604 chip read in windowed mode (2048x400) Input files: 339s DO category: Type: Explanation: Required: 339s SCREEN_FLAT_PMOS Raw Flat field exposures Y 339s LAMP_PMOS Raw Arc lamp exposure Y 339s MASTER_BIAS or BIAS Calib Bias frame Y 339s MASTER_LINECAT Calib Line catalog Y 339s GRISM_TABLE Calib Grism table . 339s MASTER_DISTORTION_TABLE Calib Master distortions table Y 339s Output files: DO category: Data type: Explanation: 339s MASTER_SCREEN_FLAT_PMOS FITS image Combined (sum) flat field 339s MASTER_NORM_FLAT_PMOS FITS image Normalised flat field 339s MAPPED_SCREEN_FLAT_PMOS FITS image Wavelength calibrated flat field 339s MAPPED_NORM_FLAT_PMOS FITS image Wavelength calibrated normalised 339s flat REDUCED_LAMP_PMOS FITS image Wavelength calibrated arc 339s spectrum DISP_COEFF_PMOS FITS table Inverse dispersion 339s coefficients DISP_RESIDUALS_PMOS FITS image Residuals in 339s wavelength calibration DISP_RESIDUALS_TABLE_PMOS FITS table 339s Residuals in wavelength calibration DELTA_IMAGE_PMOS FITS 339s image Offset vs linear wavelength calib WAVELENGTH_MAP_PMOS 339s FITS image Wavelength for each pixel on CCD SPECTRA_DETECTION_PMOS 339s FITS image Check for preliminary detection SLIT_MAP_PMOS 339s FITS image Map of central wavelength on CCD CURV_TRACES_PMOS 339s FITS table Spectral curvature traces CURV_COEFF_PMOS FITS 339s table Spectral curvature coefficients SPATIAL_MAP_PMOS 339s FITS image Spatial position along slit on CCD 339s SPECTRAL_RESOLUTION_PMOS FITS table Resolution at reference arc 339s lines SLIT_LOCATION_PMOS FITS table Slits on product frames 339s and CCD 339s 339s Parameters: 339s dispersion: Expected spectral dispersion (Angstrom/pixel) 339s (float; default: 0.0) 339s peakdetection: Initial peak detection threshold (ADU) (float; 339s default: 0.0) 339s wdegree: Degree of wavelength calibration polynomial (int; 339s default: 0) 339s wradius: Search radius if iterating pattern-matching with 339s first-guess method (int; default: 4) 339s wreject: Rejection threshold in dispersion relation fit 339s (pixel) (float; default: 0.7) 339s wcolumn: Name of line catalog table column with wavelengths 339s (str; default: 'WLEN') 339s cdegree: Degree of spectral curvature polynomial (int; 339s default: 0) 339s cmode: Interpolation mode of curvature solution (0 = no 339s interpolation, 1 = fill gaps, 2 = global model) 339s (int; default: 1) 339s startwavelength: Start wavelength in spectral extraction (float; 339s default: 0.0) 339s endwavelength: End wavelength in spectral extraction (float; 339s default: 0.0) 339s stack_method: Frames combination method (str; default: 'average') 339s minrejection: Number of lowest values to be rejected (int; 339s default: 1) 339s maxrejection: Number of highest values to be rejected (int; 339s default: 1) 339s klow: Low threshold in ksigma method (float; default: 3.0) 339s khigh: High threshold in ksigma method (float; default: 339s 3.0) 339s kiter: Max number of iterations in ksigma method (int; 339s default: 999) 339s ddegree: Degree of flat field fitting polynomial along 339s dispersion direction (int; default: -1) 339s dradius: Smooth box radius for flat field along dispersion 339s direction (int; default: 10) 339s qc: Compute QC1 parameters (bool; default: True) 339s check: Create intermediate products (bool; default: False) 339s Author: Carlo Izzo 339s 339s 339s Recipe fors_pmos_extract: 339s version 5.5.7 339s Parameters: {'dispersion': 0.0, 'skyalign': 0, 'wcolumn': 'WLEN', 'startwavelength': 0.0, 'endwavelength': 0.0, 'flux': True, 'flatfield': False, 'skyglobal': False, 'skymedian': False, 'skylocal': True, 'cosmics': False, 'slit_margin': 3, 'ext_radius': 6, 'cont_radius': 0, 'ext_mode': 1, 'time_normalise': True, 'chromatism': True, 'check': False} 339s Docstring: Extraction of scientific spectra 339s 339s This recipe is used to reduce scientific spectra using the extraction 339s mask and the products created by the recipe fors_mpol_calib. The 339s spectra are bias subtracted, flat fielded (if a normalised flat field 339s is specified) and remapped eliminating the optical distortions. The 339s wavelength calibration can be optionally upgraded using a number of 339s sky lines: if no sky lines catalog of wavelengths is specified, an 339s internal one is used instead. If the alignment to the sky lines is 339s performed, the input dispersion coefficients table is upgraded and 339s saved to disk, and a new CCD wavelengths map is created. This recipe 339s accepts both FORS1 and FORS2 frames. A grism table (typically 339s depending on the instrument mode, and in particular on the grism used) 339s may also be specified: this table contains a default recipe parameter 339s setting to control the way spectra are extracted for a specific 339s instrument mode, as it is used for automatic run of the pipeline on 339s Paranal and in Garching. If this table is specified, it will modify 339s the default recipe parameter setting, with the exception of those 339s parameters which have been explicitly modifyed on the command line. If 339s a grism table is not specified, the input recipe parameters values 339s will always be read from the command line, or from an esorex 339s configuration file if present, or from their generic default values 339s (that are rarely meaningful). Either a scientific or a standard star 339s exposure can be specified in input. The acronym SCI on products should 339s be read STD in case of standard stars observations. Input files: 339s DO category: Type: Explanation: Required: 339s SCIENCE_PMOS Raw Scientific exposure Y 339s or STANDARD_PMOS Raw Standard star exposure Y 339s MASTER_BIAS Calib Master bias Y 339s GRISM_TABLE Calib Grism table . 339s MASTER_SKYLINECAT Calib Sky lines catalog . 339s MASTER_NORM_FLAT_PMOS Calib Normalised flat field . 339s DISP_COEFF_PMOS Calib Inverse dispersion Y 339s CURV_COEFF_PMOS Calib Spectral curvature Y 339s SLIT_LOCATION_PMOS Calib Slits positions table Y 339s RETARDER_WAVEPLATE_CHROMATISM Calib Chromatism correction . 339s Output files: DO category: Data type: Explanation: 339s REDUCED_SCI_PMOS FITS image Extracted scientific spectra 339s REDUCED_SKY_SCI_PMOS FITS image Extracted sky spectra 339s REDUCED_ERROR_SCI_PMOS FITS image Errors on extracted spectra 339s REDUCED_SCI_X_PMOS FITS image X Stokes parameter (and L) 339s REDUCED_ERROR_X_PMOS FITS image Error on X Stokes parameter 339s REDUCED_NUL_X_PMOS FITS image Null parameter for X 339s REDUCED_POL_ANGLE_PMOS FITS image Direction of linear 339s polarization REDUCED_POL_ANGLE_ERROR_PMOS FITS image Error on 339s polarization direction UNMAPPED_SCI_PMOS FITS image Sky 339s subtracted scientific spectra MAPPED_SCI_PMOS FITS 339s image Rectified scientific spectra MAPPED_ALL_SCI_PMOS 339s FITS image Rectified science spectra with sky MAPPED_SKY_SCI_PMOS 339s FITS image Rectified sky spectra UNMAPPED_SKY_SCI_PMOS FITS 339s image Sky on CCD GLOBAL_SKY_SPECTRUM_PMOS FITS table Global 339s sky spectrum OBJECT_TABLE_SCI_PMOS FITS table Positions of 339s detected objects OBJECT_TABLE_POL_SCI_PMOS FITS table Positions 339s of real objects Only if the sky-alignment of the wavelength 339s solution is requested: DISP_COEFF_SCI_PMOS FITS table 339s Upgraded dispersion coefficients WAVELENGTH_MAP_SCI_PMOS FITS 339s image Upgraded wavelength map 339s 339s Parameters: 339s dispersion: Resampling step (Angstrom/pixel) (float; default: 339s 0.0) 339s skyalign: Polynomial order for sky lines alignment, or -1 to 339s avoid alignment (int; default: 0) 339s wcolumn: Name of sky line catalog table column with 339s wavelengths (str; default: 'WLEN') 339s startwavelength: Start wavelength in spectral extraction (float; 339s default: 0.0) 339s endwavelength: End wavelength in spectral extraction (float; 339s default: 0.0) 339s flux: Apply flux conservation (bool; default: True) 339s flatfield: Apply flat field (bool; default: False) 339s skyglobal: Subtract global sky spectrum from CCD (bool; 339s default: False) 339s skymedian: Sky subtraction from extracted slit spectra (bool; 339s default: False) 339s skylocal: Sky subtraction from CCD slit spectra (bool; 339s default: True) 339s cosmics: Eliminate cosmic rays hits (only if global sky 339s subtraction is also requested) (bool; default: 339s False) 339s slit_margin: Number of pixels to exclude at each slit in object 339s detection and extraction (int; default: 3) 339s ext_radius: Maximum extraction radius for detected objects 339s (pixel) (int; default: 6) 339s cont_radius: Minimum distance at which two objects of equal 339s luminosity do not contaminate each other (pixel) 339s (int; default: 0) 339s ext_mode: Object extraction method: 0 = aperture, 1 = Horne 339s optimal extraction (int; default: 1) 339s time_normalise: Normalise output spectra by the exposure time (bool; 339s default: True) 339s chromatism: Chromatism correction to polarization angles (bool; 339s default: True) 339s check: Create intermediate products (bool; default: False) 339s Author: Carlo Izzo 339s 339s 339s Recipe fors_pmos_science: 339s version 5.5.7 339s Parameters: {'dispersion': 0.0, 'rebin': 1, 'skyalign': 0, 'wcolumn': 'WLEN', 'startwavelength': 0.0, 'endwavelength': 0.0, 'flux': True, 'flatfield': True, 'skymedian': False, 'skylocal': True, 'cosmics': False, 'slit_margin': 3, 'ext_radius': 12, 'cont_radius': 0, 'ext_mode': 1, 'match_tolerance': 5.0, 'time_normalise': True, 'chromatism': True, 'wollaston': True, 'qc': True} 339s Docstring: Extraction of scientific spectra 339s 339s This recipe is used to reduce scientific spectra using the extraction 339s mask and the products created by the recipe fors_mpol_calib. The 339s spectra are bias subtracted, flat fielded (if a normalised flat field 339s is specified) and remapped eliminating the optical distortions. The 339s wavelength calibration can be optionally upgraded using a number of 339s sky lines: if no sky lines catalog of wavelengths is specified, an 339s internal one is used instead. If the alignment to the sky lines is 339s performed, the input dispersion coefficients table is upgraded and 339s saved to disk, and a new CCD wavelengths map is created. This recipe 339s accepts both FORS1 and FORS2 frames. A grism table (typically 339s depending on the instrument mode, and in particular on the grism used) 339s may also be specified: this table contains a default recipe parameter 339s setting to control the way spectra are extracted for a specific 339s instrument mode, as it is used for automatic run of the pipeline on 339s Paranal and in Garching. If this table is specified, it will modify 339s the default recipe parameter setting, with the exception of those 339s parameters which have been explicitly modifyed on the command line. If 339s a grism table is not specified, the input recipe parameters values 339s will always be read from the command line, or from an esorex 339s configuration file if present, or from their generic default values 339s (that are rarely meaningful). Either a scientific or a standard star 339s exposure can be specified in input. The acronym SCI on products should 339s be read STD in case of standard stars observations. Input files: 339s DO category: Type: Explanation: 339s Required: SCIENCE_PMOS Raw Scientific 339s exposure Y or STANDARD_PMOS Raw Standard 339s star exposure Y MASTER_BIAS Calib Master 339s bias Y GRISM_TABLE Calib Grism 339s table . MASTER_SKYLINECAT Calib Sky 339s lines catalog . MASTER_NORM_FLAT_PMOS Calib 339s Normalised flat field . DISP_COEFF_PMOS Calib 339s Inverse dispersion Y CURV_COEFF_PMOS Calib 339s Spectral curvature Y SLIT_LOCATION_PMOS Calib 339s Slits positions table Y RETARDER_WAVEPLATE_CHROMATISM Calib 339s Chromatism correction . STD_PMOS_TABLE Calib 339s Linear pol. of std stars . Output files: DO category: 339s Data type: Explanation: REDUCED_SCI_PMOS FITS image 339s Extracted scientific spectra REDUCED_SKY_SCI_PMOS FITS image 339s Extracted sky spectra REDUCED_ERROR_SCI_PMOS FITS image 339s Errors on extracted spectra REDUCED_X_SCI_PMOS FITS image 339s X Stokes parameter (and L) REDUCED_ERROR_X_SCI_PMOS FITS image 339s Error on X Stokes parameter REDUCED_NUL_X_SCI_PMOS FITS image 339s Null parameter for X REDUCED_ANGLE_SCI_PMOS FITS image 339s Direction of linear polarization REDUCED_ERROR_ANGLE_SCI_PMOS FITS 339s image Error on polarization direction UNMAPPED_SCI_PMOS 339s FITS image Sky subtracted scientific spectra MAPPED_SCI_PMOS 339s FITS image Rectified scientific spectra MAPPED_ALL_SCI_PMOS 339s FITS image Rectified science spectra with sky MAPPED_SKY_SCI_PMOS 339s FITS image Rectified sky spectra UNMAPPED_SKY_SCI_PMOS FITS 339s image Sky on CCD OBJECT_TABLE_SCI_PMOS FITS table Positions 339s of detected objects OBJECT_TABLE_POL_SCI_PMOS FITS table 339s Positions of real objects Only if the sky-alignment of the 339s wavelength solution is requested: DISP_COEFF_SCI_PMOS FITS 339s table Upgraded dispersion coefficients WAVELENGTH_MAP_SCI_PMOS 339s FITS image Upgraded wavelength map 339s 339s Parameters: 339s dispersion: Expected spectral dispersion (Angstrom/pixel) 339s (float; default: 0.0) 339s rebin: Rebin (pixel) (int; default: 1) 339s skyalign: Polynomial order for sky lines alignment, or -1 to 339s avoid alignment (int; default: 0) 339s wcolumn: Name of sky line catalog table column with 339s wavelengths (str; default: 'WLEN') 339s startwavelength: Start wavelength in spectral extraction (float; 339s default: 0.0) 339s endwavelength: End wavelength in spectral extraction (float; 339s default: 0.0) 339s flux: Apply flux conservation (bool; default: True) 339s flatfield: Apply flat field (bool; default: True) 339s skymedian: Sky subtraction from extracted slit spectra (bool; 339s default: False) 339s skylocal: Sky subtraction from CCD slit spectra (bool; 339s default: True) 339s cosmics: Eliminate cosmic rays hits (only if local sky 339s subtraction is also requested) (bool; default: 339s False) 339s slit_margin: Number of pixels to exclude at each slit in object 339s detection and extraction (int; default: 3) 339s ext_radius: Maximum extraction radius for detected objects 339s (pixel) (int; default: 12) 339s cont_radius: Minimum distance at which two objects of equal 339s luminosity do not contaminate each other (pixel) 339s (int; default: 0) 339s ext_mode: Object extraction method: 0 = aperture, 1 = Horne 339s optimal extraction (int; default: 1) 339s match_tolerance: Tolerance for matching spectra from the same object 339s at different angles and beams (pixel) (float; 339s default: 5.0) 339s time_normalise: Normalise output spectra by the exposure time (bool; 339s default: True) 339s chromatism: Chromatism correction to polarization angles (bool; 339s default: True) 339s wollaston: Wollaston mounting (FORS2 only): true = 0 degrees 339s (ord. beam on top, extr. beam on bottom), false = 339s 180 degrees (beams are reversed), for FORS1 is 339s frozen to true (bool; default: True) 339s qc: Compute QC1 parameters (bool; default: True) 339s Author: Carlo Izzo 339s 339s 339s Recipe fors_remove_bias: 339s version 5.5.7 339s Parameters: {} 339s Docstring: Subtract bias from input frame 339s 339s This recipe is used to subtract the overscan and master bias(produced 339s by the recipe fors_bias) from one raw data frame. The overscan 339s regions, if present, are used to compensate for variations of the 339s overall bias level between master bias and input raw frame. The 339s overscan regions are then trimmed from the result. The recipe should 339s allow any fors frame. Input files: DO category: 339s Type: Explanation: Required: ANY_CAT 339s Raw Raw data frame Y MASTER_BIAS 339s Calib Master bias frame Y Output files: DO category: 339s Data type: Explanation: ANY_CAT_UNBIAS FITS image Bias 339s subtracted frame 339s 339s No parameters 339s Author: Carlo Izzo 339s 339s 339s Recipe fors_resample: 339s version 5.5.7 339s Parameters: {'dispersion': 0.0, 'startwavelength': 0.0, 'endwavelength': 0.0, 'flux': True} 339s Docstring: Resample input spectra at constant wavelength step 339s 339s This recipe is used to resample at constant wavelength step spatially 339s rectified spectra. The input frames are produced using either the 339s recipe fors_extract_slits in the case of MOS/MXU multi slit exposures, 339s or the recipes fors_remove_bias and fors_flatfield in the case of LSS 339s or long-slit like MOS/MXU data. Only in case of LSS or LSS-like data 339s the SLIT_LOCATION table is required in input. Please refer to the FORS 339s Pipeline User's Manual for more details. In the table below the MXU 339s acronym can also be read as MOS and LSS, SCI can be read as STD, and 339s SCIENCE as STANDARD. Input files: DO category: Type: 339s Explanation: Required: LAMP_UNBIAS_MXU or 339s SCIENCE_UNBIAS_MXU or SCIENCE_UNFLAT_MXU or RECTIFIED_LAMP_MXU 339s or RECTIFIED_ALL_SCI_MXU or RECTIFIED_SCI_MXU or 339s RECTIFIED_SKY_SCI_MXU Calib Frame to resample Y 339s DISP_COEFF_MXU or DISP_COEFF_SCI_MXU Calib Dispersion 339s coefficients Y SLIT_LOCATION_MXU Calib Slit location 339s table Y GRISM_TABLE Calib Grism table 339s . Output files: DO category: Data type: 339s Explanation: MAPPED_LAMP_MXU or MAPPED_ALL_SCI_MXU or 339s MAPPED_SCI_MXU or MAPPED_SKY_SCI_MXU FITS image Resampled 339s spectra 339s 339s Parameters: 339s dispersion: Expected spectral dispersion (Angstrom/pixel) 339s (float; default: 0.0) 339s startwavelength: Start wavelength in spectral extraction (float; 339s default: 0.0) 339s endwavelength: End wavelength in spectral extraction (float; 339s default: 0.0) 339s flux: Apply flux conservation (bool; default: True) 339s Author: Carlo Izzo 339s 339s 339s Recipe fors_science: 339s version 5.5.7 339s Parameters: {'skyalign': -1, 'flatfield': True, 'skyglobal': False, 'skymedian': False, 'skylocal': True, 'cosmics': False, 'slit_margin': 3, 'ext_radius': 12, 'cont_radius': 0, 'ext_mode': 1, 'resp_fit_nknots': -2, 'resp_fit_degree': -2, 'resp_ignore_mode': 'stellar_absorption,telluric,command_line', 'resp_ignore_points': '', 'resp_use_flat_sed': 'grism_table', 'nonlinear_level': 60000.0, 'generate_idp': True} 339s Docstring: Extraction of scientific spectra 339s 339s This recipe is used to reduce scientific spectra using the extraction 339s mask and the products created by the recipe fors_calib. The spectra 339s are bias subtracted, flat fielded (if a normalised flat field is 339s specified) and remapped eliminating the optical distortions. The 339s wavelength calibration can be optionally upgraded using a number of 339s sky lines: if no sky lines catalog of wavelengths is specified, an 339s internal one is used instead. If the alignment to the sky lines is 339s performed, the input dispersion coefficients table is upgraded and 339s saved to disk, and a new CCD wavelengths map is created. This recipe 339s accepts both FORS1 and FORS2 frames. A grism table (typically 339s depending on the instrument mode, and in particular on the grism used) 339s may also be specified: this table contains a default recipe parameter 339s setting to control the way spectra are extracted for a specific 339s instrument mode, as it is used for automatic run of the pipeline on 339s Paranal and in Garching. If this table is specified, it will modify 339s the default recipe parameter setting, with the exception of those 339s parameters which have been explicitly modifyed on the command line. If 339s a grism table is not specified, the input recipe parameters values 339s will always be read from the command line, or from an esorex 339s configuration file if present, or from their generic default values 339s (that are rarely meaningful). In the table below the MXU acronym can 339s be read alternatively as MOS and LSS, depending on the instrument mode 339s of the input data. The acronym SCI on products should be read STD in 339s case of standard stars observations A CURV_COEFF table is not (yet) 339s expected for LSS data. Either a scientific or a standard star exposure 339s can be specified in input. Only in case of a standard star exposure 339s input, the atmospheric extinction table and a table with the physical 339s fluxes of the observed standard star must be specified in input, and a 339s spectro-photometric table is created in output. This table can then be 339s input again to this recipe, always with an atmospheric extinction 339s table, and if a photometric calibration is requested then flux 339s calibrated spectra (in units of erg/cm/cm/s/Angstrom) are also written 339s in output. Input files: DO category: Type: 339s Explanation: Required: SCIENCE_MXU Raw 339s Scientific exposure Y or STANDARD_MXU Raw 339s Standard star exposure Y MASTER_BIAS Calib 339s Master bias Y GRISM_TABLE Calib 339s Grism table . MASTER_SKYLINECAT Calib 339s Sky lines catalog . MASTER_NORM_FLAT_MXU Calib 339s Normalised flat field . DISP_COEFF_MXU Calib 339s Inverse dispersion Y CURV_COEFF_MXU Calib 339s Spectral curvature Y SLIT_LOCATION_MXU Calib 339s Slits positions table Y FLAT_SED_MXU Calib 339s Slits dispersion profile . or, in case of LSS-like MOS/MXU data, 339s MASTER_NORM_FLAT_LONG_MXU Calib Normalised flat field . 339s DISP_COEFF_LONG_MXU Calib Inverse dispersion Y 339s SLIT_LOCATION_LONG_MXU Calib Slits positions table Y 339s GLOBAL_DISTORTION_TABLE Calib Global distortion . 339s In case STANDARD_MXU is specified in input, EXTINCT_TABLE 339s Calib Atmospheric extinction Y STD_FLUX_TABLE 339s Calib Standard star flux Y TELLURIC_CONTAMINATION 339s Calib Telluric regions list . The following input files 339s are mandatory if photometric calibrated spectra are desired: 339s EXTINCT_TABLE Calib Atmospheric extinction Y 339s SPECPHOT_TABLE Calib Response curves Y 339s If requested for standard star data, the SPECPHOT_TABLE can be 339s dropped: in this case the correction is applied using the 339s SPECPHOT_TABLE produced in the same run. Output files: DO 339s category: Data type: Explanation: REDUCED_SCI_MXU 339s FITS image Extracted scientific spectra REDUCED_SKY_SCI_MXU 339s FITS image Extracted sky spectra REDUCED_ERROR_SCI_MXU FITS 339s image Errors on extracted spectra UNMAPPED_SCI_MXU FITS 339s image Sky subtracted scientific spectra MAPPED_SCI_MXU 339s FITS image Rectified scientific spectra MAPPED_ALL_SCI_MXU 339s FITS image Rectified science spectra with sky MAPPED_SKY_SCI_MXU 339s FITS image Rectified sky spectra UNMAPPED_SKY_SCI_MXU FITS 339s image Sky on CCD OBJECT_TABLE_SCI_MXU FITS table Positions 339s of detected objects Only if the global sky subtraction is 339s requested: GLOBAL_SKY_SPECTRUM_MXU FITS table Global sky 339s spectrum Only if the sky-alignment of the wavelength solution is 339s requested: SKY_SHIFTS_LONG_SCI_MXU FITS table Sky lines offsets 339s (LSS-like data) or SKY_SHIFTS_SLIT_SCI_MXU FITS table Sky lines 339s offsets (MOS-like data) DISP_COEFF_SCI_MXU FITS table 339s Upgraded dispersion coefficients WAVELENGTH_MAP_SCI_MXU FITS 339s image Upgraded wavelength map Only if a STANDARD_MXU is specified 339s in input: SPECPHOT_TABLE FITS table Efficiency and 339s response curves Only if a photometric calibration was requested: 339s REDUCED_FLUX_SCI_MXU FITS image Flux calibrated scientific 339s spectra REDUCED_FLUX_ERROR_SCI_MXU FITS image Errors on flux 339s calibrated spectra MAPPED_FLUX_SCI_MXU FITS image Flux 339s calibrated slit spectra 339s 339s Parameters: 339s skyalign: Polynomial order for sky lines alignment, or -1 339s to avoid alignment (int; default: -1) 339s flatfield: Apply flat field (bool; default: True) 339s skyglobal: Subtract global sky spectrum from CCD (bool; 339s default: False) 339s skymedian: Sky subtraction from extracted slit spectra 339s (bool; default: False) 339s skylocal: Sky subtraction from CCD slit spectra (bool; 339s default: True) 339s cosmics: Eliminate cosmic rays hits, only if either global 339s or local (not for LSS) sky subtraction is also 339s requested. (bool; default: False) 339s slit_margin: Number of pixels to exclude at each slit in 339s object detection and extraction (int; default: 3) 339s ext_radius: Maximum extraction radius for detected objects 339s (unbinned pixel) (int; default: 12) 339s cont_radius: Minimum distance at which two objects of equal 339s luminosity do not contaminate each other (pixel) 339s (int; default: 0) 339s ext_mode: Object extraction method: 0 = aperture, 1 = Horne 339s optimal extraction (int; default: 1) 339s resp_fit_nknots: Number of knots in spline fitting of the 339s instrument response. (-1: No fitting. -2: Read 339s from grism table) (int; default: -2) 339s resp_fit_degree: Degree of polynomial in fitting of the instrument 339s response. (-1: No fitting. -2: Read from grism 339s table) (int; default: -2) 339s resp_ignore_mode: Types of lines/regions to ignore in response. 339s Valid ones are 'stellar_absorption', 'telluric' 339s and 'command_line' (from parameter 339s resp_ignore_lines) (str; default: 339s 'stellar_absorption,telluric,command_line') 339s resp_ignore_points: Extra lines/regions to ignore in response. Use a 339s comma separated list of values. A range can be 339s specified like 4500.0-4600.0 (str; default: '') 339s resp_use_flat_sed: Use the flat SED to normalise the observed 339s spectra. Value are true, false, grism_table. 339s (str; default: 'grism_table') 339s nonlinear_level: Level above which the detector is not linear 339s (float; default: 60000.0) 339s generate_idp: Set to TRUE to request IDP generation (bool; 339s default: True) 339s Author: Carlo Izzo 339s 339s 339s Recipe fors_spec_mflat: 339s version 5.5.7 339s Parameters: {'smooth_sed': 0.0, 'stack_method': 'sum', 'klow': 3.0, 'khigh': 3.0, 'kiter': 999, 'nonlinear_level': 50000.0, 'max_nonlinear_ratio': 0.2} 339s Docstring: Computes master spectroscopic flat, removing bias first 339s 339s This recipe is used to subtract the master bias, produced by the 339s recipe fors_bias, from a set of raw flat field frames. The input raw 339s frames are summed, the master bias frame is rescaled accordingly, and 339s subtracted from the result. The overscan regions, if present, are used 339s to compensate for variations of the bias level between master bias and 339s input raw frames. The overscan regions are then trimmed from the 339s result. In the table below the MXU acronym can be alternatively read 339s as MOS and LSS. Input files: DO category: Type: 339s Explanation: Required: SCREEN_FLAT_MXU Raw 339s Raw data frame Y SLIT_LOCATION_MXU Calib 339s Slits positions on CCD Y CURV_COEFF_MXU Calib 339s Slits tracing fits Y DISP_COEFF_MXU Calib 339s Wavelength calibration Y MASTER_BIAS Calib 339s Master bias frame Y Output files: DO category: 339s Data type: Explanation: MASTER_SCREEN_FLAT_MXU FITS image Bias 339s subtracted sum frame 339s 339s Parameters: 339s smooth_sed: Smoothing size for each flat sed (float; 339s default: 0.0) 339s stack_method: Frames combination method (str; default: 'sum') 339s klow: Low threshold in ksigma method (float; default: 339s 3.0) 339s khigh: High threshold in ksigma method (float; default: 339s 3.0) 339s kiter: Max number of iterations in ksigma method (int; 339s default: 999) 339s nonlinear_level: Level above which the detector is not linear 339s (float; default: 50000.0) 339s max_nonlinear_ratio: Maximum allowed ratio of non-linear pixels per 339s slit (float; default: 0.2) 339s Author: Carlo Izzo 339s 339s 339s Recipe fors_subtract_sky: 339s version 5.5.7 339s Parameters: {'dispersion': 0.0, 'startwavelength': 0.0, 'endwavelength': 0.0, 'cosmics': False} 339s Docstring: Subtract sky from scientific spectra 339s 339s This recipe is used to subtract the sky emission from unrebinned slit 339s spectra. This is obtained by robust fitting (i.e., excluding the 339s signal from possible point-like objects in slit) of the emission along 339s the CCD columns within each spectrum). This method doesn't work if 339s extended objects are in slit (it really destroys the object spectra), 339s and is not applicable to LSS data. The input scientific frames are 339s produced by the recipes fors_remove_bias and fors_flatfield. This 339s recipe cannot be applied to LSS or long-slit like data (MOS/MXU with 339s all slits at the same offset). No automatic recipe is available for 339s this. Please refer to the FORS Pipeline User's Manual for more 339s details. In the table below the MXU acronym can be alternatively read 339s as MOS, and SCI as STD. Input files: DO category: 339s Type: Explanation: Required: SCIENCE_UNBIAS_MXU or 339s SCIENCE_UNFLAT_MXU or STANDARD_UNBIAS_MXU or STANDARD_UNFLAT_MXU 339s Calib Frame with sky lines Y CURV_COEFF_MXU 339s Calib Spectral curvature Y SLIT_LOCATION_MXU 339s Calib Slit location on CCD Y GRISM_TABLE 339s Calib Grism table . Output files: DO category: 339s Data type: Explanation: UNMAPPED_SCI_MXU or UNMAPPED_STD_MXU 339s FITS image Sky subtracted scientific frame UNMAPPED_SKY_SCI_MXU 339s or UNMAPPED_SKY_STD_MXU FITS image Subtracted sky frame 339s 339s Parameters: 339s dispersion: Expected spectral dispersion (Angstrom/pixel) 339s (float; default: 0.0) 339s startwavelength: Start wavelength in spectral extraction (float; 339s default: 0.0) 339s endwavelength: End wavelength in spectral extraction (float; 339s default: 0.0) 339s cosmics: Eliminate cosmic rays hits (bool; default: False) 339s Author: Carlo Izzo 339s 339s 339s Recipe fors_subtract_sky_lss: 339s version 5.5.7 339s Parameters: {} 339s Docstring: Subtract sky from calibrated long slit exposure 339s 339s This recipe is used to subtract the sky from wavelength calibrated 339s scientific spectra produced by the recipe fors_resample. A simple 339s median signal level is subtracted from each image column. In the table 339s below the MXU acronym can be read alternatively as MOS and LSS, 339s depending on the instrument mode of the input data. The acronym SCI 339s may be read STD in case of standard stars observations. Note that only 339s LSS or LSS-like MOS/MXU data are to be processed by this recipe. 339s Input files: DO category: Type: Explanation: 339s Required: MAPPED_ALL_SCI_MXU Raw Scientific exposure 339s Y Output files: DO category: Data type: 339s Explanation: MAPPED_SCI_MXU FITS image Rectified 339s scientific spectra MAPPED_SKY_SCI_MXU FITS image Rectified 339s sky spectra 339s 339s No parameters 339s Author: Carlo Izzo 339s 339s 339s Recipe fors_sumflux: 339s version 5.5.7 339s Parameters: {'xlow': 0, 'ylow': 0, 'xhigh': 0, 'yhigh': 0} 339s Docstring: Integrate flux from all or part of the input frame 339s 339s This recipe is used to monitor any lamp flux on the CCD. The input raw 339s image should be either a FLUX_ARC_LSS or a FLUX_FLAT_LSS frame. After 339s the background subtraction the total signal is integrated and divided 339s by the exposure time and by the total number of CCD original pixels 339s (keeping into account a possible rebinned readout). In the case of 339s FORS2 frames the background is the median level evaluated from the 339s available overscan regions. In the case of FORS1 data, where overscan 339s regions are missing, the background is evaluated as the median level 339s of the first 200 CCD columns for flat field data, while for arc lamp 339s data a background map evaluated from the regions without spectral 339s lines is computed and subtracted. The background subtracted frame is 339s written to output in all cases, and the QC parameters QC LAMP FLUX and 339s QC LAMP FLUXERR are computed. Input files: DO category: Type: 339s Explanation: Required: FLUX_FLAT_LSS Raw Flat 339s field exposure Y or FLUX_ARC_LSS Raw Arc lamp exposure 339s Y Output files: DO category: Data type: Explanation: 339s FLUX_LAMP_LSS FITS image Background subtracted integration region 339s 339s Parameters: 339s xlow: X coordinate of lower left corner of integration region 339s (pixel) (int; default: 0) 339s ylow: Y coordinate of lower left corner of integration region 339s (pixel) (int; default: 0) 339s xhigh: X coordinate of upper right corner of integration region 339s (pixel) (0 = CCD size) (int; default: 0) 339s yhigh: Y coordinate of upper right corner of integration region 339s (pixel) (0 = CCD size) (int; default: 0) 339s Author: Carlo Izzo 339s 339s 339s Recipe fors_trace_flat: 339s version 5.5.7 339s Parameters: {'dispersion': 0.0, 'startwavelength': 0.0, 'endwavelength': 0.0, 'cdegree': 0, 'cmode': 1} 339s Docstring: Determine spectral curvature model 339s 339s This recipe is used to trace the edges of MOS/MXU flat field slit 339s spectra and determine the spectral curvature solution. The input 339s master flat field image, product of the recipe fors_flat, is expected 339s to be oriented with horizontal dispersion direction and red 339s wavelengths on the right side. The input slits location table should 339s be the product of the recipe fors_detect_spectra. The input master 339s flat image is shifted one pixel down and is subtracted from the 339s original image. The result is a vertical gradient map. Next, the 339s negative values are forced positive, to obtain an absolute gradient 339s map. The map is passed with a horizontal median filter, and after that 339s the gradient peaks are traced starting from the slits positions listed 339s in the input slits location table. The number of pixels to the left 339s and to the right of the reference pixel is trivially derived from the 339s specified spectral range and spectral dispersion. The output spectral 339s curvature table contains the coefficients of the polynomial fitting of 339s the found traces, while the output trace table contains the traced 339s spectral edges positions in CCD (Y) coordinates for each spectrum, and 339s their comparison with their modeling. A spatial map is also created, 340s where to each CCD pixel is assigned the value of the spatial 340s coordinate along the slit (in pixel). For more details please refer to 340s the FORS Pipeline User's Manual. Note that specifying an input 340s GRISM_TABLE will set some of the recipe configuration parameters to 340s default values valid for a particular grism. Again, see the pipeline 340s manual for more details. In the table below the MXU acronym can be 340s alternatively read as MOS. Input files: DO category: 340s Type: Explanation: Required: MASTER_SCREEN_FLAT_MXU 340s Calib Master flat frame Y SLIT_LOCATION_DETECT_MXU 340s Calib Slits location Y GRISM_TABLE 340s Calib Grism table . Output files: DO category: 340s Data type: Explanation: CURV_TRACES_MXU FITS table Flat 340s field tracings CURV_COEFF_MXU FITS table Spectral 340s curvature table SPATIAL_MAP_MXU FITS image Map of 340s spatial coordinate 340s 340s Parameters: 340s dispersion: Expected spectral dispersion (Angstrom/pixel) 340s (float; default: 0.0) 340s startwavelength: Start wavelength in spectral extraction (float; 340s default: 0.0) 340s endwavelength: End wavelength in spectral extraction (float; 340s default: 0.0) 340s cdegree: Degree of spectral curvature polynomial (int; 340s default: 0) 340s cmode: Interpolation mode of curvature solution applicable 340s to MOS-like data (0 = no interpolation, 1 = fill 340s gaps, 2 = global model) (int; default: 1) 340s Author: Carlo Izzo 340s 340s 340s Recipe fors_wave_calib: 340s version 5.5.7 340s Parameters: {'dispersion': 0.0, 'peakdetection': 0.0, 'wdegree': 0, 'wradius': 4, 'wreject': 0.7, 'wcolumn': 'WLEN', 'startwavelength': 0.0, 'endwavelength': 0.0} 340s Docstring: Derive dispersion relation from rectified arc lamp frame 340s 340s This recipe is used to wavelength calibrate MOS/MXU slit spectra 340s contained in the rectified arc lamp exposure produced with recipe 340s fors_extract_slits. A pattern-matching algorithm is applied as in 340s recipe fors_detect_spectra. The input spatial map is used in the 340s production of the wavelength map. Use recipe fors_wave_calib_lss for 340s LSS data, or for MOS/MXU data where all slits have the same offset. 340s For more details on this data reduction strategy please refer to the 340s FORS Pipeline User's Manual. Note that specifying an input 340s GRISM_TABLE will set some of the recipe configuration parameters to 340s default values valid for a particular grism. In the table below the 340s MXU acronym can be alternatively read as MOS. Input files: DO 340s category: Type: Explanation: Required: 340s SPATIAL_MAP_MXU Calib Spatial map Y 340s RECTIFIED_LAMP_MXU Calib Rectified arc exposure Y 340s SLIT_LOCATION_MXU Calib Slit location table Y 340s CURV_COEFF_MXU Calib Spectral curvature Y 340s MASTER_LINECAT Calib Line catalog Y 340s GRISM_TABLE Calib Grism table . 340s Output files: DO category: Data type: Explanation: 340s REDUCED_LAMP_MXU FITS image Calibrated arc lamp exposure 340s DISP_COEFF_MXU FITS table Inverse dispersion coefficients 340s DISP_RESIDUALS_MXU FITS image Image of modeling residuals 340s WAVELENGTH_MAP_MXU FITS image Wavelengths mapped on CCD 340s SPECTRAL_RESOLUTION_MXU FITS table Spectral resolution table 340s 340s Parameters: 340s dispersion: Expected spectral dispersion (Angstrom/pixel) 340s (float; default: 0.0) 340s peakdetection: Initial peak detection threshold (ADU) (float; 340s default: 0.0) 340s wdegree: Degree of wavelength calibration polynomial (int; 340s default: 0) 340s wradius: Search radius if iterating pattern-matching with 340s first-guess method (int; default: 4) 340s wreject: Rejection threshold in dispersion relation fit 340s (pixel) (float; default: 0.7) 340s wcolumn: Name of line catalog table column with wavelengths 340s (str; default: 'WLEN') 340s startwavelength: Start wavelength in spectral extraction (float; 340s default: 0.0) 340s endwavelength: End wavelength in spectral extraction (float; 340s default: 0.0) 340s Author: Carlo Izzo 340s 340s 340s Recipe fors_wave_calib_lss: 340s version 5.5.7 340s Parameters: {'dispersion': 0.0, 'peakdetection': 0.0, 'wdegree': 0, 'wradius': 4, 'wreject': 0.7, 'wcolumn': 'WLEN', 'startwavelength': 0.0, 'endwavelength': 0.0, 'wmode': 2} 340s Docstring: Derive dispersion relation from long-slit arc lamp frame 340s 340s This recipe is used to wavelength calibrate one long slit spectrum, 340s i.e., a FORS spectral obtained either in LSS mode or in MOS/MXU mode 340s with all slits at the same offset. A pattern-matching algorithm is 340s applied as in recipe fors_detect_spectra. For more details on this 340s data reduction strategy please refer to the FORS Pipeline User's 340s Manual. Note that specifying an input GRISM_TABLE will set some of 340s the recipe configuration parameters to default values valid for a 340s particular grism. In the table below the LSS acronym can be 340s alternatively read as MOS or MXU. Input files: DO category: 340s Type: Explanation: Required: LAMP_UNBIAS_LSS 340s Calib Arc lamp exposure Y MASTER_LINECAT 340s Calib Line catalog Y GRISM_TABLE 340s Calib Grism table . Output files: DO category: 340s Data type: Explanation: REDUCED_LAMP_LSS FITS image 340s Calibrated arc lamp exposure DISP_COEFF_LSS FITS table 340s Inverse dispersion coefficients DISP_RESIDUALS_LSS FITS 340s image Image of modeling residuals WAVELENGTH_MAP_LSS FITS 340s image Wavelengths mapped on CCD SLIT_LOCATION_LSS FITS 340s image Background subtracted arc frame SPECTRAL_RESOLUTION_LSS 340s FITS table Spectral resolution table 340s 340s Parameters: 340s dispersion: Expected spectral dispersion (Angstrom/pixel) 340s (float; default: 0.0) 340s peakdetection: Initial peak detection threshold (ADU) (float; 340s default: 0.0) 340s wdegree: Degree of wavelength calibration polynomial (int; 340s default: 0) 340s wradius: Search radius if iterating pattern-matching with 340s first-guess method (int; default: 4) 340s wreject: Rejection threshold in dispersion relation fit 340s (pixel) (float; default: 0.7) 340s wcolumn: Name of line catalog table column with wavelengths 340s (str; default: 'WLEN') 340s startwavelength: Start wavelength in spectral extraction (float; 340s default: 0.0) 340s endwavelength: End wavelength in spectral extraction (float; 340s default: 0.0) 340s wmode: Interpolation mode of wavelength solution (0 = no 340s interpolation, 1 = fill gaps, 2 = global model) 340s (int; default: 2) 340s Author: Carlo Izzo 340s 340s 340s Recipe fors_zeropoint: 340s version 5.5.7 340s Parameters: {'sex_exe': '/usr/bin/source-extractor', 'sex_config': '/usr/share/cpl-plugins/fors-5.5.7/config/fors.sex', 'sex_mag': 'MAG_APER', 'sex_magerr': 'MAGERR_APER', 'sex_radius': 64, 'maxoffset': 150.0, 'magcutE': 1.0, 'magcutk': 5.0, 'magsyserr': 0.01} 340s Docstring: Compute zeropoint 340s 340s Input files: DO category: Type: Explanation: 340s Number: STANDARD_IMG FITS image Phot. standard field 340s 1 MASTER_BIAS FITS image Master bias 340s 1 MASTER_SKY_FLAT_IMG FITS image Master sky flatfield 340s 1 FLX_STD_IMG FITS table Standard star catalog 340s 1+ PHOT_TABLE FITS table Filter ext. coeff, color 340s 1 Output files: DO category: Data type: Explanation: 340s SOURCES_STD_IMG FITS image Unfiltered SExtractor output 340s ALIGNED_PHOT FITS table PHOT_BACKGROUND_STD_IMG 340s FITS image Reduced science image background STANDARD_REDUCED_IMG 340s FITS image Reduced std image 340s 340s Parameters: 340s sex_exe: SExtractor executable (str; default: '/usr/bin/source- 340s extractor') 340s sex_config: SExtractor configuration file (str; default: 340s '/usr/share/cpl- plugins/fors-5.5.7/config/fors.sex') 340s sex_mag: SExtractor magnitude (str; default: 'MAG_APER') 340s sex_magerr: SExtractor magnitude error (str; default: 'MAGERR_APER') 340s sex_radius: Background error map median filter radius (unbinned 340s pixels) (int; default: 64) 340s maxoffset: Maximum acceptable offset between the image and catalogue 340s WCS (pixels) (float; default: 150.0) 340s magcutE: Zeropoint absolute cutoff (magnitude) (float; default: 340s 1.0) 340s magcutk: Zeropoint kappa rejection parameter (float; default: 5.0) 340s magsyserr: Systematic error in magnitude (float; default: 0.01) 340s Author: Jonas M. Larsen 340s 340s 340s autopkgtest [01:05:03]: test test-recipe.py: -----------------------] 344s autopkgtest [01:05:07]: test test-recipe.py: - - - - - - - - - - results - - - - - - - - - - 344s test-recipe.py PASS (superficial) 348s autopkgtest [01:05:11]: @@@@@@@@@@@@@@@@@@@@ summary 348s test-recipe.py PASS (superficial)