0s autopkgtest [00:53:52]: starting date and time: 2024-04-19 00:53:52+0000 0s autopkgtest [00:53:52]: git checkout: 43bc6cdf gitlab-ci: do not include the salsa pipeline 0s autopkgtest [00:53:52]: host juju-7f2275-prod-proposed-migration-environment-2; command line: /home/ubuntu/autopkgtest/runner/autopkgtest --output-dir /tmp/autopkgtest-work.8vbqpp74/out --timeout-copy=6000 --setup-commands /home/ubuntu/autopkgtest-cloud/worker-config-production/setup-canonical.sh --apt-pocket=proposed=src:gsl --apt-upgrade cpl-plugin-vimos --timeout-short=300 --timeout-copy=20000 --timeout-build=20000 --env=ADT_TEST_TRIGGERS=gsl/2.7.1+dfsg-6ubuntu2 -- ssh -s /home/ubuntu/autopkgtest/ssh-setup/nova -- --flavor autopkgtest --security-groups autopkgtest-juju-7f2275-prod-proposed-migration-environment-2@bos03-arm64-11.secgroup --name adt-noble-arm64-cpl-plugin-vimos-20240419-005352-juju-7f2275-prod-proposed-migration-environment-2-077ad2d9-9559-44e8-8ffd-ddd1051f3534 --image adt/ubuntu-noble-arm64-server --keyname testbed-juju-7f2275-prod-proposed-migration-environment-2 --net-id=net_prod-proposed-migration -e TERM=linux -e ''"'"'http_proxy=http://squid.internal:3128'"'"'' -e ''"'"'https_proxy=http://squid.internal:3128'"'"'' -e ''"'"'no_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'"'"'' --mirror=http://ftpmaster.internal/ubuntu/ 383s Creating nova instance adt-noble-arm64-cpl-plugin-vimos-20240419-005352-juju-7f2275-prod-proposed-migration-environment-2-077ad2d9-9559-44e8-8ffd-ddd1051f3534 from image adt/ubuntu-noble-arm64-server-20240418.img (UUID c141647a-22ea-481a-97c5-a98894f31daa)... 383s nova boot failed (attempt #1): 383s DEBUG (extension:189) found extension EntryPoint.parse('v1password = swiftclient.authv1:PasswordLoader') 383s DEBUG (extension:189) found extension EntryPoint.parse('noauth = cinderclient.contrib.noauth:CinderNoAuthLoader') 383s DEBUG (extension:189) found extension EntryPoint.parse('admin_token = keystoneauth1.loading._plugins.admin_token:AdminToken') 383s DEBUG (extension:189) found extension EntryPoint.parse('none = keystoneauth1.loading._plugins.noauth:NoAuth') 383s DEBUG (extension:189) found extension EntryPoint.parse('password = keystoneauth1.loading._plugins.identity.generic:Password') 383s DEBUG (extension:189) found extension EntryPoint.parse('token = keystoneauth1.loading._plugins.identity.generic:Token') 383s DEBUG (extension:189) found extension EntryPoint.parse('v2password = keystoneauth1.loading._plugins.identity.v2:Password') 383s DEBUG (extension:189) found extension EntryPoint.parse('v2token = keystoneauth1.loading._plugins.identity.v2:Token') 383s DEBUG (extension:189) found extension EntryPoint.parse('v3adfspassword = keystoneauth1.extras._saml2._loading:ADFSPassword') 383s DEBUG (extension:189) found extension EntryPoint.parse('v3applicationcredential = keystoneauth1.loading._plugins.identity.v3:ApplicationCredential') 383s DEBUG (extension:189) found extension EntryPoint.parse('v3fedkerb = keystoneauth1.extras.kerberos._loading:MappedKerberos') 383s DEBUG (extension:189) found extension EntryPoint.parse('v3kerberos = keystoneauth1.extras.kerberos._loading:Kerberos') 383s DEBUG (extension:189) found extension EntryPoint.parse('v3multifactor = keystoneauth1.loading._plugins.identity.v3:MultiFactor') 383s DEBUG (extension:189) found extension EntryPoint.parse('v3oauth1 = keystoneauth1.extras.oauth1._loading:V3OAuth1') 383s DEBUG (extension:189) found extension EntryPoint.parse('v3oidcaccesstoken = keystoneauth1.loading._plugins.identity.v3:OpenIDConnectAccessToken') 383s DEBUG (extension:189) found extension EntryPoint.parse('v3oidcauthcode = keystoneauth1.loading._plugins.identity.v3:OpenIDConnectAuthorizationCode') 383s DEBUG (extension:189) found extension EntryPoint.parse('v3oidcclientcredentials = keystoneauth1.loading._plugins.identity.v3:OpenIDConnectClientCredentials') 383s DEBUG (extension:189) found extension EntryPoint.parse('v3oidcpassword = keystoneauth1.loading._plugins.identity.v3:OpenIDConnectPassword') 383s DEBUG (extension:189) found extension EntryPoint.parse('v3password = keystoneauth1.loading._plugins.identity.v3:Password') 383s DEBUG (extension:189) found extension EntryPoint.parse('v3samlpassword = keystoneauth1.extras._saml2._loading:Saml2Password') 383s DEBUG (extension:189) found extension EntryPoint.parse('v3token = keystoneauth1.loading._plugins.identity.v3:Token') 383s DEBUG (extension:189) found extension EntryPoint.parse('v3tokenlessauth = keystoneauth1.loading._plugins.identity.v3:TokenlessAuth') 383s DEBUG (extension:189) found extension EntryPoint.parse('v3totp = keystoneauth1.loading._plugins.identity.v3:TOTP') 383s DEBUG (session:517) REQ: curl -g -i -X GET https://keystone.ps6.canonical.com:5000/v3 -H "Accept: application/json" -H "User-Agent: nova keystoneauth1/4.0.0 python-requests/2.22.0 CPython/3.8.10" 383s DEBUG (connectionpool:962) Starting new HTTPS connection (1): keystone.ps6.canonical.com:5000 383s DEBUG (connectionpool:429) https://keystone.ps6.canonical.com:5000 "GET /v3 HTTP/1.1" 200 267 383s DEBUG (session:548) RESP: [200] Connection: Keep-Alive Content-Length: 267 Content-Type: application/json Date: Fri, 19 Apr 2024 00:54:14 GMT Keep-Alive: timeout=75, max=1000 Server: Apache/2.4.52 (Ubuntu) Vary: X-Auth-Token x-openstack-request-id: req-fcb62215-0363-4224-9c1b-4be84a19d0a9 383s DEBUG (session:580) RESP BODY: {"version": {"id": "v3.14", "status": "stable", "updated": "2020-04-07T00:00:00Z", "links": [{"rel": "self", "href": "https://keystone.ps6.canonical.com:5000/v3/"}], "media-types": [{"base": "application/json", "type": "application/vnd.openstack.identity-v3+json"}]}} 383s DEBUG (session:946) GET call to https://keystone.ps6.canonical.com:5000/v3 used request id req-fcb62215-0363-4224-9c1b-4be84a19d0a9 383s DEBUG (base:182) Making authentication request to https://keystone.ps6.canonical.com:5000/v3/auth/tokens 383s DEBUG (connectionpool:429) https://keystone.ps6.canonical.com:5000 "POST /v3/auth/tokens HTTP/1.1" 201 12445 383s DEBUG (base:187) {"token": {"methods": ["password"], "user": {"domain": {"id": "default", "name": "Default"}, "id": "369f50a481564a2c9433776a4ebd224d", "name": "prod-proposed-migration-arm64", "password_expires_at": null}, "audit_ids": ["d2Rt4cLLQMOM50rSg-q25Q"], "expires_at": "2024-04-20T00:54:15.000000Z", "issued_at": "2024-04-19T00:54:15.000000Z", "project": {"domain": {"id": "default", "name": "Default"}, "id": "bd8b3df3f03d43a0a9303b7c0434fdab", "name": "prod-proposed-migration-arm64_project"}, "is_domain": false, "roles": [{"id": "86bf3043974746c2bf52c2a9f362f986", "name": "reader"}, {"id": "15cf997650e345b7b21c02b5cdb7d84a", "name": "member"}], "is_admin_project": false, "catalog": [{"endpoints": [{"id": "213cdf38198c4581bd5b7d6d0836923b", "interface": "internal", "region_id": "prodstack6", "url": "https://radosgw-internal.ps6.canonical.com:443/", "region": "prodstack6"}, {"id": "67061eee26944a1a8009f9d07be19738", "interface": "public", "region_id": "prodstack6", "url": "https://radosgw.ps6.canonical.com:443/", "region": "prodstack6"}, {"id": "fc88c52c749a47d08a24a2c7efbde01b", "interface": "admin", "region_id": "prodstack6", "url": "https://radosgw-admin.ps6.canonical.com:443/", "region": "prodstack6"}], "id": "06e4714942634054bf9aa11715312b4e", "type": "s3", "name": "s3"}, {"endpoints": [{"id": "8aa44c94b63746bd9b37f1008ad55fa8", "interface": "admin", "region_id": "prodstack6", "url": "https://aodh-admin.ps6.canonical.com:8042", "region": "prodstack6"}, {"id": "92cf08a80a0242ebbca8ec893cf332b1", "interface": "public", "region_id": "prodstack6", "url": "https://aodh.ps6.canonical.com:8042", "region": "prodstack6"}, {"id": "d8139c6e11ae4edcb78981c12bd53212", "interface": "internal", "region_id": "prodstack6", "url": "https://aodh-internal.ps6.canonical.com:8042", "region": "prodstack6"}], "id": "2fb939b0b969435c8f0c5fa4edb4de94", "type": "alarming", "name": "aodh"}, {"endpoints": [{"id": "a49fcc80e658411885f88cdd8432a571", "interface": "internal", "region_id": "prodstack6", "url": "https://heat-internal.ps6.canonical.com:8000/v1", "region": "prodstack6"}, {"id": "b23866fddba8415885b06c064c34b94b", "interface": "public", "region_id": "prodstack6", "url": "https://heat.ps6.canonical.com:8000/v1", "region": "prodstack6"}, {"id": "f84ae55197f94b8392a678f35c82ca26", "interface": "admin", "region_id": "prodstack6", "url": "https://heat-admin.ps6.canonical.com:8000/v1", "region": "prodstack6"}], "id": "3d4b59f7dab644b2b527e8e96b697545", "type": "cloudformation", "name": "heat-cfn"}, {"endpoints": [{"id": "2e0143334c6241169f45f1c11970c6bc", "interface": "public", "region_id": "prodstack6", "url": "https://heat.ps6.canonical.com:8004/v1/bd8b3df3f03d43a0a9303b7c0434fdab", "region": "prodstack6"}, {"id": "5e19c32243c04a3faf1e5f9ab900c260", "interface": "internal", "region_id": "prodstack6", "url": "https://heat-internal.ps6.canonical.com:8004/v1/bd8b3df3f03d43a0a9303b7c0434fdab", "region": "prodstack6"}, {"id": "b3fc5c88ec8543a691fec75726b86967", "interface": "admin", "region_id": "prodstack6", "url": "https://heat-admin.ps6.canonical.com:8004/v1/bd8b3df3f03d43a0a9303b7c0434fdab", "region": "prodstack6"}], "id": "43b926205044476b8093b18d8ce0a9e4", "type": "orchestration", "name": "heat"}, {"endpoints": [{"id": "a47569b96e5b4146a312e4673504557c", "interface": "public", "region_id": "prodstack6", "url": "https://glance.ps6.canonical.com:9292", "region": "prodstack6"}, {"id": "bba35c4ab04f4114a2a34e65568537bd", "interface": "internal", "region_id": "prodstack6", "url": "https://glance-internal.ps6.canonical.com:9292", "region": "prodstack6"}, {"id": "ef769f1117c74a62a279131486c89628", "interface": "admin", "region_id": "prodstack6", "url": "https://glance-admin.ps6.canonical.com:9292", "region": "prodstack6"}], "id": "49de724549524bd78e9cd46a4477226f", "type": "image", "name": "glance"}, {"endpoints": [{"id": "a1a41e9a1e2d42e5b6cd5380cd1e21bf", "interface": "admin", "region_id": "prodstack6", "url": "https://cinder-admin.ps6.canonical.com:8776/v3/bd8b3df3f03d43a0a9303b7c0434fdab", "region": "prodstack6"}, {"id": "d2309a99724b4111827482c68a832c0c", "interface": "public", "region_id": "prodstack6", "url": "https://cinder.ps6.canonical.com:8776/v3/bd8b3df3f03d43a0a9303b7c0434fdab", "region": "prodstack6"}, {"id": "f8a02e3949ff42afa772eb5e74dbef9f", "interface": "internal", "region_id": "prodstack6", "url": "https://cinder-internal.ps6.canonical.com:8776/v3/bd8b3df3f03d43a0a9303b7c0434fdab", "region": "prodstack6"}], "id": "5bf6578a631349e3af4bf36d7adb18e1", "type": "volumev3", "name": "cinderv3"}, {"endpoints": [{"id": "01d84128f36444e9b01549b86bd69116", "interface": "admin", "region_id": "prodstack6", "url": "https://barbican-admin.ps6.canonical.com:9312", "region": "prodstack6"}, {"id": "0ce4a8777e0b40a88f7fc0f77e34a605", "interface": "public", "region_id": "prodstack6", "url": "https://barbican.ps6.canonical.com:9311", "region": "prodstack6"}, {"id": "f507ba49e4a7435cb330234217c92449", "interface": "internal", "region_id": "prodstack6", "url": "https://barbican-internal.ps6.canonical.com:9311", "region": "prodstack6"}], "id": "62cb1c3d9f6c45979c13516a6b3ff114", "type": "key-manager", "name": "barbican"}, {"endpoints": [{"id": "3cb6121bd8f14da8aa2fba7be823a2b4", "interface": "internal", "region_id": "prodstack6", "url": "https://neutron-internal.ps6.canonical.com:9696", "region": "prodstack6"}, {"id": "46ba11d133fe4e8f9e8f9097ba737682", "interface": "admin", "region_id": "prodstack6", "url": "https://neutron-admin.ps6.canonical.com:9696", "region": "prodstack6"}, {"id": "d872eb6aa23d40009165aa3dcdce3948", "interface": "public", "region_id": "prodstack6", "url": "https://neutron.ps6.canonical.com:9696", "region": "prodstack6"}], "id": "759cb6fdfbc146dd8b9d1ba444c4b9db", "type": "network", "name": "neutron"}, {"endpoints": [{"id": "4349d565f72446da9699269f85df5e8b", "interface": "internal", "region_id": "prodstack6", "url": "https://manila-internal.ps6.canonical.com:8786/v2/bd8b3df3f03d43a0a9303b7c0434fdab", "region": "prodstack6"}, {"id": "a483dcc58f5e415e9ec739c94474e609", "interface": "public", "region_id": "prodstack6", "url": "https://manila.ps6.canonical.com:8786/v2/bd8b3df3f03d43a0a9303b7c0434fdab", "region": "prodstack6"}, {"id": "c1f14236723e42878562d8dd63d5a6a0", "interface": "admin", "region_id": "prodstack6", "url": "https://manila-admin.ps6.canonical.com:8786/v2/bd8b3df3f03d43a0a9303b7c0434fdab", "region": "prodstack6"}], "id": "93fc4008035946deb1f433c2dd905a5d", "type": "sharev2", "name": "manilav2"}, {"endpoints": [{"id": "0fa148793c7249c8b187b6b4ff425731", "interface": "internal", "region_id": "prodstack6", "url": "https://radosgw-internal.ps6.canonical.com:443/swift/v1/AUTH_e4b04ca58d734ed0aa29e306adad4f79/simplestreams/data", "region": "prodstack6"}, {"id": "555ade266a6b4bcc81b6e5abf607aec5", "interface": "public", "region_id": "prodstack6", "url": "https://radosgw.ps6.canonical.com:443/swift/v1/AUTH_e4b04ca58d734ed0aa29e306adad4f79/simplestreams/data", "region": "prodstack6"}, {"id": "7dad1a7b1552465686424fc014463173", "interface": "admin", "region_id": "prodstack6", "url": "https://radosgw-admin.ps6.canonical.com:443/swift/simplestreams/data", "region": "prodstack6"}], "id": "977dd359af1a4fcc91a9daf4dc33b0f3", "type": "product-streams", "name": "image-stream"}, {"endpoints": [{"id": "12d30eabcdec4831bd15273d55b1cbab", "interface": "internal", "region_id": "prodstack6", "url": "https://manila-internal.ps6.canonical.com:8786/v1/bd8b3df3f03d43a0a9303b7c0434fdab", "region": "prodstack6"}, {"id": "29d35b2b483346479f1ff1a13604d50e", "interface": "admin", "region_id": "prodstack6", "url": "https://manila-admin.ps6.canonical.com:8786/v1/bd8b3df3f03d43a0a9303b7c0434fdab", "region": "prodstack6"}, {"id": "4aa1422b8f5945d8aed9ba6a8d670e5c", "interface": "public", "region_id": "prodstack6", "url": "https://manila.ps6.canonical.com:8786/v1/bd8b3df3f03d43a0a9303b7c0434fdab", "region": "prodstack6"}], "id": "ac5e4f28fa794cde99f1d7ffc1b664e5", "type": "share", "name": "manila"}, {"endpoints": [{"id": "c7db93d54a684d8caeae1d9e18a59118", "interface": "admin", "region_id": "prodstack6", "url": "https://nova-admin.ps6.canonical.com:8774/v2.1", "region": "prodstack6"}, {"id": "dd7a796f401b477f9f1b5bbc05747d8d", "interface": "public", "region_id": "prodstack6", "url": "https://nova.ps6.canonical.com:8774/v2.1", "region": "prodstack6"}, {"id": "e7ecb038d830462ea67b0b463af5e013", "interface": "internal", "region_id": "prodstack6", "url": "https://nova-internal.ps6.canonical.com:8774/v2.1", "region": "prodstack6"}], "id": "b4519af08e174d4a8333a2d14ac3ba3b", "type": "compute", "name": "nova"}, {"endpoints": [{"id": "02ef5b6154934ffd97d8b5b8e4d70d2a", "interface": "internal", "region_id": "prodstack6", "url": "https://radosgw-internal.ps6.canonical.com:443/swift/v1/AUTH_bd8b3df3f03d43a0a9303b7c0434fdab", "region": "prodstack6"}, {"id": "2741abe526e94842a4fa801423ba1ef0", "interface": "public", "region_id": "prodstack6", "url": "https://radosgw.ps6.canonical.com:443/swift/v1/AUTH_bd8b3df3f03d43a0a9303b7c0434fdab", "region": "prodstack6"}, {"id": "3742f9406c604516933d6fd8c29e0880", "interface": "admin", "region_id": "prodstack6", "url": "https://radosgw-admin.ps6.canonical.com:443/swift", "region": "prodstack6"}], "id": "c7f07a7b3b3c408c96200dfd1d1a0f6f", "type": "object-store", "name": "swift"}, {"endpoints": [{"id": "06d4ed6c160a43f2b7fa7f80ad1dc709", "interface": "internal", "region_id": "prodstack6", "url": "https://designate-internal.ps6.canonical.com:9001", "region": "prodstack6"}, {"id": "1e240624a50c4ca0aaa6ef63cbc94f1b", "interface": "admin", "region_id": "prodstack6", "url": "https://designate-admin.ps6.canonical.com:9001", "region": "prodstack6"}, {"id": "f94d7d17997a43fd9c63b34c43301c6e", "interface": "public", "region_id": "prodstack6", "url": "https://designate.ps6.canonical.com:9001", "region": "prodstack6"}], "id": "cf82013d63844fedbe96bcacb6bd1fef", "type": "dns", "name": "designate"}, {"endpoints": [{"id": "4a688340be464710bfa60bf3f88f41c4", "interface": "admin", "region_id": "prodstack6", "url": "https://gnocchi-admin.ps6.canonical.com:8041", "region": "prodstack6"}, {"id": "a5a95506c96d4716adb4efc3ac9051be", "interface": "public", "region_id": "prodstack6", "url": "https://gnocchi.ps6.canonical.com:8041", "region": "prodstack6"}, {"id": "eebc17a086834f8fa8bb6b35c8061a8c", "interface": "internal", "region_id": "prodstack6", "url": "https://gnocchi-internal.ps6.canonical.com:8041", "region": "prodstack6"}], "id": "d10589e854a446a5b852593f33f170a7", "type": "metric", "name": "gnocchi"}, {"endpoints": [{"id": "08f66df28d0f47f3bec12f29e06d85ac", "interface": "admin", "region_id": "prodstack6", "url": "https://keystone-admin.ps6.canonical.com:35357/v3", "region": "prodstack6"}, {"id": "46d270b45ceb42db902f4d241afa6a70", "interface": "public", "region_id": "prodstack6", "url": "https://keystone.ps6.canonical.com:5000/v3", "region": "prodstack6"}, {"id": "a4addee11d9349cfa46ec6660dbad947", "interface": "internal", "region_id": "prodstack6", "url": "https://keystone-internal.ps6.canonical.com:5000/v3", "region": "prodstack6"}], "id": "deb38a775a9b4e87a8de9e3eed779882", "type": "identity", "name": "keystone"}, {"endpoints": [{"id": "18b4af5f40664babb94e884c6a53ccf3", "interface": "admin", "region_id": "prodstack6", "url": "https://octavia-admin.ps6.canonical.com:9876", "region": "prodstack6"}, {"id": "2b6f7ba7f9944ee1aebd6dccc5223b2d", "interface": "internal", "region_id": "prodstack6", "url": "https://octavia-internal.ps6.canonical.com:9876", "region": "prodstack6"}, {"id": "5e3012e9c79e4890be4d964b6208f5c6", "interface": "public", "region_id": "prodstack6", "url": "https://octavia.ps6.canonical.com:9876", "region": "prodstack6"}], "id": "e00337be20d54948b66a1c3109b885c6", "type": "load-balancer", "name": "octavia"}, {"endpoints": [{"id": "2d2942b35f3041389ad810f679d02f22", "interface": "public", "region_id": "prodstack6", "url": "https://placement.ps6.canonical.com:8778", "region": "prodstack6"}, {"id": "2e3beaac7ac14284b72e2592820ad725", "interface": "admin", "region_id": "prodstack6", "url": "https://placement-admin.ps6.canonical.com:8778", "region": "prodstack6"}, {"id": "91060f6df9ae444f81808adf40540d94", "interface": "internal", "region_id": "prodstack6", "url": "https://placement-internal.ps6.canonical.com:8778", "region": "prodstack6"}], "id": "edc6e37f154f4c0ab3dd4d52b82bf873", "type": "placement", "name": "placement"}]}} 383s REQ: curl -g -i -X GET https://nova.ps6.canonical.com:8774/v2.1 -H "Accept: application/json" -H "User-Agent: python-novaclient" -H "X-Auth-Token: {SHA256}94c7f566cdf46380775b90c73cb848c0b2469a4183e0dae112754566510620b1" 383s DEBUG (session:517) REQ: curl -g -i -X GET https://nova.ps6.canonical.com:8774/v2.1 -H "Accept: application/json" -H "User-Agent: python-novaclient" -H "X-Auth-Token: {SHA256}94c7f566cdf46380775b90c73cb848c0b2469a4183e0dae112754566510620b1" 383s DEBUG (connectionpool:962) Starting new HTTPS connection (1): nova.ps6.canonical.com:8774 383s DEBUG (connectionpool:429) https://nova.ps6.canonical.com:8774 "GET /v2.1 HTTP/1.1" 302 0 383s RESP: [302] Connection: Keep-Alive Content-Length: 0 Content-Type: text/plain; charset=utf8 Date: Fri, 19 Apr 2024 00:54:15 GMT Keep-Alive: timeout=75, max=1000 Location: https://nova.ps6.canonical.com:8774/v2.1/ Server: Apache/2.4.52 (Ubuntu) x-compute-request-id: req-76ac90af-16bf-47e7-a58d-ea64cab7395d x-openstack-request-id: req-76ac90af-16bf-47e7-a58d-ea64cab7395d 383s DEBUG (session:548) RESP: [302] Connection: Keep-Alive Content-Length: 0 Content-Type: text/plain; charset=utf8 Date: Fri, 19 Apr 2024 00:54:15 GMT Keep-Alive: timeout=75, max=1000 Location: https://nova.ps6.canonical.com:8774/v2.1/ Server: Apache/2.4.52 (Ubuntu) x-compute-request-id: req-76ac90af-16bf-47e7-a58d-ea64cab7395d x-openstack-request-id: req-76ac90af-16bf-47e7-a58d-ea64cab7395d 383s RESP BODY: Omitted, Content-Type is set to text/plain; charset=utf8. Only application/json responses have their bodies logged. 383s DEBUG (session:580) RESP BODY: Omitted, Content-Type is set to text/plain; charset=utf8. Only application/json responses have their bodies logged. 383s DEBUG (connectionpool:429) https://nova.ps6.canonical.com:8774 "GET /v2.1/ HTTP/1.1" 200 397 383s RESP: [200] Connection: Keep-Alive Content-Length: 397 Content-Type: application/json Date: Fri, 19 Apr 2024 00:54:15 GMT Keep-Alive: timeout=75, max=999 OpenStack-API-Version: compute 2.1 Server: Apache/2.4.52 (Ubuntu) Vary: OpenStack-API-Version,X-OpenStack-Nova-API-Version X-OpenStack-Nova-API-Version: 2.1 x-compute-request-id: req-68ebfaec-9bf5-441f-9b6c-30e88f994c66 x-openstack-request-id: req-68ebfaec-9bf5-441f-9b6c-30e88f994c66 383s DEBUG (session:548) RESP: [200] Connection: Keep-Alive Content-Length: 397 Content-Type: application/json Date: Fri, 19 Apr 2024 00:54:15 GMT Keep-Alive: timeout=75, max=999 OpenStack-API-Version: compute 2.1 Server: Apache/2.4.52 (Ubuntu) Vary: OpenStack-API-Version,X-OpenStack-Nova-API-Version X-OpenStack-Nova-API-Version: 2.1 x-compute-request-id: req-68ebfaec-9bf5-441f-9b6c-30e88f994c66 x-openstack-request-id: req-68ebfaec-9bf5-441f-9b6c-30e88f994c66 383s RESP BODY: {"version": {"id": "v2.1", "status": "CURRENT", "version": "2.90", "min_version": "2.1", "updated": "2013-07-23T11:33:21Z", "links": [{"rel": "self", "href": "https://nova.ps6.canonical.com:8774/v2.1/"}, {"rel": "describedby", "type": "text/html", "href": "http://docs.openstack.org/"}], "media-types": [{"base": "application/json", "type": "application/vnd.openstack.compute+json;version=2.1"}]}} 383s DEBUG (session:580) RESP BODY: {"version": {"id": "v2.1", "status": "CURRENT", "version": "2.90", "min_version": "2.1", "updated": "2013-07-23T11:33:21Z", "links": [{"rel": "self", "href": "https://nova.ps6.canonical.com:8774/v2.1/"}, {"rel": "describedby", "type": "text/html", "href": "http://docs.openstack.org/"}], "media-types": [{"base": "application/json", "type": "application/vnd.openstack.compute+json;version=2.1"}]}} 383s GET call to compute for https://nova.ps6.canonical.com:8774/v2.1/ used request id req-68ebfaec-9bf5-441f-9b6c-30e88f994c66 383s DEBUG (session:936) GET call to compute for https://nova.ps6.canonical.com:8774/v2.1/ used request id req-68ebfaec-9bf5-441f-9b6c-30e88f994c66 383s DEBUG (extension:189) found extension EntryPoint.parse('v1password = swiftclient.authv1:PasswordLoader') 383s DEBUG (extension:189) found extension EntryPoint.parse('noauth = cinderclient.contrib.noauth:CinderNoAuthLoader') 383s DEBUG (extension:189) found extension EntryPoint.parse('admin_token = keystoneauth1.loading._plugins.admin_token:AdminToken') 383s DEBUG (extension:189) found extension EntryPoint.parse('none = keystoneauth1.loading._plugins.noauth:NoAuth') 383s DEBUG (extension:189) found extension EntryPoint.parse('password = keystoneauth1.loading._plugins.identity.generic:Password') 383s DEBUG (extension:189) found extension EntryPoint.parse('token = keystoneauth1.loading._plugins.identity.generic:Token') 383s DEBUG (extension:189) found extension EntryPoint.parse('v2password = keystoneauth1.loading._plugins.identity.v2:Password') 383s DEBUG (extension:189) found extension EntryPoint.parse('v2token = keystoneauth1.loading._plugins.identity.v2:Token') 383s DEBUG (extension:189) found extension EntryPoint.parse('v3adfspassword = keystoneauth1.extras._saml2._loading:ADFSPassword') 383s DEBUG (extension:189) found extension EntryPoint.parse('v3applicationcredential = keystoneauth1.loading._plugins.identity.v3:ApplicationCredential') 383s DEBUG (extension:189) found extension EntryPoint.parse('v3fedkerb = keystoneauth1.extras.kerberos._loading:MappedKerberos') 383s DEBUG (extension:189) found extension EntryPoint.parse('v3kerberos = keystoneauth1.extras.kerberos._loading:Kerberos') 383s DEBUG (extension:189) found extension EntryPoint.parse('v3multifactor = keystoneauth1.loading._plugins.identity.v3:MultiFactor') 383s DEBUG (extension:189) found extension EntryPoint.parse('v3oauth1 = keystoneauth1.extras.oauth1._loading:V3OAuth1') 383s DEBUG (extension:189) found extension EntryPoint.parse('v3oidcaccesstoken = keystoneauth1.loading._plugins.identity.v3:OpenIDConnectAccessToken') 383s DEBUG (extension:189) found extension EntryPoint.parse('v3oidcauthcode = keystoneauth1.loading._plugins.identity.v3:OpenIDConnectAuthorizationCode') 383s DEBUG (extension:189) found extension EntryPoint.parse('v3oidcclientcredentials = keystoneauth1.loading._plugins.identity.v3:OpenIDConnectClientCredentials') 383s DEBUG (extension:189) found extension EntryPoint.parse('v3oidcpassword = keystoneauth1.loading._plugins.identity.v3:OpenIDConnectPassword') 383s DEBUG (extension:189) found extension EntryPoint.parse('v3password = keystoneauth1.loading._plugins.identity.v3:Password') 383s DEBUG (extension:189) found extension EntryPoint.parse('v3samlpassword = keystoneauth1.extras._saml2._loading:Saml2Password') 383s DEBUG (extension:189) found extension EntryPoint.parse('v3token = keystoneauth1.loading._plugins.identity.v3:Token') 383s DEBUG (extension:189) found extension EntryPoint.parse('v3tokenlessauth = keystoneauth1.loading._plugins.identity.v3:TokenlessAuth') 383s DEBUG (extension:189) found extension EntryPoint.parse('v3totp = keystoneauth1.loading._plugins.identity.v3:TOTP') 383s DEBUG (session:517) REQ: curl -g -i -X GET https://glance.ps6.canonical.com:9292/v2/images/c141647a-22ea-481a-97c5-a98894f31daa -H "Accept: application/json" -H "OpenStack-API-Version: compute 2.87" -H "User-Agent: python-novaclient" -H "X-Auth-Token: {SHA256}94c7f566cdf46380775b90c73cb848c0b2469a4183e0dae112754566510620b1" -H "X-OpenStack-Nova-API-Version: 2.87" 383s DEBUG (connectionpool:962) Starting new HTTPS connection (1): glance.ps6.canonical.com:9292 383s DEBUG (connectionpool:429) https://glance.ps6.canonical.com:9292 "GET /v2/images/c141647a-22ea-481a-97c5-a98894f31daa HTTP/1.1" 200 1935 383s DEBUG (session:548) RESP: [200] Connection: Keep-Alive Content-Length: 1935 Content-Type: application/json Date: Fri, 19 Apr 2024 00:54:15 GMT Keep-Alive: timeout=75, max=1000 Server: Apache/2.4.52 (Ubuntu) X-Openstack-Request-Id: req-1389a4d4-e4d4-440d-a05b-49138a24587b 383s DEBUG (session:580) RESP BODY: {"base_image_ref": "09c3944a-cd0d-425d-b22f-cde7ec51d155", "boot_roles": "reader,member", "hw_cdrom_bus": "scsi", "hw_disk_bus": "virtio", "hw_machine_type": "virt", "hw_video_model": "virtio", "hw_vif_model": "virtio", "image_location": "snapshot", "image_state": "available", "image_type": "snapshot", "instance_uuid": "b24dd948-363c-48e6-9b86-facf7c9fed82", "owner_id": "bd8b3df3f03d43a0a9303b7c0434fdab", "owner_project_name": "prod-proposed-migration-arm64_project", "owner_specified.openstack.md5": "087a26f2222dab8516c553374a9d1b4d", "owner_specified.openstack.object": "images/adt/ubuntu-noble-arm64-server-20240201.img", "owner_specified.openstack.sha256": "095b278df09de76f01843de514daf3f8eb0a0cc67fee4b3491161913153619db", "owner_user_name": "prod-proposed-migration-arm64", "user_id": "369f50a481564a2c9433776a4ebd224d", "name": "adt/ubuntu-noble-arm64-server-20240418.img", "disk_format": "qcow2", "container_format": "bare", "visibility": "private", "size": 3170828288, "virtual_size": 21474836480, "status": "active", "checksum": "967949a536f30e3b8dc5d8cd9f3bec76", "protected": false, "min_ram": 0, "min_disk": 20, "owner": "bd8b3df3f03d43a0a9303b7c0434fdab", "os_hidden": false, "os_hash_algo": "sha512", "os_hash_value": "57e1f3354039df20b36b8bae25d7504332874d1d2e1f3f4884ae05b01c7b63aec485fff63fc4f12db0f6ee937345a90fc8b6c98041119c33bd2f765f11b329a4", "id": "c141647a-22ea-481a-97c5-a98894f31daa", "created_at": "2024-04-18T13:38:39Z", "updated_at": "2024-04-18T13:39:25Z", "locations": [{"url": "rbd://eea9d068-c18c-11ed-8dc0-013aacb71b80/glance/c141647a-22ea-481a-97c5-a98894f31daa/snap", "metadata": {"store": "ceph"}}], "direct_url": "rbd://eea9d068-c18c-11ed-8dc0-013aacb71b80/glance/c141647a-22ea-481a-97c5-a98894f31daa/snap", "tags": [], "self": "/v2/images/c141647a-22ea-481a-97c5-a98894f31daa", "file": "/v2/images/c141647a-22ea-481a-97c5-a98894f31daa/file", "schema": "/v2/schemas/image", "stores": "ceph"} 383s DEBUG (session:936) GET call to image for https://glance.ps6.canonical.com:9292/v2/images/c141647a-22ea-481a-97c5-a98894f31daa used request id req-1389a4d4-e4d4-440d-a05b-49138a24587b 383s DEBUG (session:517) REQ: curl -g -i -X GET https://nova.ps6.canonical.com:8774/v2.1/flavors/autopkgtest -H "Accept: application/json" -H "OpenStack-API-Version: compute 2.87" -H "User-Agent: python-novaclient" -H "X-Auth-Token: {SHA256}94c7f566cdf46380775b90c73cb848c0b2469a4183e0dae112754566510620b1" -H "X-OpenStack-Nova-API-Version: 2.87" 383s DEBUG (connectionpool:429) https://nova.ps6.canonical.com:8774 "GET /v2.1/flavors/autopkgtest HTTP/1.1" 404 84 383s DEBUG (session:548) RESP: [404] Connection: Keep-Alive Content-Length: 84 Content-Type: application/json; charset=UTF-8 Date: Fri, 19 Apr 2024 00:54:15 GMT Keep-Alive: timeout=75, max=998 OpenStack-API-Version: compute 2.87 Server: Apache/2.4.52 (Ubuntu) Vary: OpenStack-API-Version,X-OpenStack-Nova-API-Version X-OpenStack-Nova-API-Version: 2.87 x-compute-request-id: req-e7bdd4bf-0309-4421-9ac2-eb32fb77ddc4 x-openstack-request-id: req-e7bdd4bf-0309-4421-9ac2-eb32fb77ddc4 383s DEBUG (session:580) RESP BODY: {"itemNotFound": {"code": 404, "message": "Flavor autopkgtest could not be found."}} 383s DEBUG (session:936) GET call to compute for https://nova.ps6.canonical.com:8774/v2.1/flavors/autopkgtest used request id req-e7bdd4bf-0309-4421-9ac2-eb32fb77ddc4 383s DEBUG (session:517) REQ: curl -g -i -X GET https://nova.ps6.canonical.com:8774/v2.1/flavors?is_public=None -H "Accept: application/json" -H "OpenStack-API-Version: compute 2.87" -H "User-Agent: python-novaclient" -H "X-Auth-Token: {SHA256}94c7f566cdf46380775b90c73cb848c0b2469a4183e0dae112754566510620b1" -H "X-OpenStack-Nova-API-Version: 2.87" 383s DEBUG (connectionpool:429) https://nova.ps6.canonical.com:8774 "GET /v2.1/flavors?is_public=None HTTP/1.1" 200 1739 383s DEBUG (session:548) RESP: [200] Connection: Keep-Alive Content-Length: 1739 Content-Type: application/json Date: Fri, 19 Apr 2024 00:54:15 GMT Keep-Alive: timeout=75, max=997 OpenStack-API-Version: compute 2.87 Server: Apache/2.4.52 (Ubuntu) Vary: OpenStack-API-Version,X-OpenStack-Nova-API-Version X-OpenStack-Nova-API-Version: 2.87 x-compute-request-id: req-8fd8884d-b3fa-4b90-92fd-0b45d9a770a9 x-openstack-request-id: req-8fd8884d-b3fa-4b90-92fd-0b45d9a770a9 383s DEBUG (session:580) RESP BODY: {"flavors": [{"id": "062428d9-35a1-461f-a33a-38436ed516b4", "name": "autopkgtest-cpu8-ram16-disk160-arm64", "links": [{"rel": "self", "href": "https://nova.ps6.canonical.com:8774/v2.1/flavors/062428d9-35a1-461f-a33a-38436ed516b4"}, {"rel": "bookmark", "href": "https://nova.ps6.canonical.com:8774/flavors/062428d9-35a1-461f-a33a-38436ed516b4"}], "description": null}, {"id": "8d27c5f0-65c7-4018-b3f7-50463875ab09", "name": "autopkgtest", "links": [{"rel": "self", "href": "https://nova.ps6.canonical.com:8774/v2.1/flavors/8d27c5f0-65c7-4018-b3f7-50463875ab09"}, {"rel": "bookmark", "href": "https://nova.ps6.canonical.com:8774/flavors/8d27c5f0-65c7-4018-b3f7-50463875ab09"}], "description": null}, {"id": "8ebe34fb-1390-4cc7-bbe5-0d38c80f2fb4", "name": "autopkgtest-cpu2-ram4-disk20-arm64", "links": [{"rel": "self", "href": "https://nova.ps6.canonical.com:8774/v2.1/flavors/8ebe34fb-1390-4cc7-bbe5-0d38c80f2fb4"}, {"rel": "bookmark", "href": "https://nova.ps6.canonical.com:8774/flavors/8ebe34fb-1390-4cc7-bbe5-0d38c80f2fb4"}], "description": null}, {"id": "a8256f9e-53ee-4584-ad7f-60e088825b83", "name": "autopkgtest-big", "links": [{"rel": "self", "href": "https://nova.ps6.canonical.com:8774/v2.1/flavors/a8256f9e-53ee-4584-ad7f-60e088825b83"}, {"rel": "bookmark", "href": "https://nova.ps6.canonical.com:8774/flavors/a8256f9e-53ee-4584-ad7f-60e088825b83"}], "description": null}, {"id": "cfc564ac-9f6e-4477-91c4-a89ccb4b744e", "name": "autopkgtest-cpu4-ram8-disk100-arm64", "links": [{"rel": "self", "href": "https://nova.ps6.canonical.com:8774/v2.1/flavors/cfc564ac-9f6e-4477-91c4-a89ccb4b744e"}, {"rel": "bookmark", "href": "https://nova.ps6.canonical.com:8774/flavors/cfc564ac-9f6e-4477-91c4-a89ccb4b744e"}], "description": null}]} 383s DEBUG (session:936) GET call to compute for https://nova.ps6.canonical.com:8774/v2.1/flavors?is_public=None used request id req-8fd8884d-b3fa-4b90-92fd-0b45d9a770a9 383s DEBUG (session:517) REQ: curl -g -i -X GET https://nova.ps6.canonical.com:8774/v2.1/flavors/8d27c5f0-65c7-4018-b3f7-50463875ab09 -H "Accept: application/json" -H "OpenStack-API-Version: compute 2.87" -H "User-Agent: python-novaclient" -H "X-Auth-Token: {SHA256}94c7f566cdf46380775b90c73cb848c0b2469a4183e0dae112754566510620b1" -H "X-OpenStack-Nova-API-Version: 2.87" 383s DEBUG (connectionpool:429) https://nova.ps6.canonical.com:8774 "GET /v2.1/flavors/8d27c5f0-65c7-4018-b3f7-50463875ab09 HTTP/1.1" 200 613 383s DEBUG (session:548) RESP: [200] Connection: Keep-Alive Content-Length: 613 Content-Type: application/json Date: Fri, 19 Apr 2024 00:54:16 GMT Keep-Alive: timeout=75, max=996 OpenStack-API-Version: compute 2.87 Server: Apache/2.4.52 (Ubuntu) Vary: OpenStack-API-Version,X-OpenStack-Nova-API-Version X-OpenStack-Nova-API-Version: 2.87 x-compute-request-id: req-fce4f8b3-1b04-4543-93ac-6ac643f341b7 x-openstack-request-id: req-fce4f8b3-1b04-4543-93ac-6ac643f341b7 383s DEBUG (session:580) RESP BODY: {"flavor": {"id": "8d27c5f0-65c7-4018-b3f7-50463875ab09", "name": "autopkgtest", "ram": 4096, "disk": 20, "swap": 0, "OS-FLV-EXT-DATA:ephemeral": 0, "OS-FLV-DISABLED:disabled": false, "vcpus": 2, "os-flavor-access:is_public": false, "rxtx_factor": 1.0, "links": [{"rel": "self", "href": "https://nova.ps6.canonical.com:8774/v2.1/flavors/8d27c5f0-65c7-4018-b3f7-50463875ab09"}, {"rel": "bookmark", "href": "https://nova.ps6.canonical.com:8774/flavors/8d27c5f0-65c7-4018-b3f7-50463875ab09"}], "description": null, "extra_specs": {"aggregate_instance_extra_specs:commit": "builder-arm64", "hw_rng:allowed": "True"}}} 383s DEBUG (session:936) GET call to compute for https://nova.ps6.canonical.com:8774/v2.1/flavors/8d27c5f0-65c7-4018-b3f7-50463875ab09 used request id req-fce4f8b3-1b04-4543-93ac-6ac643f341b7 383s DEBUG (session:517) REQ: curl -g -i -X POST https://nova.ps6.canonical.com:8774/v2.1/servers -H "Accept: application/json" -H "Content-Type: application/json" -H "OpenStack-API-Version: compute 2.87" -H "User-Agent: python-novaclient" -H "X-Auth-Token: {SHA256}94c7f566cdf46380775b90c73cb848c0b2469a4183e0dae112754566510620b1" -H "X-OpenStack-Nova-API-Version: 2.87" -d '{"server": {"name": "adt-noble-arm64-cpl-plugin-vimos-20240419-005352-juju-7f2275-prod-proposed-migration-environment-2-077ad2d9-9559-44e8-8ffd-ddd1051f3534", "imageRef": "c141647a-22ea-481a-97c5-a98894f31daa", "flavorRef": "8d27c5f0-65c7-4018-b3f7-50463875ab09", "user_data": "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", "key_name": "testbed-juju-7f2275-prod-proposed-migration-environment-2", "min_count": 1, "max_count": 1, "security_groups": [{"name": "autopkgtest-juju-7f2275-prod-proposed-migration-environment-2@bos03-arm64-11.secgroup"}], "networks": [{"uuid": "6ea4839c-9760-4b54-ab7d-70a6312667d1"}]}}' 383s DEBUG (connectionpool:429) https://nova.ps6.canonical.com:8774 "POST /v2.1/servers HTTP/1.1" 403 115 383s DEBUG (session:548) RESP: [403] Connection: Keep-Alive Content-Length: 115 Content-Type: application/json; charset=UTF-8 Date: Fri, 19 Apr 2024 00:54:16 GMT Keep-Alive: timeout=75, max=995 OpenStack-API-Version: compute 2.87 Server: Apache/2.4.52 (Ubuntu) Vary: OpenStack-API-Version,X-OpenStack-Nova-API-Version X-OpenStack-Nova-API-Version: 2.87 x-compute-request-id: req-e72f26d3-e511-40cc-a220-dca47df1db14 x-openstack-request-id: req-e72f26d3-e511-40cc-a220-dca47df1db14 383s DEBUG (session:580) RESP BODY: {"forbidden": {"code": 403, "message": "Quota exceeded for cores: Requested 2, but already used 210 of 210 cores"}} 383s DEBUG (session:936) POST call to compute for https://nova.ps6.canonical.com:8774/v2.1/servers used request id req-e72f26d3-e511-40cc-a220-dca47df1db14 383s DEBUG (shell:822) Quota exceeded for cores: Requested 2, but already used 210 of 210 cores (HTTP 403) (Request-ID: req-e72f26d3-e511-40cc-a220-dca47df1db14) 383s Traceback (most recent call last): 383s File "/usr/lib/python3/dist-packages/novaclient/shell.py", line 820, in main 383s OpenStackComputeShell().main(argv) 383s File "/usr/lib/python3/dist-packages/novaclient/shell.py", line 742, in main 383s args.func(self.cs, args) 383s File "/usr/lib/python3/dist-packages/novaclient/v2/shell.py", line 971, in do_boot 383s server = cs.servers.create(*boot_args, **boot_kwargs) 383s File "/usr/lib/python3/dist-packages/novaclient/v2/servers.py", line 1477, in create 383s return self._boot(response_key, *boot_args, **boot_kwargs) 383s File "/usr/lib/python3/dist-packages/novaclient/v2/servers.py", line 836, in _boot 383s return self._create('/servers', body, response_key, 383s File "/usr/lib/python3/dist-packages/novaclient/base.py", line 363, in _create 383s resp, body = self.api.client.post(url, body=body) 383s File "/usr/lib/python3/dist-packages/keystoneauth1/adapter.py", line 392, in post 383s return self.request(url, 'POST', **kwargs) 383s File "/usr/lib/python3/dist-packages/novaclient/client.py", line 78, in request 383s raise exceptions.from_response(resp, body, url, method) 383s novaclient.exceptions.Forbidden: Quota exceeded for cores: Requested 2, but already used 210 of 210 cores (HTTP 403) (Request-ID: req-e72f26d3-e511-40cc-a220-dca47df1db14) 383s ERROR (Forbidden): Quota exceeded for cores: Requested 2, but already used 210 of 210 cores (HTTP 403) (Request-ID: req-e72f26d3-e511-40cc-a220-dca47df1db14) 386s autopkgtest [01:00:18]: testbed dpkg architecture: arm64 386s autopkgtest [01:00:18]: testbed apt version: 2.7.14build2 386s autopkgtest [01:00:18]: @@@@@@@@@@@@@@@@@@@@ test bed setup 387s Get:1 http://ftpmaster.internal/ubuntu noble-proposed InRelease [117 kB] 387s Get:2 http://ftpmaster.internal/ubuntu noble-proposed/main Sources [54.2 kB] 387s Get:3 http://ftpmaster.internal/ubuntu noble-proposed/universe Sources [376 kB] 387s Get:4 http://ftpmaster.internal/ubuntu noble-proposed/multiverse Sources [2340 B] 387s Get:5 http://ftpmaster.internal/ubuntu noble-proposed/restricted Sources [12.2 kB] 387s Get:6 http://ftpmaster.internal/ubuntu noble-proposed/main arm64 Packages [130 kB] 387s Get:7 http://ftpmaster.internal/ubuntu noble-proposed/main arm64 c-n-f Metadata [3144 B] 387s Get:8 http://ftpmaster.internal/ubuntu noble-proposed/restricted arm64 Packages [92.9 kB] 387s Get:9 http://ftpmaster.internal/ubuntu noble-proposed/restricted arm64 c-n-f Metadata [116 B] 387s Get:10 http://ftpmaster.internal/ubuntu noble-proposed/universe arm64 Packages [563 kB] 387s Get:11 http://ftpmaster.internal/ubuntu noble-proposed/universe arm64 c-n-f Metadata [8528 B] 387s Get:12 http://ftpmaster.internal/ubuntu noble-proposed/multiverse arm64 c-n-f Metadata [116 B] 388s Fetched 1360 kB in 1s (1468 kB/s) 388s Reading package lists... 393s Reading package lists...Setting LLMNR support level "yes" for "2", but the global support level is "no". 393s 394s Building dependency tree... 394s Reading state information... 394s Calculating upgrade... 395s The following packages will be upgraded: 395s apport apport-core-dump-handler libkeyutils1 libnuma1 libunwind8 make man-db 395s netcat-openbsd numactl python3-apport python3-problem-report 395s 11 upgraded, 0 newly installed, 0 to remove and 0 not upgraded. 395s Need to get 1797 kB of archives. 395s After this operation, 1024 B of additional disk space will be used. 395s Get:1 http://ftpmaster.internal/ubuntu noble/main arm64 python3-problem-report all 2.28.1-0ubuntu1 [23.8 kB] 395s Get:2 http://ftpmaster.internal/ubuntu noble/main arm64 python3-apport all 2.28.1-0ubuntu1 [92.1 kB] 395s Get:3 http://ftpmaster.internal/ubuntu noble/main arm64 apport-core-dump-handler all 2.28.1-0ubuntu1 [16.8 kB] 395s Get:4 http://ftpmaster.internal/ubuntu noble/main arm64 apport all 2.28.1-0ubuntu1 [83.5 kB] 395s Get:5 http://ftpmaster.internal/ubuntu noble/main arm64 libkeyutils1 arm64 1.6.3-3build1 [9654 B] 395s Get:6 http://ftpmaster.internal/ubuntu noble/main arm64 netcat-openbsd arm64 1.226-1ubuntu2 [43.8 kB] 395s Get:7 http://ftpmaster.internal/ubuntu noble/main arm64 libnuma1 arm64 2.0.18-1build1 [23.6 kB] 395s Get:8 http://ftpmaster.internal/ubuntu noble/main arm64 man-db arm64 2.12.0-4build2 [1232 kB] 396s Get:9 http://ftpmaster.internal/ubuntu noble/main arm64 libunwind8 arm64 1.6.2-3build1 [53.5 kB] 396s Get:10 http://ftpmaster.internal/ubuntu noble/main arm64 make arm64 4.3-4.1build2 [178 kB] 396s Get:11 http://ftpmaster.internal/ubuntu noble/main arm64 numactl arm64 2.0.18-1build1 [39.5 kB] 396s Preconfiguring packages ... 396s Fetched 1797 kB in 1s (2488 kB/s) 396s (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 ... 112118 files and directories currently installed.) 396s Preparing to unpack .../00-python3-problem-report_2.28.1-0ubuntu1_all.deb ... 396s Unpacking python3-problem-report (2.28.1-0ubuntu1) over (2.28.0-0ubuntu1) ... 397s Preparing to unpack .../01-python3-apport_2.28.1-0ubuntu1_all.deb ... 397s Unpacking python3-apport (2.28.1-0ubuntu1) over (2.28.0-0ubuntu1) ... 397s Preparing to unpack .../02-apport-core-dump-handler_2.28.1-0ubuntu1_all.deb ... 397s Unpacking apport-core-dump-handler (2.28.1-0ubuntu1) over (2.28.0-0ubuntu1) ... 397s Preparing to unpack .../03-apport_2.28.1-0ubuntu1_all.deb ... 397s Unpacking apport (2.28.1-0ubuntu1) over (2.28.0-0ubuntu1) ... 397s Preparing to unpack .../04-libkeyutils1_1.6.3-3build1_arm64.deb ... 397s Unpacking libkeyutils1:arm64 (1.6.3-3build1) over (1.6.3-3) ... 397s Preparing to unpack .../05-netcat-openbsd_1.226-1ubuntu2_arm64.deb ... 397s Unpacking netcat-openbsd (1.226-1ubuntu2) over (1.226-1ubuntu1) ... 397s Preparing to unpack .../06-libnuma1_2.0.18-1build1_arm64.deb ... 397s Unpacking libnuma1:arm64 (2.0.18-1build1) over (2.0.18-1) ... 397s Preparing to unpack .../07-man-db_2.12.0-4build2_arm64.deb ... 397s Unpacking man-db (2.12.0-4build2) over (2.12.0-4build1) ... 397s Preparing to unpack .../08-libunwind8_1.6.2-3build1_arm64.deb ... 397s Unpacking libunwind8:arm64 (1.6.2-3build1) over (1.6.2-3) ... 397s Preparing to unpack .../09-make_4.3-4.1build2_arm64.deb ... 397s Unpacking make (4.3-4.1build2) over (4.3-4.1build1) ... 398s Preparing to unpack .../10-numactl_2.0.18-1build1_arm64.deb ... 398s Unpacking numactl (2.0.18-1build1) over (2.0.18-1) ... 398s Setting up libkeyutils1:arm64 (1.6.3-3build1) ... 398s Setting up python3-problem-report (2.28.1-0ubuntu1) ... 398s Setting up netcat-openbsd (1.226-1ubuntu2) ... 398s Setting up man-db (2.12.0-4build2) ... 398s Updating database of manual pages ... 400s man-db.service is a disabled or a static unit not running, not starting it. 400s Setting up libunwind8:arm64 (1.6.2-3build1) ... 400s Setting up python3-apport (2.28.1-0ubuntu1) ... 400s Setting up make (4.3-4.1build2) ... 400s Setting up libnuma1:arm64 (2.0.18-1build1) ... 400s Setting up numactl (2.0.18-1build1) ... 400s Setting up apport-core-dump-handler (2.28.1-0ubuntu1) ... 401s Setting up apport (2.28.1-0ubuntu1) ... 401s Installing new version of config file /etc/apport/crashdb.conf ... 402s apport-autoreport.service is a disabled or a static unit not running, not starting it. 403s Processing triggers for libc-bin (2.39-0ubuntu8) ... 403s Reading package lists... 403s Building dependency tree... 403s Reading state information... 404s 0 upgraded, 0 newly installed, 0 to remove and 0 not upgraded. 405s Hit:1 http://ftpmaster.internal/ubuntu noble InRelease 405s Hit:2 http://ftpmaster.internal/ubuntu noble-updates InRelease 406s Hit:3 http://ftpmaster.internal/ubuntu noble-security InRelease 406s Hit:4 http://ftpmaster.internal/ubuntu noble-proposed InRelease 407s Reading package lists... 407s Reading package lists... 407s Building dependency tree... 407s Reading state information... 408s Calculating upgrade... 408s 0 upgraded, 0 newly installed, 0 to remove and 0 not upgraded. 409s Reading package lists... 409s Building dependency tree... 409s Reading state information... 409s 0 upgraded, 0 newly installed, 0 to remove and 0 not upgraded. 410s autopkgtest [01:00:42]: rebooting testbed after setup commands that affected boot 454s autopkgtest-virt-ssh: WARNING: ssh connection failed. Retrying in 3 seconds... 470s autopkgtest [01:01:42]: testbed running kernel: Linux 6.8.0-22-generic #22-Ubuntu SMP PREEMPT_DYNAMIC Fri Apr 5 02:52:09 UTC 2024 474s autopkgtest [01:01:46]: @@@@@@@@@@@@@@@@@@@@ apt-source cpl-plugin-vimos 480s Get:1 http://ftpmaster.internal/ubuntu noble/universe cpl-plugin-vimos 4.1.7+dfsg-2build3 (dsc) [2550 B] 480s Get:2 http://ftpmaster.internal/ubuntu noble/universe cpl-plugin-vimos 4.1.7+dfsg-2build3 (tar) [2197 kB] 480s Get:3 http://ftpmaster.internal/ubuntu noble/universe cpl-plugin-vimos 4.1.7+dfsg-2build3 (diff) [12.4 kB] 480s gpgv: Signature made Mon Apr 1 05:39:53 2024 UTC 480s gpgv: using RSA key A089FB36AAFBDAD5ACC1325069F790171A210984 480s gpgv: Can't check signature: No public key 480s dpkg-source: warning: cannot verify inline signature for ./cpl-plugin-vimos_4.1.7+dfsg-2build3.dsc: no acceptable signature found 482s autopkgtest [01:01:54]: testing package cpl-plugin-vimos version 4.1.7+dfsg-2build3 483s autopkgtest [01:01:55]: build not needed 571s autopkgtest [01:03:23]: test test-recipe.py: preparing testbed 573s Reading package lists... 573s Building dependency tree... 573s Reading state information... 574s Starting pkgProblemResolver with broken count: 0 574s Starting 2 pkgProblemResolver with broken count: 0 574s Done 576s The following additional packages will be installed: 576s cpl-plugin-vimos libblas3 libcext0 libcfitsio10t64 libcplcore26 libcpldfs26 576s libcpldrs26 libcplui26 liberfa1 libfftw3-double3 libfftw3-single3 576s libgfortran5 libgomp1 libgsl27 libgslcblas0 libjs-jquery 576s libjs-jquery-hotkeys libjs-jquery-isonscreen libjs-jquery-metadata 576s libjs-jquery-tablesorter libjs-jquery-throttle-debounce libjs-sphinxdoc 576s libjs-underscore liblapack3 libwcs8 python3-astropy 576s python3-astropy-iers-data python3-coverage python3-cpl python3-dateutil 576s python3-erfa python3-hypothesis python3-iniconfig python3-numpy 576s python3-packaging python3-pluggy python3-ply python3-pytest 576s python3-pytest-arraydiff python3-pytest-astropy 576s python3-pytest-astropy-header python3-pytest-cov python3-pytest-doctestplus 576s python3-pytest-filter-subpackage python3-pytest-mock 576s python3-pytest-remotedata python3-sortedcontainers 576s Suggested packages: 576s cpl-plugin-vimos-calib cpl-plugin-vimos-doc libfftw3-bin libfftw3-dev 576s gsl-ref-psdoc | gsl-doc-pdf | gsl-doc-info | gsl-ref-html libxml2-utils 576s python-astropy-doc python3-astropy-affiliated python3-bs4 python3-h5py 576s python3-matplotlib python3-pandas python-coverage-doc gdb 576s python-hypothesis-doc gcc gfortran python3-dev python-ply-doc 576s python-pytest-mock-doc python-sortedcontainers-doc 576s Recommended packages: 576s javascript-common libjs-jquery-datatables python3-scipy python3-click 576s The following NEW packages will be installed: 576s autopkgtest-satdep cpl-plugin-vimos libblas3 libcext0 libcfitsio10t64 576s libcplcore26 libcpldfs26 libcpldrs26 libcplui26 liberfa1 libfftw3-double3 576s libfftw3-single3 libgfortran5 libgomp1 libgsl27 libgslcblas0 libjs-jquery 576s libjs-jquery-hotkeys libjs-jquery-isonscreen libjs-jquery-metadata 576s libjs-jquery-tablesorter libjs-jquery-throttle-debounce libjs-sphinxdoc 576s libjs-underscore liblapack3 libwcs8 python3-astropy 576s python3-astropy-iers-data python3-coverage python3-cpl python3-dateutil 576s python3-erfa python3-hypothesis python3-iniconfig python3-numpy 576s python3-packaging python3-pluggy python3-ply python3-pytest 576s python3-pytest-arraydiff python3-pytest-astropy 576s python3-pytest-astropy-header python3-pytest-cov python3-pytest-doctestplus 576s python3-pytest-filter-subpackage python3-pytest-mock 576s python3-pytest-remotedata python3-sortedcontainers 576s 0 upgraded, 48 newly installed, 0 to remove and 0 not upgraded. 576s Need to get 19.2 MB/19.2 MB of archives. 576s After this operation, 85.1 MB of additional disk space will be used. 576s Get:1 /tmp/autopkgtest.y0IoQo/1-autopkgtest-satdep.deb autopkgtest-satdep arm64 0 [732 B] 576s Get:2 http://ftpmaster.internal/ubuntu noble/main arm64 libjs-jquery all 3.6.1+dfsg+~3.5.14-1 [328 kB] 577s Get:3 http://ftpmaster.internal/ubuntu noble/universe arm64 libjs-jquery-hotkeys all 0~20130707+git2d51e3a9+dfsg-2ubuntu2 [11.5 kB] 577s Get:4 http://ftpmaster.internal/ubuntu noble/universe arm64 libcext0 arm64 7.3.2+ds-1build3 [31.6 kB] 577s Get:5 http://ftpmaster.internal/ubuntu noble/universe arm64 libcfitsio10t64 arm64 4.3.1-1.1build2 [520 kB] 577s Get:6 http://ftpmaster.internal/ubuntu noble/main arm64 libgomp1 arm64 14-20240412-0ubuntu1 [144 kB] 577s Get:7 http://ftpmaster.internal/ubuntu noble/main arm64 libfftw3-double3 arm64 3.3.10-1ubuntu3 [384 kB] 577s Get:8 http://ftpmaster.internal/ubuntu noble/main arm64 libfftw3-single3 arm64 3.3.10-1ubuntu3 [583 kB] 577s Get:9 http://ftpmaster.internal/ubuntu noble/universe arm64 libcplcore26 arm64 7.3.2+ds-1build3 [446 kB] 577s Get:10 http://ftpmaster.internal/ubuntu noble/universe arm64 libcplui26 arm64 7.3.2+ds-1build3 [36.5 kB] 577s Get:11 http://ftpmaster.internal/ubuntu noble/universe arm64 libcpldfs26 arm64 7.3.2+ds-1build3 [39.0 kB] 577s Get:12 http://ftpmaster.internal/ubuntu noble/universe arm64 libwcs8 arm64 8.2.2+ds-3build2 [253 kB] 577s Get:13 http://ftpmaster.internal/ubuntu noble/universe arm64 libcpldrs26 arm64 7.3.2+ds-1build3 [62.8 kB] 577s Get:14 http://ftpmaster.internal/ubuntu noble-proposed/universe arm64 libgslcblas0 arm64 2.7.1+dfsg-6ubuntu2 [72.8 kB] 577s Get:15 http://ftpmaster.internal/ubuntu noble-proposed/universe arm64 libgsl27 arm64 2.7.1+dfsg-6ubuntu2 [918 kB] 577s Get:16 http://ftpmaster.internal/ubuntu noble/universe arm64 cpl-plugin-vimos arm64 4.1.7+dfsg-2build3 [1118 kB] 577s Get:17 http://ftpmaster.internal/ubuntu noble/main arm64 libblas3 arm64 3.12.0-3build1 [143 kB] 577s Get:18 http://ftpmaster.internal/ubuntu noble/main arm64 libgfortran5 arm64 14-20240412-0ubuntu1 [444 kB] 577s Get:19 http://ftpmaster.internal/ubuntu noble/universe arm64 libjs-jquery-metadata all 12-4 [6582 B] 577s Get:20 http://ftpmaster.internal/ubuntu noble/universe arm64 libjs-jquery-tablesorter all 1:2.31.3+dfsg1-3 [193 kB] 577s Get:21 http://ftpmaster.internal/ubuntu noble/universe arm64 libjs-jquery-throttle-debounce all 1.1+dfsg.1-2 [12.5 kB] 577s Get:22 http://ftpmaster.internal/ubuntu noble/main arm64 libjs-underscore all 1.13.4~dfsg+~1.11.4-3 [118 kB] 577s Get:23 http://ftpmaster.internal/ubuntu noble/main arm64 libjs-sphinxdoc all 7.2.6-6 [149 kB] 577s Get:24 http://ftpmaster.internal/ubuntu noble/main arm64 liblapack3 arm64 3.12.0-3build1 [2241 kB] 577s Get:25 http://ftpmaster.internal/ubuntu noble/universe arm64 python3-iniconfig all 1.1.1-2 [6024 B] 577s Get:26 http://ftpmaster.internal/ubuntu noble/main arm64 python3-packaging all 24.0-1 [41.1 kB] 577s Get:27 http://ftpmaster.internal/ubuntu noble/universe arm64 python3-pluggy all 1.4.0-1 [20.4 kB] 577s Get:28 http://ftpmaster.internal/ubuntu noble/universe arm64 python3-pytest all 7.4.4-1 [305 kB] 577s Get:29 http://ftpmaster.internal/ubuntu noble/main arm64 python3-dateutil all 2.8.2-3ubuntu1 [79.4 kB] 577s Get:30 http://ftpmaster.internal/ubuntu noble/main arm64 python3-sortedcontainers all 2.4.0-2 [27.6 kB] 577s Get:31 http://ftpmaster.internal/ubuntu noble/universe arm64 python3-hypothesis all 6.98.15-1 [311 kB] 577s Get:32 http://ftpmaster.internal/ubuntu noble/main arm64 python3-numpy arm64 1:1.26.4+ds-6ubuntu1 [3565 kB] 577s Get:33 http://ftpmaster.internal/ubuntu noble/universe arm64 python3-pytest-arraydiff all 0.6.1-2 [10.2 kB] 577s Get:34 http://ftpmaster.internal/ubuntu noble/universe arm64 python3-pytest-astropy-header all 0.2.2-1 [8190 B] 577s Get:35 http://ftpmaster.internal/ubuntu noble/universe arm64 python3-coverage arm64 7.4.4+dfsg1-0ubuntu2 [148 kB] 577s Get:36 http://ftpmaster.internal/ubuntu noble/universe arm64 libjs-jquery-isonscreen all 1.2.0-1.1 [3244 B] 577s Get:37 http://ftpmaster.internal/ubuntu noble/universe arm64 python3-pytest-cov all 4.1.0-1 [21.5 kB] 577s Get:38 http://ftpmaster.internal/ubuntu noble/universe arm64 python3-pytest-doctestplus all 1.2.0-1 [23.1 kB] 577s Get:39 http://ftpmaster.internal/ubuntu noble/universe arm64 python3-pytest-filter-subpackage all 0.2.0-1 [6094 B] 577s Get:40 http://ftpmaster.internal/ubuntu noble/universe arm64 python3-pytest-mock all 3.12.0-1.1 [11.3 kB] 577s Get:41 http://ftpmaster.internal/ubuntu noble/universe arm64 python3-pytest-remotedata all 0.4.1-1 [8650 B] 578s Get:42 http://ftpmaster.internal/ubuntu noble/universe arm64 python3-pytest-astropy all 0.11.0-1 [5902 B] 578s Get:43 http://ftpmaster.internal/ubuntu noble/main arm64 python3-ply all 3.11-6 [46.5 kB] 578s Get:44 http://ftpmaster.internal/ubuntu noble/universe arm64 python3-astropy-iers-data all 0.2024.01.01.00.33.39-1 [2046 kB] 578s Get:45 http://ftpmaster.internal/ubuntu noble/universe arm64 liberfa1 arm64 2.0.1-1 [136 kB] 578s Get:46 http://ftpmaster.internal/ubuntu noble/universe arm64 python3-erfa arm64 2.0.1.1+ds-3 [311 kB] 578s Get:47 http://ftpmaster.internal/ubuntu noble/universe arm64 python3-astropy arm64 6.0.0-1ubuntu2 [3797 kB] 578s Get:48 http://ftpmaster.internal/ubuntu noble/universe arm64 python3-cpl arm64 0.7.4-2build10 [34.8 kB] 579s Fetched 19.2 MB in 2s (12.1 MB/s) 579s Selecting previously unselected package libjs-jquery. 579s (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 ... 112117 files and directories currently installed.) 579s Preparing to unpack .../00-libjs-jquery_3.6.1+dfsg+~3.5.14-1_all.deb ... 579s Unpacking libjs-jquery (3.6.1+dfsg+~3.5.14-1) ... 579s Selecting previously unselected package libjs-jquery-hotkeys. 579s Preparing to unpack .../01-libjs-jquery-hotkeys_0~20130707+git2d51e3a9+dfsg-2ubuntu2_all.deb ... 579s Unpacking libjs-jquery-hotkeys (0~20130707+git2d51e3a9+dfsg-2ubuntu2) ... 579s Selecting previously unselected package libcext0:arm64. 579s Preparing to unpack .../02-libcext0_7.3.2+ds-1build3_arm64.deb ... 579s Unpacking libcext0:arm64 (7.3.2+ds-1build3) ... 579s Selecting previously unselected package libcfitsio10t64:arm64. 579s Preparing to unpack .../03-libcfitsio10t64_4.3.1-1.1build2_arm64.deb ... 579s Unpacking libcfitsio10t64:arm64 (4.3.1-1.1build2) ... 579s Selecting previously unselected package libgomp1:arm64. 579s Preparing to unpack .../04-libgomp1_14-20240412-0ubuntu1_arm64.deb ... 579s Unpacking libgomp1:arm64 (14-20240412-0ubuntu1) ... 579s Selecting previously unselected package libfftw3-double3:arm64. 580s Preparing to unpack .../05-libfftw3-double3_3.3.10-1ubuntu3_arm64.deb ... 580s Unpacking libfftw3-double3:arm64 (3.3.10-1ubuntu3) ... 580s Selecting previously unselected package libfftw3-single3:arm64. 580s Preparing to unpack .../06-libfftw3-single3_3.3.10-1ubuntu3_arm64.deb ... 580s Unpacking libfftw3-single3:arm64 (3.3.10-1ubuntu3) ... 580s Selecting previously unselected package libcplcore26:arm64. 580s Preparing to unpack .../07-libcplcore26_7.3.2+ds-1build3_arm64.deb ... 580s Unpacking libcplcore26:arm64 (7.3.2+ds-1build3) ... 580s Selecting previously unselected package libcplui26:arm64. 580s Preparing to unpack .../08-libcplui26_7.3.2+ds-1build3_arm64.deb ... 580s Unpacking libcplui26:arm64 (7.3.2+ds-1build3) ... 580s Selecting previously unselected package libcpldfs26:arm64. 580s Preparing to unpack .../09-libcpldfs26_7.3.2+ds-1build3_arm64.deb ... 580s Unpacking libcpldfs26:arm64 (7.3.2+ds-1build3) ... 580s Selecting previously unselected package libwcs8:arm64. 580s Preparing to unpack .../10-libwcs8_8.2.2+ds-3build2_arm64.deb ... 580s Unpacking libwcs8:arm64 (8.2.2+ds-3build2) ... 580s Selecting previously unselected package libcpldrs26:arm64. 580s Preparing to unpack .../11-libcpldrs26_7.3.2+ds-1build3_arm64.deb ... 580s Unpacking libcpldrs26:arm64 (7.3.2+ds-1build3) ... 580s Selecting previously unselected package 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(0.7.4-2build10) ... 595s Setting up autopkgtest-satdep (0) ... 595s Processing triggers for man-db (2.12.0-4build2) ... 596s Processing triggers for libc-bin (2.39-0ubuntu8) ... 602s (Reading database ... 115997 files and directories currently installed.) 602s Removing autopkgtest-satdep (0) ... 603s autopkgtest [01:03:55]: test test-recipe.py: [----------------------- 604s Recipe vimos_ima_fringe: 604s version 4.1.7 604s Parameters: {'prettynames': False, 'psm_ipix': 5, 'psm_thresh': 3.0, 'psm_nbsize': 64} 604s Docstring: Fringe frame creation for imaging 604s 604s vimos_ima_fringe -- VIMOS fringe frame creation recipe. Take a list 604s of science frames and correct them to remove bias, dark and flat field 604s signatures. Combine the images to form a new master fringe frame The 604s program accepts the following files in the SOF: Tag 604s Description ------------------------------------------------------ 604s ----------------- OBJECT A list of raw science 604s images MASTER_BIAS A master bias frame MASTER_DARK 604s A master dark frame MASTER_TWILIGHT_FLAT A master flat frame 604s MASTER_CONF A master confidence map MASTER_READGAIN 604s A master readgain table All of these are required. 604s 604s Parameters: 604s prettynames: Use pretty product names? (bool; default: False) 604s psm_ipix: Minimum pixel area for each detected object (int; 604s default: 5) 604s psm_thresh: Detection threshold in sigma above sky (float; default: 604s 3.0) 604s psm_nbsize: Background smoothing box size (int; default: 64) 604s Author: Jim Lewis 604s 604s 604s Recipe vmifucombinecube: 604s version 4.1.7 604s Parameters: {} 604s Docstring: Rearrange into cube format images of extracted spectraproduced by 604s vmifucalib, vmifuscience, and vmifustandard. 604s 604s This recipe is used to rearrange into a single cube the images of 604s extracted spectra from different VIMOS quadrants. Such images are 604s created by the recipes vmifucalib, vmifuscience, and vmifustandard, 604s and the classification tag of the product depends on the 604s classification tag of the inputs: Input 604s Output IFU_ARC_SPECTRUM_EXTRACTED IFU_ARC_SPECTRUM_CUBE 604s IFU_FLAT_SPECTRUM_EXTRACTED IFU_FLAT_SPECTRUM_CUBE 604s IFU_SCIENCE_REDUCED IFU_SCIENCE_CUBE 604s IFU_SCIENCE_FLUX_REDUCED IFU_SCIENCE_FLUX_CUBE 604s IFU_STANDARD_REDUCED IFU_STANDARD_CUBE The input images must 604s belong to different quadrants, so that they cannot be more than 4. The 604s allocated cubes are the smallest possible, depending on the number of 604s quadrants involved and on whether the IFU shutter was on or off. The 604s smallest cubes (20x20xN) are produced when just one quadrant is input 604s and the shutter was on. The largest cubes (80x80xN) are produced when 604s 3 or more quadrants are given in input (and when either quadrants 1 604s and 3, or 2 and 4, are input), and the shutter was off. Pixels 604s belonging to missing quadrants are padded with zeroes if necessary. 604s 604s No parameters 604s Author: ESO VIMOS Pipeline Team and VIMOS Consortium 604s 604s 604s Recipe vmifuscience: 604s version 4.1.7 604s Parameters: {'BiasMethod': 'Zmaster', 'CleanBadPixel': False, 'ApplyTransmission': True, 'CalibrateFlux': False, 'UseSkylines': True, 'UseSkyIndividual': False, 'ComputeQC': False} 604s Docstring: Extract spectra from an IFU scientific exposure. 604s 604s This recipe extracts IFU scientific spectra using the input extraction 604s mask, after aligning it to the brightest fiber spectra detected on the 604s input exposure. The extracted spectra are then resampled at a constant 604s wavelength step, after aligning the input wavelength calibration to 604s the positions of a set of identified sky lines. The extracted spectra 604s are eventually corrected for the relative differences in transmission 604s from fiber to fiber. Input files: DO category: Type: 604s Explanation: Required: IFU_SCIENCE Raw 604s Scientific spectra Y MASTER_BIAS Calib 604s Master bias Y IFU_TRACE Calib 604s Extraction mask Y IFU_IDS Calib 604s Wavelength calibration Y IFU_TRANSMISSION Calib 604s Transmission correction Y EXTINCT_TABLE Calib 604s Atmospheric extinction . IFU_SPECPHOT_TABLE Calib 604s Response curve . CCD_TABLE Calib 604s Bad pixel table . Output files: DO category: 604s Data type: Explanation: IFU_SCIENCE_REDUCED FITS image 604s Reduced scientific spectra IFU_SCIENCE_FLUX_REDUCED FITS image 604s Reduced scientific spectra IFU_FOV FITS image 604s Reconstructed IFU field-of-view IFU_SKY_TRACE FITS table 604s Science aligned extraction mask Only if sky alignment is requested: 604s IFU_SKY_IDS FITS table Sky aligned wavelength solution 604s The extraction mask, the wavelength calibration, and the relative 604s transmission table, are those generated by the recipe vmifucalib. A 604s CCD table must be specified only if a bad pixel cleaning is requested. 604s For more details, please refer to the VIMOS Pipeline User's Guide. 604s 604s Parameters: 604s BiasMethod: Bias removal method. (str; default: 'Zmaster') 604s CleanBadPixel: Bad pixel correction on master flat field. (bool; 604s default: False) 604s ApplyTransmission: Apply transmission correction to extracted 604s scientific spectra (bool; default: True) 604s CalibrateFlux: Extracted spectra are flux calibrated. (bool; 604s default: False) 604s UseSkylines: Use sky lines to refine the wavelength calibration 604s (bool; default: True) 604s UseSkyIndividual: Use sky lines to refine the wavelength calibration 604s individually for each spectrum (bool; default: 604s False) 604s ComputeQC: Compute QC1 parameters (bool; default: False) 604s Author: ESO VIMOS Pipeline Team 604s 604s 604s Recipe vmmoscalib: 604s version 4.1.7 604s Parameters: {'dispersion': 0.0, 'peakdetection': 0.0, 'wdegree': 0, 'wradius': 4, 'wreject': 1.0, 'wmodelss': 2, 'wmodemos': 1, 'ignore_lines': '', 'used_linesets': 'standard', 'cdegree': 0, 'cmode': 1, 'startwavelength': 0.0, 'endwavelength': 0.0, 'reference': 0.0, 'slit_ident': True, 's_degree': -1, 'sradius': -1, 'd_nknots': -1, 'dradius': 10, 'fit_threshold': 0.01, 'line_ident_tol': 0.05, 'normalise_spa_local': True} 604s Docstring: Determination of the extraction mask 604s 604s This recipe is used to identify reference lines on MOS arc lamp 604s exposures, and trace the spectral edges on the corresponding flat 604s field exposures. This information is used to determine the spectral 604s extraction mask to be applied in the scientific data reduction, 604s performed with the recipe vimos_science. The input arc lamp and flat 604s field exposures are assumed to be obtained quasi-simultaneously, so 604s that they would be described by exactly the same instrument 604s distortions. A line catalog must be specified, containing the 604s wavelengths of the reference arc lamp lines used for the wavelength 604s calibration. A grism table (typically depending on the instrument 604s mode, and in particular on the grism used) may also be specified: this 604s table contains a default recipe parameter setting to control the way 604s spectra are extracted for a specific instrument mode, as it is used 604s for automatic run of the pipeline on Paranal and in Garching. If this 604s table is specified, it will modify the default recipe parameter 604s setting, with the exception of those parameters which have been 604s explicitly modifyed on the command line. If a grism table is not 604s specified, the input recipe parameters values will always be read from 604s the command line, or from an esorex configuration file if present, or 604s from their generic default values (that are rarely meaningful). 604s Finally a master bias frame must be input to this recipe. In the table 604s below the MOS_CURV_COEFF, MOS_CURV_TRACES, MOS_SPATIAL_MAP 604s MOS_ARC_SPECTRUM_EXTRACTED, MOS_SPECTRA_DETECTION, MOS_SLIT_MAP, and 604s MOS_SLIT_LOCATION, are never created in case of long-slit-like data. 604s The products MOS_SPECTRA_DETECTION, MOS_SLIT_MAP, and 604s MOS_DISP_RESIDUALS, are just created if the --check parameter is set 604s to true. The product GLOBAL_DISTORTION_TABLE is just created if more 604s than 12 separate spectra are found in the CCD. Input files: DO 604s category: Type: Explanation: Required: 604s MOS_SCREEN_FLAT Raw Flat field exposures Y 604s MOS_ARC_SPECTRUM Raw Arc lamp exposure Y 604s MASTER_BIAS Calib Bias frame Y 604s LINE_CATALOG Calib Line catalog Y 604s CONFIG_TABLE Calib Grism table . 604s Output files: DO category: Data type: Explanation: 604s MOS_COMBINED_SCREEN_FLAT FITS image Combined (sum) flat field 604s MOS_MASTER_SCREEN_FLAT FITS image Normalised flat field 604s MOS_ARC_SPECTRUM_EXTRACTED FITS image Wavelength calibrated arc 604s spectrum MOS_DISP_COEFF FITS table Inverse dispersion 604s coefficients MOS_DISP_RESIDUALS FITS image Residuals in 604s wavelength calibration MOS_DISP_RESIDUALS_TABLE FITS table 604s Residuals in wavelength calibration MOS_DELTA_IMAGE FITS 604s image Offset vs linear wavelength calib MOS_WAVELENGTH_MAP 604s FITS image Wavelength for each pixel on CCD MOS_SPECTRA_DETECTION 604s FITS image Check for preliminary detection MOS_SLIT_MAP 604s FITS image Map of central wavelength on CCD MOS_CURV_TRACES 604s FITS table Spectral curvature traces MOS_CURV_COEFF 604s FITS table Spectral curvature coefficients MOS_SPATIAL_MAP 604s FITS image Spatial position along slit on CCD 604s MOS_SPECTRAL_RESOLUTION FITS table Resolution at reference arc 604s lines MOS_SLIT_LOCATION FITS table Slits on product frames 604s and CCD GLOBAL_DISTORTION_TABLE FITS table Global distortions 604s table 604s 604s Parameters: 604s dispersion: Expected spectral dispersion (Angstrom/pixel) 604s (float; default: 0.0) 604s peakdetection: Initial peak detection threshold (ADU) (float; 604s default: 0.0) 604s wdegree: Degree of wavelength calibration polynomial 604s (int; default: 0) 604s wradius: Search radius if iterating pattern-matching with 604s first-guess method (pixel) (int; default: 4) 604s wreject: Rejection threshold in dispersion relation fit 604s (pixel) (float; default: 1.0) 604s wmodelss: Interpolation mode of wavelength solution (0 = 604s no interpolation, 1 = fill gaps, 2 = global 604s model) (int; default: 2) 604s wmodemos: Interpolation mode of wavelength solution (0 = 604s no interpolation, 1 = local (slit) solution, 2 = 604s global model) (int; default: 1) 604s ignore_lines: Catalog lines nearest to wavelengths in this 604s list will be ignored for wavelength calibration 604s (str; default: '') 604s used_linesets: Linesets to use. Valid are 'standard' 604s and'extended' (see column LINE_SET in the line 604s catalogue) (str; default: 'standard') 604s cdegree: Degree of spectral curvature polynomial (int; 604s default: 0) 604s cmode: Interpolation mode of curvature solution 604s applicable to MOS-like data (0 = no 604s interpolation, 1 = fill gaps, 2 = global model) 604s (int; default: 1) 604s startwavelength: Start wavelength in spectral extraction (float; 604s default: 0.0) 604s endwavelength: End wavelength in spectral extraction (float; 604s default: 0.0) 604s reference: Reference wavelength for slit map (float; 604s default: 0.0) 604s slit_ident: Attempt slit identification.For multiplexing 604s data slit identification is always performed. 604s Switching it off will cause systematic errors in 604s the absolute flux calibration if the FLAT_SED 604s correction is used (see pipeline manual for 604s details) (bool; default: True) 604s s_degree: Polynomial degree for the flat field fitting 604s along spatial direction (int; default: -1) 604s sradius: Smooth box radius for flat field along spatial 604s direction (used if s_degree < 0) (int; default: 604s -1) 604s d_nknots: Number of knots in flat field fitting splines 604s along dispersion direction (int; default: -1) 604s dradius: Smooth box radius for flat field along 604s dispersion direction (if d_knots < 0) (int; 604s default: 10) 604s fit_threshold: Threshold percentage for flat spline fitting 604s with respect to the maximum (float; default: 604s 0.01) 604s line_ident_tol: Tolerance for the ratio of detected lines vs 604s reference lines. This is used during for arc 604s line identification. (float; default: 0.05) 604s normalise_spa_local: If TRUE the normalization along the spatial axis 604s is performed row-by- row otherwise a collapsed 604s slit is used. (bool; default: True) 604s Author: Carlo Izzo 604s 604s 604s Recipe vmifucalib: 604s version 4.1.7 604s Parameters: {'AllowSingleFrames': True, 'StackMethod': 'MinMax', 'KSigmaLow': 5.0, 'KSigmaHigh': 5.0, 'MinRejection': 0, 'MaxRejection': 1, 'BiasMethod': 'Zmaster', 'CleanBadPixel': False, 'ApplyTransmission': True, 'MaxIdsRms': 2.0, 'LineIdent': 'Blind', 'MaxTraceRejection': 33, 'ComputeQC': True} 604s Docstring: Generate IFU calibrations from a set of flat and arc lamp exposures. 604s 604s This recipe produces the extraction mask, the wavelength calibration, 604s and the relative transmission correction, from a set of flat field and 604s one arc lamp exposures (IFU mode). Input files: DO category: 604s Type: Explanation: Required: IFU_SCREEN_FLAT 604s Raw Flat field Y IFU_ARC_SPECTRUM Raw 604s Arc spectrum . LINE_CATALOG Calib Arc 604s line catalog . MASTER_BIAS Calib Master 604s bias Y IFU_IDENT Calib Fiber 604s identification . CCD_TABLE Calib Bad pixel 604s table . Output files: DO category: Data 604s type: Explanation: IFU_MASTER_SCREEN_FLAT FITS image Stack 604s of all raw flat fields IFU_ARC_SPECTRUM_EXTRACTED FITS image 604s Extracted arc spectra IFU_FLAT_SPECTRUM_EXTRACTED FITS image 604s Extracted flat field spectra IFU_TRACE FITS table 604s Extraction mask IFU_IDS FITS table Wavelength 604s calibration IFU_TRANSMISSION FITS table Transmission 604s correction An arc spectrum exposure may not be specified in input, 604s but in that case no wavelength calibration nor fiber relative 604s transmission correction will be computed, and further reduction of 604s associated scientific data will not be possible; the only products in 604s this case will be the stack of all the input raw flat field exposures, 604s and the extraction mask. If the arc spectrum exposure is specified in 604s input, then also a line catalog must be given. The fiber 604s identification table, if given, ensures that all spectra will be 604s safely identified and assigned to the correct spatial position, but in 604s most cases it will be possible to reduce the data even without 604s specifying this table in the input SOF. A CCD table must be specified 604s only if a bad pixel cleaning is requested. For more details, please 604s refer to the VIMOS Pipeline User's Guide. 604s 604s Parameters: 604s AllowSingleFrames: Flat fields combination method is ignored. (bool; 604s default: True) 604s StackMethod: Flat fields combination method. (str; default: 604s 'MinMax') 604s KSigmaLow: Low threshold for K-sigma clipping method. (float; 604s default: 5.0) 604s KSigmaHigh: High threshold for K-sigma clipping method. 604s (float; default: 5.0) 604s MinRejection: Number of lowest rejected values for rejection 604s method. (int; default: 0) 604s MaxRejection: Number of highest rejected values for rejection 604s method. (int; default: 1) 604s BiasMethod: Bias removal method. (str; default: 'Zmaster') 604s CleanBadPixel: Bad pixel correction on master flat field. (bool; 604s default: False) 604s ApplyTransmission: Apply transmission correction to extracted arc 604s lamp spectra (bool; default: True) 604s MaxIdsRms: Maximum tolerated RMS of residuals in IDS fit 604s (float; default: 2.0) 604s LineIdent: Arc line identification method. (str; default: 604s 'Blind') 604s MaxTraceRejection: Maximum percentage of rejected positions in fiber 604s spectra tracing (int; default: 33) 604s ComputeQC: Compute QC1 parameters (bool; default: True) 604s Author: ESO VIMOS Pipeline Team and VIMOS Consortium 604s 604s 604s Recipe vimos_ima_det_noise: 604s version 4.1.7 604s Parameters: {'thresh': 5.0} 604s Docstring: Detector noise for imaging 604s 604s vimos_ima_det_noise -- VIMOS recipe to find readnoise and gain. 604s Compute the readnoise and gain for the vimos detectors using two bias 604s frames and two flat field frames. The program accepts the following 604s files in the SOF: Tag Description --------- 604s -------------------------------------------------------------- 604s BIAS A list of raw bias images FLAT_TWILIGHT 604s A list of raw flat images MASTER_BPM Optional master 604s bad pixel mask or MASTER_CONF Optional master confidence 604s map If a master bad pixel mask or confidence map is included then 604s thebad pixels will be flagged during the statistical analysis 604s 604s Parameters: 604s thresh: Rejection threshold in sigma above background (float; 604s default: 5.0) 604s Author: Jim Lewis 604s 604s 604s Recipe vimos_ima_twilight_flat: 604s version 4.1.7 604s Parameters: {'lthr': 4000.0, 'hthr': 60000.0, 'combtype': 'median', 'scaletype': 'multiplicative', 'xrej': True, 'thresh': 5.0, 'ncells': 8, 'prettynames': False} 604s Docstring: Twilight flat combination for imaging 604s 604s vimos_ima_twilight_flat -- VIMOS twilight flat combine recipe. 604s Combine a list of twilight flat frames into a mean frame. Optionally 604s compare the output frame to a reference twilight flat frame The 604s program accepts the following files in the SOF: Tag 604s Description ------------------------------------------------------ 604s ----------------- FLAT_TWILIGHT A list of raw twilight 604s flat images MASTER_BIAS A master bias frame 604s MASTER_DARK A master dark frame REFERENCE_TWILIGHT_FLAT 604s Optional reference twilight flat frame If no reference twilight flat 604s is made available, then no comparison will be done. This means there 604s will be no output ratio image and no stats 604s 604s Parameters: 604s lthr: Low rejection threshold for underexpsed images (float; 604s default: 4000.0) 604s hthr: High rejection threshold for overexposed images (float; 604s default: 60000.0) 604s combtype: Combination algorithm (str; default: 'median') 604s scaletype: Scaling algorithm (str; default: 'multiplicative') 604s xrej: True if using extra rejection cycle (bool; default: 604s True) 604s thresh: Rejection threshold in sigma above background (float; 604s default: 5.0) 604s ncells: Number of cells for diff image stats (int; default: 8) 604s prettynames: Use pretty output file names? (bool; default: False) 604s Author: Jim Lewis 604s 604s 604s Recipe vimos_ima_standard: 604s version 4.1.7 604s Parameters: {'preview_only': False, 'minphotom': 1, 'prettynames': False, 'savemstd': False, 'cdssearch_astrom': 'none', 'cdssearch_photom': 'none', 'ignore_fringe': False, 'src_cat_ipix': 5, 'src_cat_thresh': 2.5, 'src_cat_icrowd': True, 'src_cat_rcore': 5.0, 'src_cat_nbsize': 128, 'cacheloc': '.', 'magerrcut': 100.0, 'lthr_mag': 15.0, 'hthr_mag': 32.0} 605s Docstring: Standard field processing for imaging 605s 605s vimos_ima_standard -- VIMOS standard star recipe. Take a list of 605s standard frames and correct them to remove bias, dark and flat field 605s signatures. Optionally defringe the reddest filter images. 605s Astrometrically and photometrically calibrate the individual images, 605s but do no stacking The program accepts the following files in the 605s SOF: Tag Description ---------------------- 605s ------------------------------------------------- STD 605s A list of raw standard images MASTER_BIAS A master bias 605s frame MASTER_DARK A master dark frame 605s MASTER_TWILIGHT_FLAT A master flat frame MASTER_CONF A 605s master confidence map MASTER_FRINGE A master fringe map 605s (optional) MASTER_FRINGE_VAR A master fringe variance map 605s (optional) MASTER_READGAIN A master readgain table 605s MASTER_2MASS_CATALOGUE_ASTROM A master 2MASS index for astrometry or 605s MASTER_PPMXL_CATALOGUE_ASTROM A master PPMXL index for astrometry or 605s MASTER_APASS_CATALOGUE_ASTROM A master APASS index for astrometry or 605s MASTER_LOCAL_CATALOGUE_ASTROM A master local catalogue index for 605s astrometry MASTER_APASS_CATALOGUE_PHOTOM A master APASS index for 605s photometry or MASTER_LOCAL_CATALOGUE_PHOTOM A master local 605s catalogue index for photometry PHOTCAL_TAB A photometric 605s calibration table SCHLEGEL_MAP_NORTH Northern Schlegel Map 605s SCHLEGEL_MAP_SOUTH Southern Schlegel Map All of these are required 605s unless specified otherwise. 605s 605s Parameters: 605s preview_only: Preview only? (bool; default: False) 605s minphotom: Minimum stars for photometry solution (int; 605s default: 1) 605s prettynames: Use pretty product names? (bool; default: False) 605s savemstd: Save matched standard catalogues? (bool; default: 605s False) 605s cdssearch_astrom: CDS astrometric catalogue (str; default: 'none') 605s cdssearch_photom: CDS photometric catalogue (str; default: 'none') 605s ignore_fringe: Ignore provided fringe frame? (bool; default: 605s False) 605s src_cat_ipix: Minimum pixel area for each detected object (int; 605s default: 5) 605s src_cat_thresh: Detection threshold in sigma above sky (float; 605s default: 2.5) 605s src_cat_icrowd: Use deblending? (bool; default: True) 605s src_cat_rcore: Value of Rcore in pixels (float; default: 5.0) 605s src_cat_nbsize: Background smoothing box size (int; default: 128) 605s cacheloc: Location for standard star cache (str; default: 605s '.') 605s magerrcut: A cut in the magnitude error (float; default: 605s 100.0) 605s lthr_mag: STD stars with magnitudes BRIGHTER than this are 605s removed. (float; default: 15.0) 605s hthr_mag: STD stars with magnitudes FAINTER than this are 605s removed. (float; default: 32.0) 605s Author: Jim Lewis 605s 605s 605s Recipe vmmosscience: 605s version 4.1.7 605s Parameters: {'skyalign': -1, 'flatfield': True, 'skyglobal': False, 'skymedian': False, 'skylocal': True, 'cosmics': True, 'slit_margin': 3, 'ext_radius': 6, 'cont_radius': 0, 'ext_mode': 1, 'detection': 2.0, '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', 'resp_shift': 0.0, 'time_normalise': True, 'anyframe': False, 'alignment': 'integer', 'stack_method': 'average', 'minrejection': 1, 'maxrejection': 1, 'klow': 3.0, 'khigh': 3.0, 'kiter': 999, 'dither': True, 'compute': False, 'fringing': True, 'offset': 3.0, 'generate_idp': False} 605s Docstring: Extraction of scientific spectra 605s 605s This recipe is used to reduce scientific spectra using the extraction 605s mask and the products created by the recipe vimos_calib. The spectra 605s are bias subtracted, flat fielded (if a normalised flat field is 605s specified) and remapped eliminating the optical distortions. The 605s wavelength calibration can be optionally upgraded using a number of 605s sky lines: if no sky lines catalog of wavelengths is specified, an 605s internal one is used instead. If the alignment to the sky lines is 605s performed, the input dispersion coefficients table is upgraded and 605s saved to disk, and a new CCD wavelengths map is created. A 605s configuration table (typically depending on the grism in use) may also 605s be specified: this table contains a default recipe parameter setting 605s to control the way spectra are extracted for a specific instrument 605s mode, as it is used for automatic run of the pipeline on Paranal and 605s in Garching. If this table is specified, it will modify the default 605s recipe parameter setting, with the exception of those parameters which 605s have been explicitly modifyed on the command line. If a configuration 605s table is not specified, the input recipe parameters values will always 605s be read from the command line, or from an esorex configuration file if 605s present, or from their generic default values (which are rarely 605s meaningful). Either a scientific or a standard star exposure can be 605s specified in input. Only in case of a standard star exposure input, 605s the atmospheric extinction table and a table with the physical fluxes 605s of the observed standard star must be specified in input, and a 605s spectro-photometric table is created in output. This table can then be 605s input again to this recipe, always with an atmospheric extinction 605s table, and if a photometric calibration is requested then flux 605s calibrated spectra (in units of erg/cm/cm/s/Angstrom) are also written 605s in output. Input files: DO category: Type: 605s Explanation: Required: MOS_SCIENCE Raw 605s Scientific exposure Y or MOS_STANDARD Raw 605s Standard star exposure Y MASTER_BIAS Calib 605s Master bias Y SKY_LINE_CATALOG Calib 605s Sky lines catalog . MOS_MASTER_SCREEN_FLAT Calib 605s Normalised flat field . MOS_DISP_COEFF Calib 605s Inverse dispersion Y MOS_CURV_COEFF Calib 605s Spectral curvature Y MOS_SLIT_LOCATION Calib 605s Slits positions table Y CONFIG_TABLE Calib 605s Configuration table . In case MOS_STANDARD is specified in 605s input, EXTINCT_TABLE Calib Atmospheric 605s extinction Y STD_FLUX_TABLE Calib Standard star 605s flux Y TELLURIC_CONTAMINATION Calib Telluric regions 605s list . In case a photometric calibration is requested for 605s scientific data, the following inputs are mandatory: 605s EXTINCT_TABLE Calib Atmospheric extinction Y 605s MOS_SPECPHOT_TABLE Calib Response curves Y If 605s requested for standard star data, the SPECPHOT_TABLE can be dropped: 605s in this case the correction is applied using the SPECPHOT_TABLE 605s produced in the same run. Output files (acronym _STD_ replaces 605s _SCI_ and _STANDARD_ replaces _SCIENCE_ in case input is MOS_STANDARD 605s rather than MOS_SCIENCE): DO category: Data type: 605s Explanation: MOS_SCIENCE_REDUCED Image Extracted 605s scientific spectra MOS_SCI_SKY_REDUCED Image Extracted 605s sky spectra MOS_SCI_ERROR_REDUCED Image Errors on extracted 605s spectra MOS_UNMAPPED_SCIENCE Image Sky subtracted 605s scientific spectra MOS_SCIENCE_EXTRACTED Image Rectified 605s scientific spectra MOS_SCIENCE_SKY_EXTRACTED Image Rectified 605s science spectra with sky MOS_SCIENCE_SKY Image 605s Rectified sky spectra MOS_SCI_UNMAPPED_SKY Image Sky on 605s CCD MOS_SCI_GLOBAL_SKY_SPECTRUM Table Global sky spectrum 605s OBJECT_SCI_TABLE Table Positions of detected objects 605s Only if fringing correction is requested (dithered exposures): 605s MOS_SCI_FRINGES Image Fringe map Only if the sky- 605s alignment of the wavelength solution is requested: 605s MOS_SCI_SKYLINES_OFFSETS_SLIT Table Sky lines offsets 605s MOS_SCI_DISP_COEFF_SKY Table Upgraded dispersion coefficients 605s MOS_SCI_WAVELENGTH_MAP_SKY Image Upgraded wavelength map Only 605s if a MOS_STANDARD is specified in input: MOS_SPECPHOT_TABLE 605s Table Efficiency and response curves Only if MOS_SPECPHOT_TABLE or 605s MOS_MASTER_RESPONSE are specified in input: MOS_SCIENCE_FLUX_REDUCED 605s Image Flux calibrated scientific spectra MOS_SCI_ERROR_FLUX_REDUCED 605s Image Errors on flux calibrated spectra MOS_SCIENCE_FLUX_EXTRACTED 605s Image Flux calibrated slit spectra 605s 605s Parameters: 605s skyalign: Polynomial order for sky lines alignment, or -1 605s to avoid alignment (int; default: -1) 605s flatfield: Apply flat field (bool; default: True) 605s skyglobal: Subtract global sky spectrum from CCD (bool; 605s default: False) 605s skymedian: Sky subtraction from extracted slit spectra 605s (bool; default: False) 605s skylocal: Sky subtraction from CCD slit spectra (bool; 605s default: True) 605s cosmics: Eliminate cosmic rays hits (only if global or 605s local sky subtraction is also requested) (bool; 605s default: True) 605s slit_margin: Number of pixels to exclude at each slit in 605s object detection and extraction (int; default: 3) 605s ext_radius: Maximum extraction radius for detected objects 605s (pixel) (int; default: 6) 605s cont_radius: Minimum distance at which two objects of equal 605s luminosity do not contaminate each other (pixel) 605s (int; default: 0) 605s ext_mode: Object extraction method: 0 = aperture, 1 = Horne 605s optimal extraction (int; default: 1) 605s detection: Object detection threshold (ADU) (float; default: 605s 2.0) 605s resp_fit_nknots: Number of knots in spline fitting of the 605s instrument response. (-1: No fitting. -2: Read 605s from grism table) (int; default: -2) 605s resp_fit_degree: Degree of polynomial in fitting of the instrument 605s response. (-1: No fitting. -2: Read from grism 605s table) (int; default: -2) 605s resp_ignore_mode: Types of lines/regions to ignore in response. 605s Valid ones are 'stellar_absorption', 'telluric' 605s and 'command_line' (from parameter 605s resp_ignore_lines) (str; default: 605s 'stellar_absorption,telluric,command_line') 605s resp_ignore_points: Extra lines/regions to ignore in response. Use a 605s comma separated list of values. A range can be 605s specified like 4500.0-4600.0 (str; default: '') 605s resp_use_flat_sed: Use the flat SED to normalise the observed 605s spectra. Value are true, false, grism_table. 605s (str; default: 'grism_table') 605s resp_shift: The extracted standard star will be shifted these 605s many angstroms before using it to compute the 605s response. This is useful for observed std stars 605s not centered in the slits. Positive values will 605s shift the spectrum to the red. Shift is given in 605s Angstroms but no fraction of pixels will be 605s shifted. (float; default: 0.0) 605s time_normalise: Normalise output spectra by the exposure time 605s (bool; default: True) 605s anyframe: Look for a standard star in any frame classified 605s as MOS_STANDARD (bool; default: False) 605s alignment: Type of alignment of dithered frames, either to 605s the nearest neighbour pixel or to fractions of 605s pixel (str; default: 'integer') 605s stack_method: Frames combination method (str; default: 605s 'average') 605s minrejection: Number of lowest values to be rejected (int; 605s default: 1) 605s maxrejection: Number of highest values to be rejected (int; 605s default: 1) 605s klow: Low threshold in ksigma method (float; default: 605s 3.0) 605s khigh: High threshold in ksigma method (float; default: 605s 3.0) 605s kiter: Max number of iterations in ksigma method (int; 605s default: 999) 605s dither: Align dithered frames before stacking(for 605s multiple input frames) (bool; default: True) 605s compute: Compute offsets of dithered images from detected 605s objects (true), or read offsets from header 605s (false) (bool; default: False) 605s fringing: Apply fringing correction (only for dithered 605s observations) (bool; default: True) 605s offset: Minimum required offset between exposures for 605s applying the sky fringing correction. (float; 605s default: 3.0) 605s generate_idp: Generate IDP products (bool; default: False) 605s Author: Carlo Izzo 605s 605s 605s Recipe vimos_ima_dark: 605s version 4.1.7 605s Parameters: {'combtype': 'median', 'scaletype': 'exptime', 'xrej': True, 'thresh': 5.0, 'ncells': 8, 'prettynames': False} 605s Docstring: Dark combination for imaging 605s 605s vimos_ima_dark -- VIMOS dark combine recipe. Combine a list of dark 605s frames into a mean dark frame. Optionally compare the output frame to 605s a reference dark frame The program accepts the following files in the 605s SOF: Tag Description ---------------------- 605s ------------------------------------------------- DARK 605s A list of raw dark images MASTER_BIAS A master bias 605s frame REFERENCE_DARK Optional reference dark frame 605s MASTER_BPM Optional master bad pixel map or MASTER_CONF 605s Optional master confidence map If no reference dark frame is made 605s available, then no comparison will be done. This means there will be 605s no output difference image and no stats tableIf neither a master bad 605s pixel map nor confidence map is provided then thestats will be done 605s assuming all pixels are good 605s 605s Parameters: 605s combtype: Combination algorithm (str; default: 'median') 605s scaletype: Scaling algorithm (str; default: 'exptime') 605s xrej: True if using extra rejection cycle (bool; default: 605s True) 605s thresh: Rejection threshold in sigma above background (float; 605s default: 5.0) 605s ncells: Number of cells for diff image stats (int; default: 8) 605s prettynames: Use pretty output file names? (bool; default: False) 605s Author: Jim Lewis 605s 605s 605s Recipe vmdark: 605s version 4.1.7 605s Parameters: {'AllowSingleFrames': True, 'StackMethod': 'Median', 'KSigmaLow': 5.0, 'KSigmaHigh': 5.0, 'MinRejection': 1, 'MaxRejection': 1, 'BiasMethod': 'Zmaster', 'CleanBadPixel': False, 'CleanCosmic': True, 'CosmicThreshold': 4.0, 'CosmicRatio': 2.0, 'ComputeQC': True} 605s Docstring: Create a master dark from set of raw dark frames. 605s 605s This recipe is used to create a master dark frame from a set of raw 605s dark frames. Input files: DO category: Type: Explanation: 605s Required: DARK Raw Dark exposure Y 605s MASTER_BIAS Calib Master bias Y CCD_TABLE Calib 605s Bad pixel table . Output files: DO category: Data type: 605s Explanation: MASTER_DARK FITS image Master dark A CCD table must 605s be specified only if a bad pixel cleaning is requested. For more 605s details, please refer to the VIMOS Pipeline User's Guide. 605s 605s Parameters: 605s AllowSingleFrames: Frame combination method is ignored. (bool; 605s default: True) 605s StackMethod: Frame combination method. (str; default: 'Median') 605s KSigmaLow: Low threshold for K-sigma clipping method. (float; 605s default: 5.0) 605s KSigmaHigh: High threshold for K-sigma clipping method. 605s (float; default: 5.0) 605s MinRejection: Number of lowest rejected values for rejection 605s method. (int; default: 1) 605s MaxRejection: Number of highest rejected values for rejection 605s method. (int; default: 1) 605s BiasMethod: Bias removal method. (str; default: 'Zmaster') 605s CleanBadPixel: Bad pixel correction on master dark. (bool; 605s default: False) 605s CleanCosmic: Cosmic ray events cleaning from raw darks. (bool; 605s default: True) 605s CosmicThreshold: Threshold to identify cosmic rays candidates. 605s (float; default: 4.0) 605s CosmicRatio: Min ratio between peak and nearby pixels for a 605s cosmic ray. (float; default: 2.0) 605s ComputeQC: Compute QC1 parameters (bool; default: True) 605s Author: ESO VIMOS Pipeline Team 605s 605s 605s Recipe vmbias: 605s version 4.1.7 605s Parameters: {'AllowSingleFrames': True, 'StackMethod': 'Median', 'KSigmaLow': 5.0, 'KSigmaHigh': 5.0, 'MinRejection': 1, 'MaxRejection': 1, 'RemoveOverscan': True, 'CleanBadPixel': False, 'CleanCosmic': False, 'ComputeQC': True} 605s Docstring: Create a master bias from set of raw bias frames. 605s 605s This recipe is used to create a master bias frame from a set of raw 605s bias frames. Input files: DO category: Type: Explanation: 605s Required: BIAS Raw Bias exposure Y 605s CCD_TABLE Calib Bad pixel table . Output files: DO 605s category: Data type: Explanation: MASTER_BIAS FITS image Master 605s bias A CCD table must be specified only if a bad pixel cleaning is 605s requested. For more details, please refer to the VIMOS Pipeline 605s User's Guide. 605s 605s Parameters: 605s AllowSingleFrames: Frame combination method is ignored. (bool; 605s default: True) 605s StackMethod: Frame combination method (str; default: 'Median') 605s KSigmaLow: Low threshold for K-sigma clipping method (float; 605s default: 5.0) 605s KSigmaHigh: High threshold for K-sigma clipping method (float; 605s default: 5.0) 605s MinRejection: Number of lowest rejected values for rejection 605s method (int; default: 1) 605s MaxRejection: Number of highest rejected values for rejection 605s method (int; default: 1) 605s RemoveOverscan: Remove overscan regions from master bias (bool; 605s default: True) 605s CleanBadPixel: Bad pixel correction on master bias (bool; 605s default: False) 605s CleanCosmic: Cosmic ray removal from each raw bias (bool; 605s default: False) 605s ComputeQC: Compute QC1 parameters (bool; default: True) 605s Author: ESO VIMOS Pipeline Team 605s 605s 605s Recipe vmifustandard: 605s version 4.1.7 605s Parameters: {'BiasMethod': 'Zmaster', 'CleanBadPixel': False, 'UseSkylines': True, 'ResponseOrder': 5, 'ReduceAnyFrame': False, 'ComputeQC': True} 605s Docstring: Extract a standard star spectrum. 605s 605s This recipe extracts IFU standard star fiber spectra using the input 605s extraction mask, after aligning it to the brightest fiber spectra 605s detected on the input exposure. The extracted spectra are then 605s resampled at a constant wavelength step, after aligning the input 605s wavelength calibration to the positions of a set of identified sky 605s lines. The extracted spectra are finally corrected for the relative 605s differences in transmission from fiber to fiber, and summed together. 605s Input files: DO category: Type: Explanation: 605s Required: IFU_STANDARD Raw Standard star spectra 605s Y MASTER_BIAS Calib Master bias Y 605s IFU_TRACE Calib Extraction mask Y 605s IFU_IDS Calib Wavelength calibration Y 605s IFU_TRANSMISSION Calib Transmission correction Y 605s EXTINCT_TABLE Calib Atmospheric extinction Y 605s STD_FLUX_TABLE Calib Standard star fluxes Y 605s CCD_TABLE Calib Bad pixel table . 605s Output files: DO category: Data type: Explanation: 605s IFU_STANDARD_REDUCED FITS image Reduced standard star spectra 605s IFU_FOV FITS image Reconstructed field-of-view image 605s IFU_STANDARD_EXTRACTED FITS table Total standard star spectrum 605s IFU_SCIENCE_SKY FITS table Total sky spectrum 605s IFU_SPECPHOT_TABLE FITS table Efficiency and response curves 605s The extraction mask, the wavelength calibration, and the relative 605s transmission table, are those generated by the recipe vmifucalib. A 605s CCD table must be specified only if a bad pixel cleaning is requested. 605s The spectra extracted from the fibers on the standard star are added 605s and compared to the catalog fluxes of the same star, to obtain the 605s efficiency curve and the response curve to use for flux calibration. 605s The procedure is the same as the one applied in the case of MOS data, 605s by recipe vmmosstandard. 605s 605s Parameters: 605s BiasMethod: Bias removal method. (str; default: 'Zmaster') 605s CleanBadPixel: Bad pixel correction on master flat field. (bool; 605s default: False) 605s UseSkylines: Use sky lines to refine the wavelength calibration 605s (bool; default: True) 605s ResponseOrder: Order of the polynomial used to smooth the instrument 605s response curve. (int; default: 5) 605s ReduceAnyFrame: Reduce any frame. (bool; default: False) 605s ComputeQC: Compute QC1 parameters (bool; default: True) 605s Author: ESO VIMOS Pipeline Team 605s 605s 605s Recipe vimos_ima_science: 605s version 4.1.7 605s Parameters: {'savecat': False, 'savemstd': False, 'preview_only': False, 'minphotom': 1, 'prettynames': False, 'chop_crud': 'hardconf_pix', 'cdssearch_astrom': 'none', 'cdssearch_photom': 'none', 'ignore_fringe': False, 'stk_cat_ipix': 10, 'stk_cat_thresh': 1.5, 'stk_cat_icrowd': True, 'stk_cat_rcore': 10.0, 'stk_cat_nbsize': 128, 'stk_lthr': 3.0, 'stk_hthr': 3.0, 'stk_method': 'linear', 'stk_seeing': False, 'stk_fast': 'auto', 'stk_nfst': 16, 'cacheloc': '.', 'magerrcut': 100.0} 605s Docstring: Science processing for imaging 605s 605s vimos_ima_science -- VIMOS science recipe. Take a list of science 605s frames and correct them to remove bias, dark and flat field 605s signatures. Optionally defringe the reddest filter images. Stack 605s jitter sequences. Astrometrically and photometrically calibrate the 605s stacks The program accepts the following files in the SOF: Tag 605s Description ------------------------------------------------------ 605s ----------------- OBJECT A list of raw science 605s images MASTER_BIAS A master bias frame MASTER_DARK 605s A master dark frame MASTER_TWILIGHT_FLAT A master flat frame 605s MASTER_CONF A master confidence map MASTER_FRINGE 605s A master fringe map (optional) MASTER_FRINGE_VAR A master 605s fringe variance map (optional) MASTER_READGAIN A master 605s readgain table MASTER_2MASS_CATALOGUE_ASTROM A master 2MASS index 605s for astrometry or MASTER_PPMXL_CATALOGUE_ASTROM A master PPMXL 605s index for astrometry or MASTER_APASS_CATALOGUE_ASTROM A master 605s APASS index for astrometry or MASTER_LOCAL_CATALOGUE_ASTROM A 605s master local index for astrometry MASTER_APASS_CATALOGUE_PHOTOM A 605s master APASS index for photometry or MASTER_LOCAL_CATALOGUE_PHOTOM 605s A master local index for photometry or OBJECT_CATALOGUE_STD A 605s master processed standard star image or table MATCHSTD_PHOTOM 605s A master photometric matched standards table (optional) 605s SCHLEGEL_MAP_NORTH Northern Schlegel Map SCHLEGEL_MAP_SOUTH 605s Southern Schlegel Map PHOTCAL_TAB A photometric 605s calibration table All of these are required unless specified 605s otherwise. 605s 605s Parameters: 605s savecat: Save catalogue? (bool; default: False) 605s savemstd: Save matched standard catalogues? (bool; default: 605s False) 605s preview_only: Preview only? (bool; default: False) 605s minphotom: Minimum stars for photometry solution (int; 605s default: 1) 605s prettynames: Use pretty product names? (bool; default: False) 605s chop_crud: Chop crud method (str; default: 'hardconf_pix') 605s cdssearch_astrom: CDS astrometric catalogue (str; default: 'none') 605s cdssearch_photom: CDS photometric catalogue (str; default: 'none') 605s ignore_fringe: Ignore provided fringe frame? (bool; default: 605s False) 605s stk_cat_ipix: Minimum pixel area for each detected object (int; 605s default: 10) 605s stk_cat_thresh: Detection threshold in sigma above sky (float; 605s default: 1.5) 605s stk_cat_icrowd: Use deblending? (bool; default: True) 605s stk_cat_rcore: Value of Rcore in pixels (float; default: 10.0) 605s stk_cat_nbsize: Background smoothing box size (int; default: 128) 605s stk_lthr: Low rejection threshold (float; default: 3.0) 605s stk_hthr: Upper rejection threshold (float; default: 3.0) 605s stk_method: Stacking method (str; default: 'linear') 605s stk_seeing: Weight by seeing? (bool; default: False) 605s stk_fast: Stack using fast algorithm? (str; default: 'auto') 605s stk_nfst: Nframes to stack in fast mode (int; default: 16) 605s cacheloc: Location for standard star cache (str; default: 605s '.') 605s magerrcut: Magnitude error cut (float; default: 100.0) 605s Author: Jim Lewis 605s 605s 605s Recipe vmifucombine: 605s version 4.1.7 605s Parameters: {} 605s Docstring: Combine partial IFU field-of-views reconstructed by vmifuscience from 605s different quadrants. 605s 605s This recipe is used to compose into a single image the reconstructed 605s images of the IFU field-of-view from different VIMOS quadrants. Such 605s images are created by the recipes vmifuscience and vmifustandard. The 605s input images must belong to different quadrants, so that they cannot 605s be more than 4. The images are simply summed together: in fact, all 605s field-of-view images are always 80x80 pixels, with only the sector 605s corresponding to one quadrant having intensities that differ from 605s zero. For more details, please refer to the VIMOS Pipeline User's 605s Guide. 605s 605s No parameters 605s Author: ESO VIMOS Pipeline Team 605s 605s 605s Recipe vmdet: 605s version 4.1.7 605s Parameters: {'CreateBadPixelMap': True, 'CreateErrorImage': False, 'DetectionThreshold': 5.0, 'DetectionMode': 'Intolerant', 'ComputeQC': True} 605s Docstring: Determine RON, gain, and bad pixels from a set of flat field 605s exposures. 605s 605s This recipe is used to estimate the read-out-noise (RON) and the gain 605s of the CCD, and to determine the positions of the bad pixels. The 605s input SOF should contain at least five pairs of flat field exposures, 605s all belonging to the same quadrant, each pair corresponding to a 605s different exposure time. The flat fields can be produced either in 605s imaging or in MOS mode. In MOS mode a HR grism is used, in order to 605s illuminate the CCD also beyond the central region used in direct 605s imaging mode, but no mask is inserted at the telescope focal plane. 605s This type of exposure cannot really be considered a spectral flat 605s field, because the CCD is exposed to white light (i.e., without a 605s wavelength dependency along the dispersion direction). The flat fields 605s generated for the purpose of determining the detector properties are 605s assigned the DO category DETECTOR_PROPERTIES, to distinguish them from 605s the more common IMG_SCREEN_FLAT or MOS_SCREEN_FLAT that are used to 605s produce master calibrations. Input files: DO category: 605s Type: Explanation: Required: DETECTOR_PROPERTIES Raw 605s Flat field Y MASTER_BIAS Calib Master bias 605s Y Output files: DO category: Data type: Explanation: 605s CCD_TABLE FITS table Bad pixel table (none) 605s FITS image Bad pixel image (none) FITS image 605s Error image Only the primary product, the bad pixel table, is copied 605s (or moved) to the product directory. Other products are generated only 605s on request (typically for debug purposes) and are not assigned a DO 605s category as they would not be used anywhere in further data processing 605s steps. For more details, please refer to the VIMOS Pipeline User's 605s Guide. 605s 605s Parameters: 605s CreateBadPixelMap: Bad pixel map creation (bool; default: True) 605s CreateErrorImage: Response slope uncertainty map creation (bool; 605s default: False) 605s DetectionThreshold: Threshold in determination of bad pixels (float; 605s default: 5.0) 605s DetectionMode: Bad pixel detection method (str; default: 605s 'Intolerant') 605s ComputeQC: Compute QC1 parameters. (bool; default: True) 605s Author: ESO VIMOS Pipeline Team 605s 605s 605s Recipe vmspphot: 605s version 4.1.7 605s Parameters: {'ApplyResponse': True} 605s Docstring: Apply to IFU or MOS 1D-extracted spectra a flux correction. 605s 605s This recipe can be used to apply a spectro-photometric flux 605s calibration to any number of 1D-extracted spectral frames generated by 605s the recipes vmmosobsstare, vmmosobsjitter, and vmifuscience. Input 605s files: DO category: Type: Explanation: 605s Required: MOS_SCIENCE_REDUCED or IFU_SCIENCE_REDUCED Product 605s Extracted MOS or IFU spectra Y EXTINCT_TABLE Calib 605s Atmospheric extinction Y MOS_SPECPHOT_TABLE or 605s IFU_SPECPHOT_TABLE Calib Response curve . 605s Output files: DO category: Data type: Explanation: 605s MOS_SCIENCE_FLUX_REDUCED or IFU_SCIENCE_FLUX_REDUCED FITS image 605s Flux calibrated objects spectra For more details, please refer to the 605s VIMOS Pipeline User's Guide. 605s 605s Parameters: 605s ApplyResponse: Apply instrument response. (bool; default: True) 605s Author: ESO VIMOS Pipeline Team 605s 605s 605s Recipe vimos_ima_bias: 605s version 4.1.7 605s Parameters: {'combtype': 'median', 'xrej': True, 'thresh': 5.0, 'ncells': 64, 'prettynames': False} 605s Docstring: Bias combination for imaging 605s 605s vimos_ima_bias -- VIMOS bias combine recipe. Combine a list of bias 605s frames into a mean bias frame. Optionally compare the output frame to 605s a reference bias frame The program accepts the following files in the 605s SOF: Tag Description ---------------------- 605s ------------------------------------------------- BIAS 605s A list of raw bias images REFERENCE_BIAS Optional reference 605s bias frame If no reference bias frame is made available, then no 605s comparison will be done. This means there will be no output difference 605s image or stats table. 605s 605s Parameters: 605s combtype: Combination algorithm (str; default: 'median') 605s xrej: True if using extra rejection cycle (bool; default: 605s True) 605s thresh: Rejection threshold in sigma above background (float; 605s default: 5.0) 605s ncells: Number of cells for diff image stats (int; default: 64) 605s prettynames: Use pretty output file names? (bool; default: False) 605s Author: Jim Lewis 605s 605s 605s autopkgtest [01:03:57]: test test-recipe.py: -----------------------] 611s autopkgtest [01:04:03]: test test-recipe.py: - - - - - - - - - - results - - - - - - - - - - 611s test-recipe.py PASS (superficial) 612s autopkgtest [01:04:04]: @@@@@@@@@@@@@@@@@@@@ summary 612s test-recipe.py PASS (superficial)