Result for D1451680F9D3DA7F47DE73E9E95EA1E4F1B04E5D

Query result

Key Value
FileName./usr/share/doc/cpl-plugin-hawki/changelog.Debian.gz
FileSize364
MD5EB3E12DD8198E7C41C8201C5280BDA85
SHA-1D1451680F9D3DA7F47DE73E9E95EA1E4F1B04E5D
SHA-25645E00591A09526455E5D4195EC465006900BEC8CD94D25202B5DC5214A0BA710
SSDEEP6:Xtoi813EeEfOPcWesQ+ERUGg2QWSH/O5tqTYa7MmVH9dFwktr0L4JlparFU9r/n:XfkkfcsM9Ggu0Uqtt9jwWwLKzaroj
TLSHT1F4E0600E89C8F06146A51B9AEEC00B4788040FC220303A403AA0CA0725D1F2083BAEE5
hashlookup:parent-total13
hashlookup:trust100

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Parents (Total: 13)

The searched file hash is included in 13 parent files which include package known and seen by metalookup. A sample is included below:

Key Value
FileSize225126
MD5CF9FA4C7CE9F844C3D7E55B9BA5844E5
PackageDescriptionESO data reduction pipeline for HAWK-I This is the data reduction pipeline for the HAWK-I instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO). . HAWK-I is a near-infrared (0.85-2.5 μm ) wide-field imager. It is being offered for the first time in Period 81. The instrument is cryogenic (120 K, detectors at 80 K) and has a full reflective design. The light passes four mirrors and two filter wheels before hitting a mosaic of four Hawaii 2RG 2048 * 2048 pixels detectors. The final F-ratio is F/4.36 ( 1 arcsec on the sky corresponds to 169 μm on the detector).
PackageMaintainerDebian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion1.8.14+dfsg-2
SHA-1568F0F9D3C91E620D966913560B7CBEA3960D69E
SHA-256B4D26EE3EA7C0A8629B579288D4950615ED647084080BEA567F7948A39315B0B
Key Value
FileSize235558
MD5B07F1716E526AC3171FDD3D19B6361F7
PackageDescriptionESO data reduction pipeline for HAWK-I This is the data reduction pipeline for the HAWK-I instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO). . HAWK-I is a near-infrared (0.85-2.5 μm ) wide-field imager. It is being offered for the first time in Period 81. The instrument is cryogenic (120 K, detectors at 80 K) and has a full reflective design. The light passes four mirrors and two filter wheels before hitting a mosaic of four Hawaii 2RG 2048 * 2048 pixels detectors. The final F-ratio is F/4.36 ( 1 arcsec on the sky corresponds to 169 μm on the detector).
PackageMaintainerDebian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion1.8.14+dfsg-2
SHA-1FF4A18E1FFAB4BD4D31FE1BE2C866401316953B6
SHA-256FF0CE99CD7E6398A4E477532FD9D5B3A7D05EA786069F1522624BC3E1B406AAA
Key Value
FileSize220538
MD531D6CCA4666BB9CF91D70F85DF43457A
PackageDescriptionESO data reduction pipeline for HAWK-I This is the data reduction pipeline for the HAWK-I instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO). . HAWK-I is a near-infrared (0.85-2.5 μm ) wide-field imager. It is being offered for the first time in Period 81. The instrument is cryogenic (120 K, detectors at 80 K) and has a full reflective design. The light passes four mirrors and two filter wheels before hitting a mosaic of four Hawaii 2RG 2048 * 2048 pixels detectors. The final F-ratio is F/4.36 ( 1 arcsec on the sky corresponds to 169 μm on the detector).
PackageMaintainerDebian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion1.8.14+dfsg-2
SHA-1260CAF94A6F4CE159F52A9364FA6A81610CC3619
SHA-256A2E741FAF01616FAD42B2B5AE51B4AB0CAF93A19207EB47B6D178189F6DF71C3
Key Value
FileSize184096
MD581950D6B382DAA6D7864B030252CD235
PackageDescriptionESO data reduction pipeline for HAWK-I This is the data reduction pipeline for the HAWK-I instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO). . HAWK-I is a near-infrared (0.85-2.5 μm ) wide-field imager. It is being offered for the first time in Period 81. The instrument is cryogenic (120 K, detectors at 80 K) and has a full reflective design. The light passes four mirrors and two filter wheels before hitting a mosaic of four Hawaii 2RG 2048 * 2048 pixels detectors. The final F-ratio is F/4.36 ( 1 arcsec on the sky corresponds to 169 μm on the detector).
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion1.8.14+dfsg-2
SHA-13A7129DA572757788BD93ABECEE5431E938EB6C5
SHA-256F8F6FC29BA3956C3DCD876B690A995927917F6A0CE60DD48F42A86EE81F81362
Key Value
FileSize196654
MD50A2841A209224E251882DC665A2EB149
PackageDescriptionESO data reduction pipeline for HAWK-I This is the data reduction pipeline for the HAWK-I instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO). . HAWK-I is a near-infrared (0.85-2.5 μm ) wide-field imager. It is being offered for the first time in Period 81. The instrument is cryogenic (120 K, detectors at 80 K) and has a full reflective design. The light passes four mirrors and two filter wheels before hitting a mosaic of four Hawaii 2RG 2048 * 2048 pixels detectors. The final F-ratio is F/4.36 ( 1 arcsec on the sky corresponds to 169 μm on the detector).
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion1.8.14+dfsg-2
SHA-1B2471E6CD8501B5A1B43B2EC659031EB8B478ED9
SHA-256332FEEC118B1D561CAAF58D189027595FB6AF81FF18CF0C8BEF702BFC56BB89A
Key Value
FileSize255070
MD560BA19F6BF0377B8FBA3875CEE3462A5
PackageDescriptionESO data reduction pipeline for HAWK-I This is the data reduction pipeline for the HAWK-I instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO). . HAWK-I is a near-infrared (0.85-2.5 μm ) wide-field imager. It is being offered for the first time in Period 81. The instrument is cryogenic (120 K, detectors at 80 K) and has a full reflective design. The light passes four mirrors and two filter wheels before hitting a mosaic of four Hawaii 2RG 2048 * 2048 pixels detectors. The final F-ratio is F/4.36 ( 1 arcsec on the sky corresponds to 169 μm on the detector).
PackageMaintainerDebian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion1.8.14+dfsg-2
SHA-1B92D27F63AADD6F46370195B071DEAE89D0852C2
SHA-256FEB09DDCD143CAB6B8E974186BC63E8D1107C0E2F52B5913BEA7451BE3149AF1
Key Value
FileSize165216
MD5E12BAB3979675ED66624430A2F31F9B7
PackageDescriptionESO data reduction pipeline for HAWK-I This is the data reduction pipeline for the HAWK-I instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO). . HAWK-I is a near-infrared (0.85-2.5 μm ) wide-field imager. It is being offered for the first time in Period 81. The instrument is cryogenic (120 K, detectors at 80 K) and has a full reflective design. The light passes four mirrors and two filter wheels before hitting a mosaic of four Hawaii 2RG 2048 * 2048 pixels detectors. The final F-ratio is F/4.36 ( 1 arcsec on the sky corresponds to 169 μm on the detector).
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion1.8.14+dfsg-2
SHA-14A0285D01B6819014CE86C3B6D1123F6534E36C5
SHA-2564F99F67FCA1A126F63922C859CAC6A04492F38E7C20EEF6402A54CC39E32AB46
Key Value
FileSize69358
MD50AEB3C469494D454D0FDDF9802125B33
PackageDescriptionESO data reduction pipeline documentation for HAWK-I This package contains the HTML documentation and manpages for the data reduction pipeline for the HAWK-I instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO).
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecpl-plugin-hawki-doc
PackageSectiondoc
PackageVersion1.8.14+dfsg-2
SHA-136B5395DBAF034DB209FC7EF056FCCCB9687D15D
SHA-2566552369E33ADB6D000DB99B733B83E8B0CCFD339A9E6D19ABA39CAE51F4E203A
Key Value
FileSize182644
MD5B913E5F643EB90DB738980D1B4AAD78B
PackageDescriptionESO data reduction pipeline for HAWK-I This is the data reduction pipeline for the HAWK-I instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO). . HAWK-I is a near-infrared (0.85-2.5 μm ) wide-field imager. It is being offered for the first time in Period 81. The instrument is cryogenic (120 K, detectors at 80 K) and has a full reflective design. The light passes four mirrors and two filter wheels before hitting a mosaic of four Hawaii 2RG 2048 * 2048 pixels detectors. The final F-ratio is F/4.36 ( 1 arcsec on the sky corresponds to 169 μm on the detector).
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion1.8.14+dfsg-2
SHA-1FA7B88CE6E858920EE04E01091AEADABC91BEEE8
SHA-256D9CB21642275832CBB1599E32BE54633E9B29C8FFD3316B6EE9E95706D7E4F26
Key Value
FileSize40996
MD56C54AF5BED884B151907D366EE8FB5CA
PackageDescriptionESO data reduction pipeline calibration data downloader for HAWK-I This package downloads calibration data of the data reduction pipeline for the HAWK-I instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO).
PackageMaintainerDebian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
PackageNamecpl-plugin-hawki-calib
PackageSectionscience
PackageVersion1.8.14+dfsg-2
SHA-1399961F8181DF34C5C568B847D3BA22095067DAC
SHA-2569E510262520CF89655ACE83499AD6DE863E93CB54B948D227E300CF3AED22976
Key Value
FileSize195760
MD5AD2C0CE7BFA6DD0C55A03053260B56BB
PackageDescriptionESO data reduction pipeline for HAWK-I This is the data reduction pipeline for the HAWK-I instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO). . HAWK-I is a near-infrared (0.85-2.5 μm ) wide-field imager. It is being offered for the first time in Period 81. The instrument is cryogenic (120 K, detectors at 80 K) and has a full reflective design. The light passes four mirrors and two filter wheels before hitting a mosaic of four Hawaii 2RG 2048 * 2048 pixels detectors. The final F-ratio is F/4.36 ( 1 arcsec on the sky corresponds to 169 μm on the detector).
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion1.8.14+dfsg-2
SHA-1086A952CA52A913571A4B157A2FACE4144827EDA
SHA-2562D7C4EE843C799609FC589F29F835C883F9AA2BE52375FA434E627D2452C14C0
Key Value
FileSize107930
MD5926A09068B7676BFE0DCC65A5D64BE59
PackageDescriptionESO data reduction pipeline documentation for HAWK-I This package contains the HTML documentation and manpages for the data reduction pipeline for the HAWK-I instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO).
PackageMaintainerDebian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
PackageNamecpl-plugin-hawki-doc
PackageSectiondoc
PackageVersion1.8.14+dfsg-2
SHA-1534194063848316CBFE069A4447D605267492D30
SHA-256C1632081A6476F7D56FF16F8F10C37C85B05618C00CDDC757C73FF1FBD80248B
Key Value
FileSize191810
MD5F94E1EDE633CCEDCBE31E09724D85AA3
PackageDescriptionESO data reduction pipeline for HAWK-I This is the data reduction pipeline for the HAWK-I instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO). . HAWK-I is a near-infrared (0.85-2.5 μm ) wide-field imager. It is being offered for the first time in Period 81. The instrument is cryogenic (120 K, detectors at 80 K) and has a full reflective design. The light passes four mirrors and two filter wheels before hitting a mosaic of four Hawaii 2RG 2048 * 2048 pixels detectors. The final F-ratio is F/4.36 ( 1 arcsec on the sky corresponds to 169 μm on the detector).
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion1.8.14+dfsg-2
SHA-1DC1833126CD4314E1C140EAE317204641EC0C86B
SHA-25687DAF936BC5231E6477B366A7A32736D2E8ECF099140D10468051527FE345A49