Result for EF658250D3AC44DC35A057586F6F61E132C39F71

Query result

Key Value
FileName./usr/share/doc/cpl-plugin-hawki/changelog.gz
FileSize72187
MD5F242E4698CE751B5751F9F44A2F8129C
SHA-1EF658250D3AC44DC35A057586F6F61E132C39F71
SHA-2568374DBF007AA0A28545D4A406A613CF4D19CE2117D74B16A13F0AC5FD006271D
SSDEEP1536:FBwKi4RbGNMIWz2ZNfMX7Ji3fuD+syEPzu+i9yTUE60B89:7wKNRbA02Zh+9F+38u+PUj0B89
TLSHT108630277D4D07C2FFA2EA4B624376D57860DF660449ECF3A2F5849AD8EEB18049D48A0
hashlookup:parent-total12
hashlookup:trust100

Network graph view

Parents (Total: 12)

The searched file hash is included in 12 parent files which include package known and seen by metalookup. A sample is included below:

Key Value
FileSize477396
MD536D3852665BA37B7D3A54BDF92495CD3
PackageDescriptionESO data reduction pipeline for the HAWK-I instrument 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
PackageVersion2.4.3+dfsg-1
SHA-1FB4CFFDCD3D3AC67745E1A84542709CE1909378B
SHA-256BD03FA5F24D6267A89ED763C03A764AAAFADAFC91D2D1AE4BA51802A7659DA82
Key Value
FileSize459464
MD5BF5AA2AF1FD8B5940C7561CD404DCF95
PackageDescriptionESO data reduction pipeline for the HAWK-I instrument 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
PackageVersion2.4.3+dfsg-1
SHA-1FBE7872286CE89B53E0544E3D1E8C86BB09581AB
SHA-256A6ECB0026D06870834397818D25A9044D0089E2CC575310F24458F40D0F1B52E
Key Value
FileSize548756
MD57B774D5D5C690C1AD50BAFC43FDDB0C4
PackageDescriptionESO data reduction pipeline for the HAWK-I instrument 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
PackageVersion2.4.3+dfsg-1
SHA-1B6C87AC7CEF51846AD1962434E51181D948F75F9
SHA-2564BB11E9B6BA556172558877F98E9B23702C96254E0C6CD3DF42D3C2B65C795F7
Key Value
FileSize76400
MD5F5D8459ED455DBB253ACDC570E9DD1C9
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
PackageVersion2.4.3+dfsg-1
SHA-1542F387722688F7F2843AA373EFD0D1FEDC30FEC
SHA-256FE73C6B44EA51D10AC846009BFDE5EBDE563721A6C4A4B534892F41882B49B1E
Key Value
FileSize468408
MD5AFB8672F4237B6E084ADD1D7965FEC77
PackageDescriptionESO data reduction pipeline for the HAWK-I instrument 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
PackageVersion2.4.3+dfsg-1
SHA-15F5A26B6ED1A94FCCDB5418A6EA9D38509C7832D
SHA-256A8BF33C01629FEB6CE296AB321AF3C889D6452D6BE48DD6507E7D949D35B2061
Key Value
FileSize477952
MD53CAA106DD6246DCF218DE138AE022F77
PackageDescriptionESO data reduction pipeline for the HAWK-I instrument 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
PackageVersion2.4.3+dfsg-1
SHA-107D5C627FC555F637353012D04FEE7C6F1E6113C
SHA-2564B04179EDF606ECC3AE590EC5EB34589B088566F820C6F00530B40016D5D6193
Key Value
FileSize471088
MD5B8FD83D2BD28D19D4560F9F25976C8F4
PackageDescriptionESO data reduction pipeline for the HAWK-I instrument 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
PackageVersion2.4.3+dfsg-1
SHA-11C8FE32120734D45F159CF07A89DF8F4AE4700E1
SHA-25633B192C73AF4F5B97638210C15508D770F5731F4969E5D34D0864DB81751A269
Key Value
FileSize547580
MD5B18CA767A1199AA5AF489CE17CD7BB65
PackageDescriptionESO data reduction pipeline for the HAWK-I instrument 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
PackageVersion2.4.3+dfsg-1
SHA-1F236FEA9C8FD567B3682BBF6658FCD7300D6B0E0
SHA-256F686E8D97B34E3D32A5A43F84F58708D1760617E24A4B37F15023F1F5FB5E51F
Key Value
FileSize515728
MD5178BC39B67CCFAC7374837B6783DEFDE
PackageDescriptionESO data reduction pipeline for the HAWK-I instrument 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
PackageVersion2.4.3+dfsg-1
SHA-11B3779DC0D999F9AA02A89F5F799490440FB4A47
SHA-25688F0D4E52748D0A396F071C0EAF70FDD8F9BB0D1A987F7729A2B4E284A95C891
Key Value
FileSize471024
MD5948CB92838A4404E1AA12023641CDAB5
PackageDescriptionESO data reduction pipeline for the HAWK-I instrument 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
PackageVersion2.4.3+dfsg-1
SHA-12E3B1A4071995F103CF47F407CA4EF4591C36C9F
SHA-256382F8A1605747E26EE33758BD402E6C71DCB38950105E0EEF9E246951EF5205A
Key Value
FileSize470896
MD504E6CDD5BC92409B9B8ACCDBDA45598D
PackageDescriptionESO data reduction pipeline for the HAWK-I instrument 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
PackageVersion2.4.3+dfsg-1
SHA-11AB820B4CF5A53A38486A13C3E51A928A2FE694D
SHA-256F4E93FD2283238717114016AB9CA5CDBD1B98D37FDA6784152CB5222AD3B3867
Key Value
FileSize167796
MD540574540DEC596DCC1B170F3330307A4
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
PackageVersion2.4.3+dfsg-1
SHA-1BEDDE3D6B0FF5F753CE66BDE6F4EF46E69436760
SHA-2562148D1A28D132F54A965FF405938AF1E317E2C0F940E037724E6472A73966E99