Result for 1279C93662C04380C4E96AFBFA5E78F18F61AC66

Query result

Key Value
FileName./usr/lib/aarch64-linux-gnu/cpl/plugins/hawki-2.2.0/hawki_dark_combine.la
FileSize1015
MD585D6B419EF141DA9F41DC76739F371AA
SHA-11279C93662C04380C4E96AFBFA5E78F18F61AC66
SHA-256172341FEB3013F8240DE1D2919DC0F76932D5422A8CC8EA32C920C6CB1FD4EF0
SSDEEP24:sKeSG1bWJ+DOiESSD5xIY+Ahmfvi4igvD2NGDe5/vp:s6GVWJ+fESSlxIY1hmfKPqLcvp
TLSHT18411EF7BC39E6965EBE04A46979E3A2F438E807D07130E5093CAD5DF1347C1A2156E3B
hashlookup:parent-total2
hashlookup:trust60

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Parents (Total: 2)

The searched file hash is included in 2 parent files which include package known and seen by metalookup. A sample is included below:

Key Value
FileSize339148
MD5C58D5E032A626182ED9262A1DA69BDEA
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).
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion2.2.0+dfsg-1build1
SHA-1A3CF036AA00324958F4AD1F5F560ACB7C87F5FAE
SHA-25606CC17F274E65C368C62414C15C314154E9EE262D76EEC3AA890F81158595536
Key Value
FileSize412076
MD508B3CE36677FB07D89A49E60A807357C
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
PackageVersion2.2.0+dfsg-1+b1
SHA-1EDDFA8E4D2940474F63B25AC9BDAB2C9340BD1C7
SHA-256F5CDE157AB1385847031F916C70B8A0015D5F3794F32164E289FACCEFEA462DA