Result for 205147BEA0E258513D73DDAED2A8C7785E5A3855

Query result

Key Value
FileName./usr/lib/powerpc64le-linux-gnu/cpl/plugins/hawki-1.8.21/hawki_cal_dark.la
FileSize998
MD5E390420B0F59EA0FC64AD17386CF6DEC
SHA-1205147BEA0E258513D73DDAED2A8C7785E5A3855
SHA-25654261CCB0A98A2504DF822083826E39BD5E54FB4531A68529EFB0CC306F22CDD
SSDEEP24:4eSGWWJJ4ifTTLxIY+Ahmfvi4nEvD2NGDe5/B9xn:UGWWJHDxIY1hmfKwOLcPx
TLSHT1ED11C57F838A9125AFD01A4667CE362EC2CD403C47150E5853C6D6EB114B5392266E76
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
FileSize224692
MD5D1343C262A1A7E0BD8BD4569E23F068D
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
PackageVersion1.8.21+dfsg-1
SHA-15671A6932A008A7BDE978A313EC947BFE2999B20
SHA-256136A0A4E926B114E41A51F5D4B1915255A9E2B8943770353493F216FBD564D4E
Key Value
FileSize190308
MD54A9C354B9047366270BE90C85A9082F1
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
PackageVersion1.8.21+dfsg-1build1
SHA-1255B34E4F87A4AB7107B747E7A67F6995239722E
SHA-256BB9CA8E6CCCE01596EB08FC791C6ECDF3554D3E2D18DC55330F7EDA7CAC17BBF