Result for 2E5C65D77258B9C6A2215D1F5D3A013CA939E32D

Query result

Key	Value
FileName	./usr/lib/x86_64-linux-gnu/cpl/plugins/hawki-1.8.21/hawki_util_stdstars.la
FileSize	1023
MD5	6873AF68022B624AB88E9370734C7687
SHA-1	2E5C65D77258B9C6A2215D1F5D3A013CA939E32D
SHA-256	EF4B75881B2B6921BEE6EA814391BDAA0F9625A312DB40992A2BA74A8BE4AE0E
SSDEEP	24:AeSGWWJiizxIY+Ahmfvi4MvD2NGDe5/bxn:sGWWJnzxIY1hmfKNLcbx
TLSH	T15111EF3B838F5129AFE40E454F9E323F42CA9038072A0F1C52EB95CB614B42A2166F36
hashlookup:parent-total	2
hashlookup:trust	60

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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
FileSize	200196
MD5	55DAFFDB7A8ADAEB25B360D7AD3A2159
PackageDescription	ESO 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).
PackageMaintainer	Ubuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageName	cpl-plugin-hawki
PackageSection	science
PackageVersion	1.8.21+dfsg-1build1
SHA-1	5604971B6C39DB285290AA6F1E48D23EE6AEBB28
SHA-256	104611200EAA2B4F7482B543F9B2A05BC611FD705EDF92FD5DD80228BAA3DB55

Key	Value
FileSize	238384
MD5	BD0858144B9991FC7E5BAE6A82F03021
PackageDescription	ESO 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).
PackageMaintainer	Debian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
PackageName	cpl-plugin-hawki
PackageSection	science
PackageVersion	1.8.21+dfsg-1
SHA-1	8DF945A85ED8F9B9ED454AE4BF385B1504291ADF
SHA-256	A63DB43EAB793C6B3E0BF690F6285C633FB2628F6470D923308272C4B5966746