Query result

Key	Value
FileName	./usr/lib/mips64el-linux-gnuabi64/cpl/plugins/hawki-2.4.3/hawki_science_postprocess.la
FileSize	1065
MD5	AD3214B5A376D0DF20645170D2DE8AE2
SHA-1	01120EF9709CE0681D4069314BFA94FA805E6A42
SHA-256	A1A6B648D395808E05024F5E18DA0705BBF2337B4BF74FB8C7F414C7F88B5975
SSDEEP	12:JHK4fWgxG+/r5WFKmH3LiBH1W1WoxIha+AAmBB7Szf77ixCF7tvT3RTZ/9IMCKbQ:TeSGsWJ7icxIY+Ahmfvi45vD2NGDe5/H
TLSH	T1E711D0B6C3CD5D766BD01545A6CE302F4A8A843C0B19097493C6D5DB278742A1157E3B
hashlookup:parent-total	1
hashlookup:trust	55

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The searched file hash is included in 1 parent files which include package known and seen by metalookup. A sample is included below:

Key	Value
FileSize	459464
MD5	BF5AA2AF1FD8B5940C7561CD404DCF95
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	2.4.3+dfsg-1
SHA-1	FBE7872286CE89B53E0544E3D1E8C86BB09581AB
SHA-256	A6ECB0026D06870834397818D25A9044D0089E2CC575310F24458F40D0F1B52E