Query result

Key	Value
FileName	./usr/lib/powerpc64le-linux-gnu/cpl/plugins/hawki-2.4.3/hawki_detector_noise.la
FileSize	1033
MD5	3808A5E220DD11AB322C031EFAF800E4
SHA-1	0AE38D6B636106EB5D0E24CA6B3A56A5D6B86FCA
SHA-256	FA38D333AFBB925D3C53CF6EA659CDE708A79D428AC7CAB5B8FEFC712BB11619
SSDEEP	24:nWeSGsWJjZmiVhhZRxIY+Ahmfvi4ivD2NGDe5/B90:neGsWJljXRxIY1hmfKxLcP0
TLSH	T1B51112BFC39A613A67D90B45568E306F428E40BA07551E5452C6DECF254BC1922B6E33
hashlookup:parent-total	1
hashlookup:trust	55

Network graph view

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	547580
MD5	B18CA767A1199AA5AF489CE17CD7BB65
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	F236FEA9C8FD567B3682BBF6658FCD7300D6B0E0
SHA-256	F686E8D97B34E3D32A5A43F84F58708D1760617E24A4B37F15023F1F5FB5E51F