Query result

Key	Value
FileName	./usr/lib/arm-linux-gnueabihf/cpl/plugins/hawki-2.4.9/hawki_detector_noise.la
FileSize	1030
MD5	24841EB8DC739785799B04E1CA513CCB
SHA-1	0A5E791D8E6DD6C94DB8C2864CF75C2C0FE6A74C
SHA-256	64B0861D85A74EBA79D8024C488FDFC09BAFC7A5E6AFC78D2B5418EFAA9B84EE
SSDEEP	24:nWeSG5WJjZmiVhhZRxIY+Ahmfvi4ivD2NGDe5/Aj7:neG5WJljXRxIY1hmfKxLcA3
TLSH	T1F71112BFC359613B67D80745568E306F424F40BA07590E5452C6CACF254BC1922A6E23
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	448916
MD5	15510D708B30FD3447AB413D215ADBF9
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	2.4.9+dfsg-1
SHA-1	617C0F0EC2D7EA25558AFB56BCCB07552925D079
SHA-256	9202A8FDCCDB13C2F3ACC2DC6A1BDFA123AD464F752FF6FE14DB8FC365CA9AE6