Result for 186794080E5302C66BBA59B912D1DD77D8CC966D

Query result

Key	Value
FileName	./usr/lib/arm-linux-gnueabihf/cpl/plugins/hawki-1.8.21/hawki_step_compute_bkg.la
FileSize	1044
MD5	A3AA5AC8A3A86AD30ABBC9BF46EEA2B4
SHA-1	186794080E5302C66BBA59B912D1DD77D8CC966D
SHA-256	73B5DD6CF1F3CB2F3EFC14AD75EEAB259D03C2AF0C3596B98350547BAA9D3872
SSDEEP	24:0ReSGWWJmyOicJJy5xIY+Ahmfvi4C1vD2NGDe5/AjGn:0LGWWJmmcJJwxIY1hmfK7pLcAy
TLSH	T1DA11E23A83CA5125AFE04586579F303F528A4C7C07276E6452C7D9FB114B81B315AE62
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	184482
MD5	2A9ACD5A8E062002F64B214A3B6B00FF
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	0600C46860A116FB748364715FA18ECAE1EBA0AC
SHA-256	2F942E0CDB1F7E91576879FA81FC9A13FD3C56B3C0AFD51DFBAD967AC412F017

Key	Value
FileSize	223236
MD5	250B250B503BC1BE132F283F2DE01047
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	745F2CE42DE269179A9D006DAA409DDB5E4373D2
SHA-256	97E966AABBC439DB1190D4805629759BA2314151762DE45E9E685D8179ACF04A