Result for 05D003B1BD4B95C2721D9297090367A6A0F2909F

Query result

Key	Value
FileName	./usr/lib/i386-linux-gnu/cpl/plugins/hawki-1.8.18/hawki_tec_filtchk.la
FileSize	1011
MD5	AA8BC9AB821B9ED2D458E63F8745C109
SHA-1	05D003B1BD4B95C2721D9297090367A6A0F2909F
SHA-256	A5291B7EAA9C7E39F2BCFD536875AE37437ECCA1A22D79A595F259E2B873CA39
SSDEEP	24:NeShxWJpiOxIK+Ahmfvi4rvD2NGDe5/oV:fHWJQOxIK1hmfKoLcoV
TLSH	T1ED111F3AC3CA752577D00F558A8F302F46C9803D17250E1863D7A5CB1247C1A21E7EA2
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	223496
MD5	DB080E4DE28E88717687F0A21F4C4B5F
PackageDescription	ESO data reduction pipeline for HAWK-I 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	1.8.18+dfsg-5
SHA-1	21DE5B54C486BE6FA5076FF26E74B0AE7FE2F64A
SHA-256	DB2B4ECBF4578BF3B0FE5F5B39E654E3643602A7E36D0E2E22F391D4FA417198

Key	Value
FileSize	221550
MD5	7CA8C8F751AC49CD58D14D76DA00B8B5
PackageDescription	ESO data reduction pipeline for HAWK-I 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	1.8.18+dfsg-4
SHA-1	BA8CEACF21DD0E05B10A5C496CD082AD9365547E
SHA-256	949029E1EA39C0BBA2A85405157D2B6E9179DF9FAFA1E585C720E7DE40B0B7D9