Result for 105C04B5129FACA1D8F5114702C3BD669CC9CD9F

Query result

Key	Value
FileName	./usr/lib/x86_64-linux-gnu/cpl/plugins/hawki-2.2.0/hawki_step_detect_obj.la
FileSize	1032
MD5	895AD2CB4262700EB5497DFEBFAC071B
SHA-1	105C04B5129FACA1D8F5114702C3BD669CC9CD9F
SHA-256	05B44891995D965E5958E28E8585B8C4CD13B9B011CCAC94CBA1A03499D2E290
SSDEEP	24:PeSG1bWJU2icBxIY+Ahmfvi45vD2NGDe5/bp:lGVWJUzcBxIY1hmfKqLcbp
TLSH	T13511AD3BD3D9713AAFD4294596CF303E4299847907312E5063C795DB224B81911A7E27
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	479446
MD5	05163626569370830CB4BA3492E0B092
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	2.2.0+dfsg-1+b1
SHA-1	CEDE6337214FC45AF5F212D7F8B8F84CD8EDCD55
SHA-256	89D9D055F1AB77CD76E039FA4BC12C013BD5702025C1FA292279C2316B1D1BB8

Key	Value
FileSize	407134
MD5	8BB75CFCA14D06B369847DA5AD3C0659
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	2.2.0+dfsg-1build1
SHA-1	57E12B5F92879BB2A2B01FC61AE6BF5307FC2945
SHA-256	0A0320B5C8F5B44A2C6CBD2E98BE1B3BEC71DBF24EF43CE8BC2912388B5663DD