Result for 274994D77550DE6F4A579CC063D35ECEFC0EE26E

Query result

Key	Value
FileName	./usr/lib/x86_64-linux-gnu/cpl/plugins/hawki-1.8.18/hawki_cal_zpoint.la
FileSize	1007
MD5	504B242A17467415D648CC50AEDCF1C5
SHA-1	274994D77550DE6F4A579CC063D35ECEFC0EE26E
SHA-256	09D52F2AC954FA9C9EA5ECDD5F4EE68760D073CE1536F45B04F7489F01ADA479
SSDEEP	24:4eShxWJ+izxIK+Ahmfvi4IvD2NGDe5/bV:UHWJ7zxIK1hmfK3LcbV
TLSH	T18F11023F93DF9127A7D00AA65B8F317E428A443847550E5092CAD5EB114743A25F7E72
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	199012
MD5	B01C49B7C03387D9F4FEB6040374C806
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	3471E1B68664943242AD6077ADE94A6DCD742EE6
SHA-256	318E3CDF027B1088E2BD10A59D696200CE37664D96E4CE2F5D0C6A0BDC7F1631

Key	Value
FileSize	198336
MD5	CA15E5417041E43053C886E1BDA5CD44
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	2F6AB05B3293B6E6D92D58EFCE8AE0437643F5A5
SHA-256	66C3B6431465CBAE37C289F7ECC5E28BFC824B5D82988FFBBC7C6CF67E5E805F