Result for 232516070E7B7CCBA03B13A90C907A035EF3A5F6

Query result

Key Value
FileName./usr/lib/x86_64-linux-gnu/cpl/plugins/hawki-2.4.3/hawki_step_detect_obj.la
FileSize1034
MD5C1F5A26049AF79BD13515E16AB7B0093
SHA-1232516070E7B7CCBA03B13A90C907A035EF3A5F6
SHA-2560BF31D95809EED04370090ADC7887B2F71116F0B81573414704D717761784C89
SSDEEP24:PeSGsWJU2icBxIY+Ahmfvi45vD2NGDe5/b0:lGsWJUzcBxIY1hmfKqLcb0
TLSHT1CC11AD3FD3DE713AAFD4194596CF303E42C9887907312E5063C795DB224B81911A7E27
hashlookup:parent-total1
hashlookup:trust55

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Parents (Total: 1)

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
FileSize515728
MD5178BC39B67CCFAC7374837B6783DEFDE
PackageDescriptionESO 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).
PackageMaintainerDebian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion2.4.3+dfsg-1
SHA-11B3779DC0D999F9AA02A89F5F799490440FB4A47
SHA-25688F0D4E52748D0A396F071C0EAF70FDD8F9BB0D1A987F7729A2B4E284A95C891