Result for 0FAD42A6EBB30836EBC77D1BBD0743EC2281FCA8

Query result

Key Value
FileName./usr/lib/powerpc64le-linux-gnu/cpl/plugins/hawki-2.4.3/hawki_tec_filtchk.la
FileSize1015
MD5D0B7A4D0E3C49649675B90DA9961D575
SHA-10FAD42A6EBB30836EBC77D1BBD0743EC2281FCA8
SHA-2566CC462089D985FFB74E23F9D33F2EB838736AA93C3369F25EF4B41017DD4C6F2
SSDEEP24:NeSGsWJpiOxIY+Ahmfvi4rvD2NGDe5/B90:fGsWJQOxIY1hmfKoLcP0
TLSHT1EF11EF3AC3CA79297BD00F45868F312F46C9403C17250E5963CBB9CB5247C1921A7E62
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
FileSize547580
MD5B18CA767A1199AA5AF489CE17CD7BB65
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-1F236FEA9C8FD567B3682BBF6658FCD7300D6B0E0
SHA-256F686E8D97B34E3D32A5A43F84F58708D1760617E24A4B37F15023F1F5FB5E51F