Result for 0988F960FBD2B436526EBE3FD664C0A523BC16AF

Query result

Key Value
FileName./usr/lib/mips64el-linux-gnuabi64/cpl/plugins/hawki-2.4.9/hawki_linearity_analyse.la
FileSize1052
MD593ED17C0E0C568B0762EBFF6B5409A22
SHA-10988F960FBD2B436526EBE3FD664C0A523BC16AF
SHA-2567EE67D5373EFC846EE09760DC15CFC286113364A8B51572B0BC92EFEFDB33E20
SSDEEP24:cDeSG5WJe9iUXXKxIY+Ahmfvi4ybvD2NGDe5/5:cRG5WJesUXXKxIY1hmfK/vLc5
TLSHT1A0114237A399193D77E40B4616CE346F47D94079C3520E9C82CAA6DF31838293367E22
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
FileSize432820
MD5C12CBBEF48D8105D146F3F56E4FC6A80
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
PackageVersion2.4.9+dfsg-1
SHA-1E41BD0569D8F9C390A871D226FEBCF087EAA5725
SHA-2561645C1BA99874DEA41DB29C0692F68499585F6E8E7C1FA36686DA058B91EFAFC