Result for 1D25C9E3119F55C699E1F51AE89F9314F5995611

Query result

Key Value
FileName./usr/lib/mips64el-linux-gnuabi64/cpl/plugins/hawki-2.4.9/hawki_dark_combine.la
FileSize1022
MD5E231593F7BB90906F0D288BDE9C7EE26
SHA-11D25C9E3119F55C699E1F51AE89F9314F5995611
SHA-256B875046EBD3E2079966CC5181F6947D515EE30A092050174BBF8CCDBCC0F3BA6
SSDEEP24:sKeSG5WJ+DOiESSD5xIY+Ahmfvi4igvD2NGDe5/5:s6G5WJ+fESSlxIY1hmfKPqLc5
TLSHT18C11FC7BC39E2969E6E00A469BAE3A2F438E80BD07120A1093C6C5DF12478192166E37
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