Result for 2AE04650681F1C81A2C166B62293D00D1A72C143

Query result

Key Value
FileName./usr/lib/x86_64-linux-gnu/cpl/plugins/hawki-1.8.14/hawki_cal_distortion.la
FileSize1037
MD5160C516B729DC1CBE0A5A513CA208BCF
SHA-12AE04650681F1C81A2C166B62293D00D1A72C143
SHA-2566BFE0A41201A66D9A66515D559B270E08E9ECAFE93DB8D782424B9DE46520158
SSDEEP24:BeSh+WJ2mioRxIK+Ahmfvi4J1vD2NGDe5/bh:7AWJowxIK1hmfKIpLcbh
TLSHT18611E23F838A9136BBD006964B8E352F42A9407846552F1093C6CADF124F83AE257E72
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
FileSize195760
MD5AD2C0CE7BFA6DD0C55A03053260B56BB
PackageDescriptionESO 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).
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion1.8.14+dfsg-2
SHA-1086A952CA52A913571A4B157A2FACE4144827EDA
SHA-2562D7C4EE843C799609FC589F29F835C883F9AA2BE52375FA434E627D2452C14C0