Result for 0A7C083EC2EB0C353EEF1C9EC2049EC5EC9D1F4F

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/cpl/plugins/hawki-2.4.11/hawki_cal_distortion.la
FileSize1025
MD5B9D5E5976E20AAC26463FABA098A910D
SHA-10A7C083EC2EB0C353EEF1C9EC2049EC5EC9D1F4F
SHA-25622BED1FF5188F5925703496CE64DB68284E47D1A6E653731D37119A31306D2F9
SSDEEP24:BeSHOWJ2mioRxIY+Ahmfvi4J1vD2NGDe5/o1:7uWJowxIY1hmfKIpLco1
TLSHT1E811E23F938A9536BFD10A86468E352F425940B847522F5093C6DEDF124F839B257F26
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
FileSize527876
MD51EDF8496263A6ADC7FA6A5315429C69F
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
PackageVersion2.4.11+dfsg-1
SHA-1B819EEA56280AD4ABCC44E5D419874F364EF861F
SHA-256591F4DC68AFEC363D198CBB54130A8FFCC76FF7F0F3FEE4034C8C6347C8CD4E0