Result for 0DBB293CFC916B39C81F3051372A9B6753C80846

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabihf/cpl/plugins/hawki-2.4.11/hawki_cal_distortion.la
FileSize1030
MD58997D44FB22F8AA9DC252D1CDE6B5E03
SHA-10DBB293CFC916B39C81F3051372A9B6753C80846
SHA-25653D4CA2CB9EC9D88138F2356086B5C6E2049CDA458DF2166517555A995AC53AD
SSDEEP24:BeSHOWJ2mioRxIY+Ahmfvi4J1vD2NGDe5/Ajy:7uWJowxIY1hmfKIpLcAW
TLSHT17A11FC3F938A8536BBD00986468E392E425A40B807522F5093CACADF124F839A257F22
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
FileSize451432
MD5806CB6A07D053F721A8E675196114EB6
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-1D4EE6BE1F295CE3F05E675E4F234B3A20BF3B199
SHA-256E2F48D24F4D2E931655F871957B4718228B438460887A47BEAC55B6C6D323744