Result for 0434D5392C34B8F0035D28188A769E4BD4861D44

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabihf/cpl/plugins/hawki-2.4.3/hawki_tec_filtchk.la
FileSize1013
MD55F6D99B88AB9101EEAC31B3512DE3720
SHA-10434D5392C34B8F0035D28188A769E4BD4861D44
SHA-25681A93924A96C03428063183F5C18E13959B4746F0A8DA736682023CDF74D15E7
SSDEEP24:NeSGsWJpiOxIY+Ahmfvi4rvD2NGDe5/Ajd:fGsWJQOxIY1hmfKoLcAp
TLSHT12611EF3AC3CA792A7BD00E45868F302F46C9443C17260E5963CBA5CB5247C1921A7EA2
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
FileSize471024
MD5948CB92838A4404E1AA12023641CDAB5
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
PackageVersion2.4.3+dfsg-1
SHA-12E3B1A4071995F103CF47F407CA4EF4591C36C9F
SHA-256382F8A1605747E26EE33758BD402E6C71DCB38950105E0EEF9E246951EF5205A