Result for 0C1EA7F8F0FC7BE11D36CC7174B05310CE53C648

Query result

Key Value
FileName./usr/lib/s390x-linux-gnu/cpl/plugins/hawki-2.4.3/hawki_detector_noise.la
FileSize1027
MD5AE57065C3A202D2CBEAAC90F898A30E8
SHA-10C1EA7F8F0FC7BE11D36CC7174B05310CE53C648
SHA-256397160CA5A655D52ECD1BA7C94181ED07761DB5155380056430DA0952CFC9023
SSDEEP24:nWeSGsWJjZmiVhhZRxIY+Ahmfvi4ivD2NGDe5/j0:neGsWJljXRxIY1hmfKxLcj0
TLSHT10E111FBFC39A613E6BD84B45568E306F428E40BA07991E5452D6CACF254BC1922B6E33
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
FileSize468408
MD5AFB8672F4237B6E084ADD1D7965FEC77
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-15F5A26B6ED1A94FCCDB5418A6EA9D38509C7832D
SHA-256A8BF33C01629FEB6CE296AB321AF3C889D6452D6BE48DD6507E7D949D35B2061