Result for 1E0F1CBED3F663C11A1475E76FD7C7E3597B7738

Query result

Key Value
FileName./usr/lib/s390x-linux-gnu/hawki-2.4.3/libcasu_catalogue.la
FileSize1006
MD5A6F8C89E2355F588968F406DD2B025C6
SHA-11E0F1CBED3F663C11A1475E76FD7C7E3597B7738
SHA-25679FF84B5FB69BEC0FC26475EFEB6E5A97A43AC78AE6DF8F129A0701F9B68AF9A
SSDEEP12:PE4fWgxG+/r5WFKkNJLi3+HO+xIha+AAmBB7Szf77ixCF93vT3RTZ/9IMCDwDqai:neSGsWDi8fxIY+Ahmfvi4tvD2N0De5/3
TLSHT12411CC7AC3AD46BA3BE01A55458F342F835A407CA71F092041CA8DDF314F8663285EF2
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