Result for 24B0D0310DAE6BFE36042C1B546A5001BC34CC93

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabi/cpl/plugins/hawki-2.4.3/hawki_step_compute_bkg.la
FileSize1041
MD5461DCA79DDF83FC187DDE818EBD74BEF
SHA-124B0D0310DAE6BFE36042C1B546A5001BC34CC93
SHA-2566DC3CD0CEBCEA0ECD9AF381DF3622C2CF115E938463A775BDAE415D01F8A257A
SSDEEP24:0ReSGsWJmyOicJJy5xIY+Ahmfvi4C1vD2NGDe5/AjD:0LGsWJmmcJJwxIY1hmfK7pLcAH
TLSHT1BC11E23AC3CA5525AFE04586579F303F428A4C7C07236E6152C7D9FB114B81B3156E22
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
FileSize477396
MD536D3852665BA37B7D3A54BDF92495CD3
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-1FB4CFFDCD3D3AC67745E1A84542709CE1909378B
SHA-256BD03FA5F24D6267A89ED763C03A764AAAFADAFC91D2D1AE4BA51802A7659DA82