Result for 1CBC12B56B6A9A9366F1EF8D5222B0409EF07B7F

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabi/cpl/plugins/hawki-2.4.3/hawki_step_stats.la
FileSize1005
MD509806A3C0EFBAABDE7C985F9EF06D926
SHA-11CBC12B56B6A9A9366F1EF8D5222B0409EF07B7F
SHA-25601CEB22AED24223E5A0749601B831864061E2CE12DCA70494F40D7A77175E00E
SSDEEP24:PpeSGsWJ5bi3UUoxIY+Ahmfvi4deEvD2NGDe5/AjD:bGsWJksxIY1hmfKrOLcAH
TLSHT17911023FE38E5526AFD00D45468F303E46C9883C07231F5052CBD5DB614B519216AF27
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