Result for 1B0B5513F39DC51EEB65425DAA361B44D686B9E9

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/cpl/plugins/hawki-1.8.21/hawki_step_apply_dist.so
FileSize14384
MD5FD4CA45C756382521FE17F87A3BE73EF
SHA-11B0B5513F39DC51EEB65425DAA361B44D686B9E9
SHA-256F17A43E7F47B16566D798BA94B9AC735AD91AEA6E71427FE150E553E2BF5697D
SSDEEP192:vF8p9ooPwDmvun5X3Qgc2EwjHtltlyzzYLRI1Ci3bjuccs5/cTan0bXJYqoz:QooPwK2BggTjNltlfYCi3rkTan0bXHo
TLSHT18E528517F7A2C9F1DAC212B0540B062DD5744821E62FEF837D8DB2889615AACD93277E
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
FileSize260978
MD55F77ED0FB77CB9283D78B6CC956FBAC7
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
PackageVersion1.8.21+dfsg-1
SHA-13D00E429E99C1B8D428D87C587056182BBA9003D
SHA-256C39FAE0786F62BF2CDED8B18E826ADF7C549FC82B84F7602C5DC53034AF832DA