Result for 114AF54CABB6F6A1AA7026EF3BB8163AA375E0D5

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabi/cpl/plugins/hawki-1.8.21/hawki_cal_flat.so
FileSize35828
MD5BC9E87F73710125847D77469579D8F0F
SHA-1114AF54CABB6F6A1AA7026EF3BB8163AA375E0D5
SHA-256441142BF8DBE45122AA83518BEF9D75070F98F730717AA163FDDE8ED71151588
SSDEEP768:Ub6bGmMw1RG6EdwMcd+bxW9ErI7YW57hsGGX6f6ZfEYJ/Yao:U+bQw16uTnlqcWEYJ/lo
TLSHT120F20AC76C61AB3BC1D0233926EE0794311117F093CAAB465E088755AD47A7DC6B7F8E
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
FileSize228074
MD5CE29F2691A6DA88FF83D73C679596827
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-1FFAB13A4EB060F369871AD9885635F1D6BDEAB73
SHA-2568D0D52E213F4C1B1787D5035FF57338A5A51EE8C5F408362A01B3492A2590DA5