Result for 1EF162A61311447A89F1C97511BCA3CDA26562CD

Query result

Key Value
FileName./usr/lib/s390x-linux-gnu/cpl/plugins/hawki-2.4.3/hawki_step_stats.la
FileSize1003
MD5C28794B7C57D19992CB54EFDE95191A5
SHA-11EF162A61311447A89F1C97511BCA3CDA26562CD
SHA-256278F00955D7651D0243ADD6CF919D5B83922235410921FB044EDFBC53247B2A1
SSDEEP24:PpeSGsWJ5bi3UUoxIY+Ahmfvi4deEvD2NGDe5/j0:bGsWJksxIY1hmfKrOLcj0
TLSHT17B11023FE38E5129AFD00E45468F303E46C9883C07231F5052CBD5DB614B419216AF37
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