Result for 04B00AFE7526DC8CF1D352D432AE9EFA19D5795E

Query result

Key Value
FileName./usr/lib/s390x-linux-gnu/cpl/plugins/hawki-2.4.3/hawki_cal_dark.la
FileSize991
MD596367CF25BD21A17852E135C2B0D5D99
SHA-104B00AFE7526DC8CF1D352D432AE9EFA19D5795E
SHA-2564F92BD081FB928F674BFD693709EB324D89E9DAD0B5E5A04EB670ABE1B567120
SSDEEP24:4eSGsWJJ4ifTTLxIY+Ahmfvi4nEvD2NGDe5/j0:UGsWJHDxIY1hmfKwOLcj0
TLSHT10B11027FD38A9129AFD01A46578E392EC2CD403C07160E5453C6D6EB114B5392366F32
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