Result for 1E7F867DEE848C63248453593BCC1BCF4824EE70

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/cpl/plugins/hawki-2.4.11/hawki_step_compute_bkg.la
FileSize1037
MD53DA7A6828DDB064CB0B71EDF08C187E2
SHA-11E7F867DEE848C63248453593BCC1BCF4824EE70
SHA-25629B4F846C22C31E4DD62A6A6A70A981D602D65C08252D5708AAAC3365B729ADF
SSDEEP24:0ReSHOWJmyOicJJy5xIY+Ahmfvi4C1vD2NGDe5/o1:0LuWJmmcJJwxIY1hmfK7pLco1
TLSHT11E11E23A93CA5525AEE04A86579F303F428A487C47236E6052C7D9FB114B82B3156F26
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
FileSize527876
MD51EDF8496263A6ADC7FA6A5315429C69F
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
PackageVersion2.4.11+dfsg-1
SHA-1B819EEA56280AD4ABCC44E5D419874F364EF861F
SHA-256591F4DC68AFEC363D198CBB54130A8FFCC76FF7F0F3FEE4034C8C6347C8CD4E0