Result for 1A75DA48A8EA9F1153D2AB593EC9A67E72B277F9

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/cpl/plugins/hawki-2.4.9/hawki_step_stitch.la
FileSize1007
MD5B44DE36E5159B26D09C072D23A53698A
SHA-11A75DA48A8EA9F1153D2AB593EC9A67E72B277F9
SHA-25670CA7B74918B1E9ADF5A3F6AA035527F15D9FF35C3B73DDA3A44DADF9D92DC7B
SSDEEP24:HeSG5WJvikxIY+Ahmfvi4tvD2NGDe5/oS:tG5WJKkxIY1hmfKaLcoS
TLSHT1D511323AA39A1135BFD00A89478F723E478A487C07710F5062F784DB118B41925A6F33
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
FileSize524536
MD53FC8B3C34A65DF11F4044DD0DED779E6
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
PackageVersion2.4.9+dfsg-1
SHA-170C4037CF07C67D800F6A6916A4412B35AFD6356
SHA-256A4615C80DE8B1365075BBBC5B4DEDF45435016BCDC59F1DE203D83F86568C5FA