Result for 17D48C0FEE2B17016922E30797E4CE95DF7368BA

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/cpl/plugins/hawki-1.8.18/hawki_cal_distortion.so
FileSize31172
MD58F07E4A219D19CE62A98F864B878DA38
SHA-117D48C0FEE2B17016922E30797E4CE95DF7368BA
SHA-2565C8B7C9B8F01CD9B037E3BDFD9F3B1A7B16915CEE4C6A4E1F45B764203185B44
SSDEEP768:/RAlLBfTRlHCcQMYJ1PM48DC3Tr1617A0Gy7:potXQ9PM48+Tr0p
TLSHT138E2C5DFE5E2C8B2FAD221F44C57456584309540E72BC3D2AB083A85562369DFAF273B
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
FileSize223496
MD5DB080E4DE28E88717687F0A21F4C4B5F
PackageDescriptionESO data reduction pipeline for HAWK-I 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).
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion1.8.18+dfsg-5
SHA-121DE5B54C486BE6FA5076FF26E74B0AE7FE2F64A
SHA-256DB2B4ECBF4578BF3B0FE5F5B39E654E3643602A7E36D0E2E22F391D4FA417198