Result for 00BEBBF86BEC3829C95C01167F882EBD47DF406F

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/cpl/plugins/hawki-1.8.14/hawki_step_detect_obj.la
FileSize1041
MD537749916756DA60D6561D2C604368BB3
SHA-100BEBBF86BEC3829C95C01167F882EBD47DF406F
SHA-2564651436FF924CACE84EA4D5B161376172D7DCAEBDA8D0DAB4F7645917DE53FC3
SSDEEP24:PeSh+WJU2icBxIK+Ahmfvi45vD2NGDe5/oh:lAWJUzcBxIK1hmfKqLcoh
TLSHT1DF11DD3FD39E713AAFD416458ACF303E42D9887A47352E5063C785DB224B81911A7E6B
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
FileSize196654
MD50A2841A209224E251882DC665A2EB149
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
PackageVersion1.8.14+dfsg-2
SHA-1B2471E6CD8501B5A1B43B2EC659031EB8B478ED9
SHA-256332FEEC118B1D561CAAF58D189027595FB6AF81FF18CF0C8BEF702BFC56BB89A