Result for 10DAC3886B835D03AA0D75618D672E4F4AF28888

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/cpl/plugins/hawki-1.8.14/hawki_util_gendist.la
FileSize1023
MD56F808C1663703050ABB22950FBB50C4A
SHA-110DAC3886B835D03AA0D75618D672E4F4AF28888
SHA-2565FC916B3B5A0B4BDA94D808572FF5B0583A3FEC9CBCCBD695A45930E9CD8FBA4
SSDEEP24:KXeSh+WJYZiirr2xIK+Ahmfvi48d1vD2NGDe5/oh:K9AWJYAirr2xIK1hmfKvdpLcoh
TLSHT1ED11123E836E612AA7D806C59B8E353F438D4039462D0E1852F6D5DB114F46D11A7F72
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