Result for 0F14D6E382092D0D17AEF4C9275F8C9DF34004C3

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabihf/cpl/plugins/hawki-1.8.14/hawki_step_stitch.la
FileSize1022
MD57773BC1A900BC107976C0FDA81C0FCDC
SHA-10F14D6E382092D0D17AEF4C9275F8C9DF34004C3
SHA-256AABCBD6244A6B09C73058F200F587E439A4D79BB0BDD8D2DE5932E58C2DE92B1
SSDEEP24:HeSh+WJvikxIK+Ahmfvi4tvD2NGDe5/Aj6:tAWJKkxIK1hmfKaLcAO
TLSHT1EB11423A935A1236ABD005890B8F713E4789487C03610F4062F784DB118B4091156E63
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
FileSize182644
MD5B913E5F643EB90DB738980D1B4AAD78B
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-1FA7B88CE6E858920EE04E01091AEADABC91BEEE8
SHA-256D9CB21642275832CBB1599E32BE54633E9B29C8FFD3316B6EE9E95706D7E4F26