Result for 14B620D96A5BB4272938987D5D8D50499085C283

Query result

Key Value
FileName./usr/lib/s390x-linux-gnu/cpl/plugins/hawki-2.4.3/hawki_step_compute_bkg.so
FileSize27888
MD539152F24624E0EB99B49631014486F22
SHA-114B620D96A5BB4272938987D5D8D50499085C283
SHA-2562965E42FA4D246D2DDE1C503BDB88B412B4ACAADAAA348BCE1C1C1AF10ADA9C3
SSDEEP384:clVrG0nq8/wV+55DthnfL8VL+8X2PcCP0jhSr7VSjd3PEC0y:cXi0nB/wUhD8FR/c0ti7VSJ
TLSHT1F0C2E6D79D62D9A9C8F07572921F8B7A8A772CB8B3854B0077ECC3701903B54AA36D71
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
FileSize468408
MD5AFB8672F4237B6E084ADD1D7965FEC77
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
PackageVersion2.4.3+dfsg-1
SHA-15F5A26B6ED1A94FCCDB5418A6EA9D38509C7832D
SHA-256A8BF33C01629FEB6CE296AB321AF3C889D6452D6BE48DD6507E7D949D35B2061