Result for 201A584F21735C6102F37F2529C82E89D959C2E8

Query result

Key Value
FileName./usr/lib/s390x-linux-gnu/cpl/plugins/hawki-2.4.8/hawki_science_postprocess.la
FileSize1056
MD5B6C9B2E4D12913B6B6FC786E85CBC9B3
SHA-1201A584F21735C6102F37F2529C82E89D959C2E8
SHA-256DB364AF8A68B95D04583208D15ED103FE60D29CA0898EEB0E33EFFD1BD2CB8BC
SSDEEP24:TeSG5WJ7icxIY+Ahmfvi45vD2NGDe5/jr:hG5WJ+cxIY1hmfKKLcjr
TLSHT19911DDBAC3C959666BD01945A6CE302F4ACA843C0B190A3493C6E4EB278742A1157E3B
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
FileSize447632
MD533FC2B0C89624E65DA7B1A1A7C293E5D
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
PackageVersion2.4.8+dfsg-4
SHA-10B922EA38B7546D45FD6C7684420AF3A767B96A4
SHA-256D1FF152F6C9ECAF1CF7282E6A5365DB706C7490C3F8999E902AAA1A8383EECE3