Result for 1D8453337DF98BE055069E7A4230F13283B2DD10

Query result

Key Value
FileName./usr/lib/s390x-linux-gnu/cpl/plugins/hawki-2.4.8/hawki_science_postprocess.so
FileSize45328
MD5E782C31D83CE066EB3A3C8B6E0127861
SHA-11D8453337DF98BE055069E7A4230F13283B2DD10
SHA-256B7B58D96119632DC57972C13A79D41E0F607149667719005E315941D9BC2BFD3
SSDEEP768:D5LoxaUezpqS9d6CjzccFdmcymUAV1ABhgh1PVQ7evlL:NdUeN9d1ccFdmc/U3v7ev
TLSHT10213E6CBCE36CBDEC5F03631A44F417AA67B0536B71B0A18779C83149953B146639BB2
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