Result for 1C457F07B9A965557954E91E221DD5226892EEE9

Query result

Key Value
FileName./usr/lib/s390x-linux-gnu/cpl/plugins/hawki-2.4.8/hawki_twilight_flat_combine.la
FileSize1068
MD59D9111759E0FA6CA65237A6EAC39F6F3
SHA-11C457F07B9A965557954E91E221DD5226892EEE9
SHA-2560369C71F09B5EB59EC393070920AE22AAF75F23117EF65339170ADCB01C9C654
SSDEEP24:JeSG5WJEOiE5xIY+Ahmfvi4HvD2NGDe5/jr:TG5WJcaxIY1hmfKELcjr
TLSHT13D11203E87BE3129A6D00A46DA9E332F47C980BA03514B1083C6EADF21934192157F77
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