Result for 1A228FE38CC9E624F4C980B3758A9EF25AA3475D

Query result

Key Value
FileName./usr/lib/powerpc64le-linux-gnu/cpl/plugins/hawki-1.8.21/hawki_step_stats.so
FileSize68424
MD5ABFD120987C6A522F2C5F830DFEBD809
SHA-11A228FE38CC9E624F4C980B3758A9EF25AA3475D
SHA-25605D19DD18A07E54022689E95744450ADD2ABBA263AB8AEDFA82EC275F677A89D
SSDEEP192:ZW58phjwtoD2Nr0p8YzUCzDit67JRjlzFU3yQSaO:ZWwjwg2Nro3DVdRhhU3h
TLSHT1866355A3B77DAE1ACBD43534A1AE027532A16E4357228313861453356FCA77C8E3E61F
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
FileSize224692
MD5D1343C262A1A7E0BD8BD4569E23F068D
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
PackageVersion1.8.21+dfsg-1
SHA-15671A6932A008A7BDE978A313EC947BFE2999B20
SHA-256136A0A4E926B114E41A51F5D4B1915255A9E2B8943770353493F216FBD564D4E