Result for 27F92FC0D49106C648AFDBED9C2637E9C1EB6B24

Query result

Key Value
FileName./usr/lib/mips-linux-gnu/cpl/plugins/hawki-2.4.3/hawki_util_gendist.so
FileSize18592
MD5E878C93AB86862222D2CDC4FC579D870
SHA-127F92FC0D49106C648AFDBED9C2637E9C1EB6B24
SHA-2569E855EBDCB15C70F34888825D9F0ECE7175042A85CC68BAD86DFD8E7E3796187
SSDEEP384:4yg4gx5GwrtAK5nljaRstbm+W62j98NhxV156tNYuq:4yDgx5GwJrtmjGNv1fx
TLSHT1B782854FA3D25D1EF0E2C3B8A857C7E622A645706EC44A33C47CB046268C65D977BE91
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
FileSize471088
MD5B8FD83D2BD28D19D4560F9F25976C8F4
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-11C8FE32120734D45F159CF07A89DF8F4AE4700E1
SHA-25633B192C73AF4F5B97638210C15508D770F5731F4969E5D34D0864DB81751A269