Result for 04551C1CD3129207D52A132C002E2F4B5D2CEAD3

Query result

Key Value
FileName./usr/lib/x86_64-linux-gnu/cpl/plugins/hawki-2.4.11/hawki_step_subtract_bkg.la
FileSize1045
MD5733A10CEDED777732F5A70FF099C5DB0
SHA-104551C1CD3129207D52A132C002E2F4B5D2CEAD3
SHA-256F728A1FBBE5B12256764F0F7241AF1572C23011E21BC850AA12569D481731294
SSDEEP24:1eSHOWJEOiw5xIY+Ahmfvi4HvD2NGDe5/b1:3uWJc2xIY1hmfKQLcb1
TLSHT148112C3A83DB9125BAD40B5D8ACF703E429948790A2B4F1043CB98DF128B43B215BE23
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
FileSize494108
MD502A3A726877552855F37063639962D69
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
PackageVersion2.4.11+dfsg-1
SHA-1F0C3B24956A696442FCB32E293471A377BAA1960
SHA-256B278D9B2C829C63930C1DD03871AC2A331689C9689B54528681565BE256BB13C