Result for 170C24890E99FACE585564EEF661F7238E5AB9E7

Query result

Key Value
FileName./usr/lib/s390x-linux-gnu/cpl/plugins/hawki-1.8.21/hawki_step_subtract_bkg.la
FileSize1046
MD5FB7769C825E9F6E8E92F4341A6379656
SHA-1170C24890E99FACE585564EEF661F7238E5AB9E7
SHA-2567B8E26BB9FDAECA6B0FE05C0E5A1A9CB7DAB61DE49887C77EBF21CFC751A3AF2
SSDEEP24:1eSGWWJEOiw5xIY+Ahmfvi4HvD2NGDe5/jxn:3GWWJc2xIY1hmfKQLcjx
TLSHT16911F03A83DB9125BED40B5D8ADF703E429948790A2A5F1053C798DF128B43B2557E23
hashlookup:parent-total2
hashlookup:trust60

Network graph view

Parents (Total: 2)

The searched file hash is included in 2 parent files which include package known and seen by metalookup. A sample is included below:

Key Value
FileSize220720
MD5E4E92A0B8190448093C1085FB0D1AB85
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-15F53BAE9EC1154ED30C70C9E236D9A12E80D8EED
SHA-2567104AFD5FC486C6AD3216BF94DBBF5645F48AF5AA637F090A9BBBDD4D0A7C17C
Key Value
FileSize182452
MD5EF08A2321C9439CC934330A4A5C4BF24
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).
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion1.8.21+dfsg-1build1
SHA-10719138B7E3D860ECEB47FD703C3FE69D4B2F7AE
SHA-256892AD0D3BC3DF8545BA7454295F7C457B2BFBD5E913D4537D99838C60A222AEC