Result for 08F8DBC83F581930BEB62DECF7E99D8730B5D2F0

Query result

Key Value
FileName./usr/lib/s390x-linux-gnu/cpl/plugins/hawki-1.8.21/hawki_step_basic_calib.la
FileSize1040
MD5D4078F381A30B1F465923C73A1B0BF25
SHA-108F8DBC83F581930BEB62DECF7E99D8730B5D2F0
SHA-256BB59CFE604B00453EA9D976253A50C9EF98CF2162F6386BA846C9F4537C2E6D7
SSDEEP24:SeSGWWJEixxIY+Ahmfvi4yvD2NGDe5/jxn:SGWWJ9xxIY1hmfKtLcjx
TLSHT1F311F07B83CE9269BEE0599586CF7C3EC28D84380A314A1452CBC4EB114B4192356F63
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