Result for 15EC74CC127F9F0B814FE76AF3908003FAA99B45

Query result

Key Value
FileName./usr/lib/s390x-linux-gnu/cpl/plugins/hawki-1.8.21/hawki_step_compute_bkg.la
FileSize1040
MD595B7F0A47E7B493193EDA163B4BDB239
SHA-115EC74CC127F9F0B814FE76AF3908003FAA99B45
SHA-2562903209A31B2F53F10841FD0888C3353A5DA8C40E2149A55D2A59736FAF2C206
SSDEEP24:0ReSGWWJmyOicJJy5xIY+Ahmfvi4C1vD2NGDe5/jxn:0LGWWJmmcJJwxIY1hmfK7pLcjx
TLSHT1A611E23A83CA5125AFE04A86579F303F428A487C07266E2052C7D9FB114B82B3156E62
hashlookup:parent-total2
hashlookup:trust60

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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