Result for 2D889D90D7B92A7313A24946BED6C444B7DA7A79

Query result

Key Value
FileName./usr/lib/s390x-linux-gnu/cpl/plugins/hawki-1.8.21/hawki_step_photom_2mass.la
FileSize1046
MD51D1B75E205491E60ED6D41CE9CCF5CB9
SHA-12D889D90D7B92A7313A24946BED6C444B7DA7A79
SHA-256BE87D374413C2E63316C93DF494F73AC42496C4BD9E813251C661368B2A21072
SSDEEP24:ueSGWWJNmifRxIY+Ahmfvi4qvD2NGDe5/jxn:mGWWJNZxIY1hmfKPLcjx
TLSHT16311423B839A152DAFE409465E8F347F43898539037D2E0442D784EF124B42932A6E22
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