Result for 154852A7C59E60D3DB78FFDF9BB55AC238D57136

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabi/cpl/plugins/hawki-2.2.0/hawki_step_apply_dist.la
FileSize1033
MD5A0292FE2EDEB7375294A15A02ED83BAB
SHA-1154852A7C59E60D3DB78FFDF9BB55AC238D57136
SHA-25671D6C19EE51AD410D21FF26866BF96BE69DC78ED70DA8DCF59E416C4F57BDBB6
SSDEEP24:FpeSG1bWJPbiNmmoxIY+Ahmfvi4rtvD2NGDe5/AjO:FzGVWJPeNmmoxIY1hmfKARLcAK
TLSHT1D711F03A934D4127EBD4158996CF313E424D883807AB2F54B3C7F4EF114F91A1156E26
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
FileSize442062
MD5E779873E6D359675CEDBC17AC57E9320
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
PackageVersion2.2.0+dfsg-1+b1
SHA-13C5CD869CACE89525DD780CA8081A8C6802AEDE3
SHA-256EB202A58AA0E86581745FF06F55E29A9F37826AF733B571458392DCD61AAD19D