Result for 152F9731F8149C75C56141EEC603F8DAA35E0FF6

Query result

Key Value
FileName./usr/lib/powerpc64le-linux-gnu/cpl/plugins/hawki-1.8.21/hawki_step_stitch.so
FileSize67936
MD51EFF35D5C2E1200E35EEA2DB06601F9F
SHA-1152F9731F8149C75C56141EEC603F8DAA35E0FF6
SHA-256D87804BDE02C25A77DD10932CAF60A854F55987BD4C6252036CC0F7F2C9505FC
SSDEEP192:ir8pOvuz72noSppR8feuk8055jPb7yPrQIIT6aZ:iBvs72noGOeuk8055jPfyPUZTb
TLSHT11F632267B3BD9E4ACB803635A19E067033616E8643128713A66853741FC7B6DCE3954B
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
FileSize190308
MD54A9C354B9047366270BE90C85A9082F1
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-1255B34E4F87A4AB7107B747E7A67F6995239722E
SHA-256BB9CA8E6CCCE01596EB08FC791C6ECDF3554D3E2D18DC55330F7EDA7CAC17BBF