Result for 0E2EE734DE63B5889359545990CB6DDE583822D5

Query result

Key Value
FileName./usr/lib/powerpc-linux-gnu/cpl/plugins/hawki-1.8.21/hawki_util_stdstars.so
FileSize67144
MD53BCD3F1D8DA9343177E5E594749EEC9F
SHA-10E2EE734DE63B5889359545990CB6DDE583822D5
SHA-2561D86EFCD69EBB63A6B16FDF1FF6A47545A2D098144ABDE0F22220808041265F7
SSDEEP96:RwQlDx1RBWBPJx7fdkBswEmxaoDpmNsjKy8tSHbbn5gXKnXaj+z+UKAL+UbWJySB:RfdR8p/fPmYUmM7bbWuqusOWgM
TLSHT18C633046B31F4827C2D03BB842EF6311632DDE81D71A832F5299125639F1B6E582ABDD
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
FileSize187838
MD5A024F16A962750A75766BD108C2F7C83
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-120C6AEEBCCC03D080FE5001A90A75B22E3AC1CE9
SHA-256CBE18A9EE3DC715B90F92BCDC01F3CC3784AD46A1370F0A245A67339F4907F7E