Result for 1246900AF990ECE80AA84761FAEA3E3A1CABD292

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabihf/cpl/plugins/hawki-1.8.21/hawki_step_apply_dist.so
FileSize10240
MD59997CB2DB061872D53C6B0F904E8AAE2
SHA-11246900AF990ECE80AA84761FAEA3E3A1CABD292
SHA-256099F4983986FA0865A53939E6C4FEA86EE0B68E23AA387CA14BB9F7BA69F59E3
SSDEEP192:fd8p9oocJ6EhYitnPH4HS/I6XUlSo2QVl:IoocIEhYOPHTI6+SUV
TLSHT1B92241CFBBD75D37C4D12978204F0E162694C4AB869B5B03778C23E81B016B9ED2DE4A
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
FileSize184482
MD52A9ACD5A8E062002F64B214A3B6B00FF
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-10600C46860A116FB748364715FA18ECAE1EBA0AC
SHA-2562F942E0CDB1F7E91576879FA81FC9A13FD3C56B3C0AFD51DFBAD967AC412F017