Result for 1F8150473F37EF9D72C7CF82F283643306834408

Query result

Key Value
FileName./usr/lib/mips64el-linux-gnuabi64/cpl/plugins/hawki-2.4.3/hawki_step_compute_bkg.so
FileSize28608
MD58E4FF0D5B586F6F0141A7EBD8B37B4BB
SHA-11F8150473F37EF9D72C7CF82F283643306834408
SHA-256B656A8B07453B7BAF081C1DA1C057FA1391CCADE13D7E7E1FD5C03BCEA458DCF
SSDEEP384:w7vm8/wR90yIO5AoNoYyZlg8x2yVICoZT+rLOG30ys/:w7vN/wR90yIO5AoNoYyZlXSj1eLU
TLSHT106D2C6A3EB542E1BD6E0CD32942F8675063D9D6AB2209743DECC82B45C4FDDC4EA194B
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
FileSize459464
MD5BF5AA2AF1FD8B5940C7561CD404DCF95
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
PackageVersion2.4.3+dfsg-1
SHA-1FBE7872286CE89B53E0544E3D1E8C86BB09581AB
SHA-256A6ECB0026D06870834397818D25A9044D0089E2CC575310F24458F40D0F1B52E