Result for 188AE4614A335BC5750300FCB6ADCF81E36DA0BE

Query result

Key Value
FileName./usr/lib/mips64el-linux-gnuabi64/hawki-2.4.9/libhawki.la
FileSize959
MD5BEDED8D703D51A1BA0AEF6C3CFB51A73
SHA-1188AE4614A335BC5750300FCB6ADCF81E36DA0BE
SHA-2560E047B3A6F9F65834390EB60DFACD2D32CBC61AD79FB0B14DFB4537B241947F0
SSDEEP12:o4fWgxGb/r5WFKiJLiORxIha+AAmBB7Szf77ixCFlvT3RTZ/9IMCDwDqaAlH/FYx:jeSG5WPimxIY+Ahmfvi4lvD2N0De5/u
TLSHT1A711BD7AD39A4A3A7BE44A555AEF302F835E847807670D1052CA99CB234782E31A5F72
hashlookup:parent-total1
hashlookup:trust55

Network graph view

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
FileSize432820
MD5C12CBBEF48D8105D146F3F56E4FC6A80
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
PackageVersion2.4.9+dfsg-1
SHA-1E41BD0569D8F9C390A871D226FEBCF087EAA5725
SHA-2561645C1BA99874DEA41DB29C0692F68499585F6E8E7C1FA36686DA058B91EFAFC