Result for 1242437342B98DFA6E01366EE228E65D118240BD

Query result

Key Value
FileName./usr/lib/mips-linux-gnu/cpl/plugins/hawki-1.8.21/hawki_tec_filtchk.so
FileSize10232
MD58E72DD75227CB7E4F9D5AC718AAC30CD
SHA-11242437342B98DFA6E01366EE228E65D118240BD
SHA-2562C48C26176C6E8E0F2994173C7B082462E5A431DD92FDB468C107BB34F8E2140
SSDEEP192:6WiSnC2kB10qy98p36KwV9v3kKFdDTk8qyelldh5jXy8S3S:6iC2fvKwVR3kKr/e3djHS3S
TLSHT19D22C68F33519D1EF1E2D338B46BCB6137984661699807279A6CF04177097AC183FEEA
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
FileSize226012
MD54C289725D3042772C3CC4229546F32DC
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
PackageVersion1.8.21+dfsg-1
SHA-1889A99B4EFD1D9875279122129BC03E6D652C846
SHA-2563E3320066BBF6E79776FAB1ECD889581BBED37D5A340ABF0247820338B9C6E8C