Result for 0DD8F0B18FDF8A48323F485DF790806E3E654AB4

Query result

Key Value
FileName./usr/lib/aarch64-linux-gnu/cpl/plugins/hawki-1.8.21/hawki_step_stitch.so
FileSize10640
MD594CCFAE9D59620A4AD0EE42193E4FC5E
SHA-10DD8F0B18FDF8A48323F485DF790806E3E654AB4
SHA-256BE020B647C90C3C89733FEB6806FF2C0D786856DD21E6F8D3D95727665C54E52
SSDEEP96:f0tAp88BWBP/1fzqulvw6ku4Dl1beF7WSwk7OmJD7pHivvoxxG/XrQrIu6F+3X1C:Tp888pBvwnu61qFqRk7JZDyPrQEu6c
TLSHT16822735DEB94DD7FD8C823355E8B1B3473918649E308C367B04C9654AFC27EB0E2258A
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
FileSize203830
MD50217B24BC288D83D67B33CC086B6DC72
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-1A3D2F47DDC44170E6E18F65F24ECF6BC5365A200
SHA-2568BAD397247F133240BFF3538BA243E921F9D81B6F302F0F295AE0F28FE15DF22