Result for 0637FC00AF030565BE4095DB08F4B60281E7B149

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabi/cpl/plugins/hawki-2.4.11/hawki_science_postprocess.la
FileSize1058
MD58FC2A899CD02988880E78DB3FC594C4B
SHA-10637FC00AF030565BE4095DB08F4B60281E7B149
SHA-25681B56264BA7EFC552496594E39B32215F3AB2552800408576512FF29242A20A2
SSDEEP24:TeSHOWJ7icxIY+Ahmfvi45vD2NGDe5/AjI:huWJ+cxIY1hmfKKLcAk
TLSHT1BD11BEBAD3CA4D666BD01545A6CE302F4A8A843C0B1A0A7493C6D5E7238742A1156E3B
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
FileSize460432
MD5C4C5EBB37D7DBB8298549F3C6954D382
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
PackageVersion2.4.11+dfsg-1
SHA-1CD3572D24E59B9C5CC2677F15ACDA24FFDA85C4C
SHA-2564ACCFB4EC42FBCD04415B3421FF1F11B47DE7CE1669F475BEC1727F12E938654