Result for 25668109011E12DCDBE13EE33BCDDC453ED01B47

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabi/cpl/plugins/hawki-2.4.11/hawki_standard_process.so
FileSize68808
MD5A0F3FCAAED02AC03B5A604A0D0BA4EE7
SHA-125668109011E12DCDBE13EE33BCDDC453ED01B47
SHA-2567EC48A341B1C2D5F1759A4EAB6BCBD44DBBF699F534106D5E7B0078FD53EE2A7
SSDEEP768:7DYR2VhX4lHa2SMjZhNyOhRbIr3ftAC98wZ/BONFO+lO6vhBJd:3YR2VI62hsOrbqfeJCONFO+lO6Fd
TLSHT19463E89BA9A25EF3C5C49530358E8629B32356B0C7DF7703550CD23C6EB259F412AB8E
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
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