Result for 11CE5D53D7C646665197916A88F0D848EC55B42D

Query result

Key Value
FileName./usr/lib/x86_64-linux-gnu/cpl/plugins/hawki-2.4.9/hawki_step_basic_calib.so
FileSize19216
MD5C77A752FFA36EF0F1EA9A33343D0D5DF
SHA-111CE5D53D7C646665197916A88F0D848EC55B42D
SHA-25695A91AABBA916BC20F8D8F1651E49A3E3097E6356B4FADF960CBAF672E19B1D5
SSDEEP192:RI3VH281DBUx9LhdpBVCpgdHiJm30wnIWji:GJDBO9VHBAg7EwnIW
TLSHT10282C5A7B2A14F7AC5D4767484C7473671787881FB30871B258822B52E417EC8A1FBDB
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
FileSize489816
MD50DC386B9AA2A31F951B2CAB6994240A4
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-1174D5C4F5AF18807F53EFF58FA4460491B0A01A0
SHA-2561A2BE31E56411C85A56DFA78B4D7E21032BB44C3A3A3C03F2A8F1F1DD66465F1