Result for 2B9D75715FC15D06391C6B77AF72EF90D2BABA87

Query result

Key Value
FileName./usr/lib/x86_64-linux-gnu/cpl/plugins/hawki-2.4.9/hawki_step_stitch.so
FileSize15032
MD5C845D61C64CCAD41525373F6F3F520B5
SHA-12B9D75715FC15D06391C6B77AF72EF90D2BABA87
SHA-25667A6F34F98E735B52C5678C14C12C343026CE19ED376D9EC2F65BD8ADF3C93D0
SSDEEP96:RF0943OBWBf1fzquJ0uNBnoz4mAZOkYCfKGJ7+eG/pcOvYimGK6qaH6/w9+iVvfo:R53O8LvPNJhmoiGJ7ExcKYnDe6pi
TLSHT13A62736BB7A48DBAC5D41270108F073526B69C65EB218B13395C61740F437D8AE2BBEB
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