Result for 148CF422E12D03DA4DD281DDC7085671C3D513D2

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/cpl/plugins/hawki-2.2.0/hawki_twilight_flat_combine.so
FileSize35428
MD5FA62FE3CB88302C2440281E5DAA39CCE
SHA-1148CF422E12D03DA4DD281DDC7085671C3D513D2
SHA-25625B2B870F9F4E70FDCD241110A28275A4002AE25A0CE4AE8FED8D6EA408BF48F
SSDEEP768:yeze0fTRlHCcQkFeqlwFT6AqF87lGvRODf9jf4UzOKstzY5T97gkE3:Bze0tXQk/6qF8EwZAUzw+M
TLSHT157F2D89EFE63C5B1D7C299F43807433FE6208611B18BC3C2A6487A64546324D9DAE77E
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
FileSize438120
MD5F14E612CDAC168854029D313E0FF1BC8
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).
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion2.2.0+dfsg-1build1
SHA-125C318905E702AE7B4F69DF645F83D37B0452B9E
SHA-256F63148016DA1AE247452781483A4BC1347D39621941BC5D9B51B2F5CE00EB9CD