Result for 0F23C8A2EF97FFE1A41FEA3DCDAEFE1259FD3EB7

Query result

Key Value
FileName./usr/lib/s390x-linux-gnu/cpl/plugins/hawki-2.2.0/hawki_cal_dark.so
FileSize23680
MD5310D816D309488FA40C8BB0599A83504
SHA-10F23C8A2EF97FFE1A41FEA3DCDAEFE1259FD3EB7
SHA-256C6332A0BEDA042B5A514D1CF864AB16663045F5440E2C9E6EDB0D64F6D33EE03
SSDEEP384:FBUk5wapVk0WK8a8aX/KJgQTHaeJGV58NLbY:FBUkbb5WHahV58NY
TLSHT112B296EF9E364EEBC4F87B32520FD579E17B093177488E14779C83544C0ABA489349A2
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
FileSize363444
MD5008665630BEAB04AA3E699DF53464A28
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-1016893D9A8DABB8BCACD581CEE5327857904F01D
SHA-256C671E8C5D435484D7BD2ADE46FC2CAA48D49C8518AE118BED3AB6D604EE5336B