Result for 0CDCC661AA5732ACE6183FD15518C8DBB8E505EB

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabihf/cpl/plugins/hawki-2.2.0/hawki_cal_dark.so
FileSize22752
MD58362AF8AC56FB011A5897172804C92A0
SHA-10CDCC661AA5732ACE6183FD15518C8DBB8E505EB
SHA-256052E7FEE69EE71816F43B19E6DAC9BD3613B37A773D7E71DD14B097B03A93423
SSDEEP384:BENFMXfPpDH6MLzzpUDeyI6Up4V0hURLg:uNFkRaQnkI6cOC
TLSHT1D4A208CD74977A2BC9D02535240F8F7729510DE08EDD0B132F4C4D941A92BAD8EBAE4E
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
FileSize353598
MD5A1BD40963DB2A77A0D7730FE85D0AF94
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-1EB736B139332F6B26DE6CFF7CB6FC31819963E2A
SHA-25697C93587330F9AE975DB4E10FD12ADD6E9FA3078083991808F019B208598BCBD