Result for 1E6918795B7F4F5B96AF32288819625330B0EEDF

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabihf/cpl/plugins/hawki-2.2.0/hawki_science_postprocess.so
FileSize39964
MD58DC173E7206330160F7B8101BED12654
SHA-11E6918795B7F4F5B96AF32288819625330B0EEDF
SHA-25688385364B87807F764A3ACF4D51BE3544976B12143C14C86508508B32EC0F672
SSDEEP768:NsclCv6pqxv2qj3Lshdb/Otzh4/m3Ue9u4mOn7ngtmXjYffPQLz:iclCvHv2cLshhKu4mOnzgteX
TLSHT1CE0308C5A8915FABC5D05231329F8B29723352B0D7CE3747910CAA493F8768E8936F5E
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