Result for 0C70A56FCE6710D32803A259E9DA1E710E381420

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/cpl/plugins/hawki-2.4.3/hawki_detector_noise.so
FileSize31040
MD51431121A647458B36394021DE2F66490
SHA-10C70A56FCE6710D32803A259E9DA1E710E381420
SHA-2569CB2AEBB67ADC4729C8DE6BDCADB8B5BE36932C017AE5B7214732082213E4EA5
SSDEEP768:SEEverOPCwzPUfTRlHCcFnHTD5EgxdAyVt:SzCw7UtXFHTD5EgfD
TLSHT1FCD2095EFBA2C5B0D4C2A5B454974629C871CD01E226C7C2AF4F37812A3175CBE2E76E
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
FileSize548756
MD57B774D5D5C690C1AD50BAFC43FDDB0C4
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
PackageVersion2.4.3+dfsg-1
SHA-1B6C87AC7CEF51846AD1962434E51181D948F75F9
SHA-2564BB11E9B6BA556172558877F98E9B23702C96254E0C6CD3DF42D3C2B65C795F7