Result for 0084A32DE3938FD39292BE547B15D867E2A92E82

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/cpl/plugins/hawki-2.4.3/hawki_cal_flat.so
FileSize44052
MD5C72F3F1A5907CC09296387CC6DC4B8AB
SHA-10084A32DE3938FD39292BE547B15D867E2A92E82
SHA-256907B84E94F8211DC0163B971E9AD075F64823CF6E89E255A4AC2F7CF5F8F1E78
SSDEEP768:AFb6CG4owBgUsfTRlHCcpGwADKyfQKX2SIn3Rorm7rtXfSnW6:AF+C+wBgUstXUwZy8n+mlXl6
TLSHT1DF13A6CDDBE2CC74F29304B514EB26B488700511B633C7D2EE89218D5E266AD9A3762F
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