Result for 03CEA9266ACD70C79C680A82A308A1D301770E6A

Query result

Key Value
FileName./usr/lib/x86_64-linux-gnu/cpl/plugins/hawki-2.2.0/hawki_step_subtract_bkg.so
FileSize15192
MD53479BD74BA6359E204BC22FAE9B088B4
SHA-103CEA9266ACD70C79C680A82A308A1D301770E6A
SHA-256A2D677B0EED19D2AB58FE135C8885FC35AA364DADF712667B5B4AE1C61495BF2
SSDEEP192:RW38mWsb/9OTKCAfaUG6d+sHDjxF2iDng+ZM33i:EWO/9O1ANZXjjPng13
TLSHT1A862C44FA7D28EBDC4D4533480CB02349A70A885FB31DB171658A5B85A067AC5F2BA9F
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
FileSize407134
MD58BB75CFCA14D06B369847DA5AD3C0659
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-157E12B5F92879BB2A2B01FC61AE6BF5307FC2945
SHA-2560A0320B5C8F5B44A2C6CBD2E98BE1B3BEC71DBF24EF43CE8BC2912388B5663DD