Result for 0A4C003BEDC94518817C6EB9379B404E56BE6289

Query result

Key Value
FileName./usr/lib/x86_64-linux-gnu/cpl/plugins/hawki-1.8.14/hawki_step_stats.so
FileSize15360
MD50DAB38A6772CBAEBF1B6EAC730A87D5D
SHA-10A4C003BEDC94518817C6EB9379B404E56BE6289
SHA-256F7E6151614A132D3A9EA49E2D2A07F50A9CFA9AA59A53D6C6A0D6EE4ABB324DF
SSDEEP192:RSkk858phDgIFnLCcQ0NKwOnEDg3yQCibkhp0q:9whFn2Kpg3k
TLSHT1A462951F7A998E3ACDE46334109F0639ADF05491FF22D35B1A4C11B89A4279C532FA6F
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
FileSize195760
MD5AD2C0CE7BFA6DD0C55A03053260B56BB
PackageDescriptionESO data reduction pipeline for HAWK-I 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
PackageVersion1.8.14+dfsg-2
SHA-1086A952CA52A913571A4B157A2FACE4144827EDA
SHA-2562D7C4EE843C799609FC589F29F835C883F9AA2BE52375FA434E627D2452C14C0