Result for 15B50B6D526BCE77494D771218311F85BFE52B62

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabihf/cpl/plugins/hawki-1.8.14/hawki_step_stats.so
FileSize10460
MD5D726B918A722E2C4AFD9D3DD2212FF49
SHA-115B50B6D526BCE77494D771218311F85BFE52B62
SHA-256C357273FD16C87EBFBA933F427ADE3C0DE6571545BF497660130E421866357A5
SSDEEP96:ypFBWBPhN3VruldxlxHDwORtLUNoC6smngOZTGjlTYDRE3yQyhXyguvH3/M:w8phKl9DweLUNVOZCjlTL3yQyC3
TLSHT14C22A89AEAE77D67C8F42075024F0A2D747DC8A057A58B435D0C00A4B9163ACE1FBF5B
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
FileSize182644
MD5B913E5F643EB90DB738980D1B4AAD78B
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-1FA7B88CE6E858920EE04E01091AEADABC91BEEE8
SHA-256D9CB21642275832CBB1599E32BE54633E9B29C8FFD3316B6EE9E95706D7E4F26