Result for 0085D8ED0710BD68455FBD40FE140D0606767F55

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabihf/cpl/plugins/hawki-1.8.14/hawki_step_detect_obj.so
FileSize18700
MD5612376B9B22F2F1669FD95743BC2AAF2
SHA-10085D8ED0710BD68455FBD40FE140D0606767F55
SHA-256B768EA69CE8D324571415FA91EB02E4FF7FC30D527578CF45BB75FA837740CAA
SSDEEP192:LBHa8prvxJgZgxljA1TH30aSpBKeEKOT5bLIbqXXtIHfP372FbtG7sOjHDmkLrsQ:dxJ3xI3vSpk9X+fPL2LG7m
TLSHT1A282B5CA6E17D897C4C52339D86FAE178B19C189B3684F5F218E54647D02ADCC23AF87
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