Result for 1ACAB3E50B9C2F0382C1C540C821501604AE1472

Query result

Key Value
FileName./usr/lib/aarch64-linux-gnu/cpl/plugins/hawki-1.8.14/hawki_step_stats.so
FileSize15232
MD506E77B6B44D15858F2B6FE37404B390D
SHA-11ACAB3E50B9C2F0382C1C540C821501604AE1472
SHA-256581A3660EEF374C277E925DFBB845A8F03114851D3E38155230960977B1BA2C8
SSDEEP96:k2qCBWBP36N3VrulVxdvwqrfnVBFnYOIzkj6W2EeVnemb9wrGjlzYMO3yQyn+3m+:kC8p36kDYq7VBZY3Damb9fjlzQ3yQy+
TLSHT1096274A9FA95D93FCDD06335498F063CB7A18409B7368383A10E0A646F437AE5D3A54E
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
FileSize165216
MD5E12BAB3979675ED66624430A2F31F9B7
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-14A0285D01B6819014CE86C3B6D1123F6534E36C5
SHA-2564F99F67FCA1A126F63922C859CAC6A04492F38E7C20EEF6402A54CC39E32AB46