Result for 2B71E5B1CF56F5BF5976F9F55B6AA3D6C0684464

Query result

Key Value
FileName./usr/lib/s390x-linux-gnu/cpl/plugins/amber-4.3.8/amber_spectral_calibration.la
FileSize1062
MD5D614FF68D2BAABE9E34C938576ECF411
SHA-12B71E5B1CF56F5BF5976F9F55B6AA3D6C0684464
SHA-256BCE2177D20CFF3B850410B828BB98B93E8F315BB360C3242686C1610F0CEB159
SSDEEP24:KSeSGWWsmiYRxIY+Ahmfvi4nvD2NGDe5/jAKn:KSGWWKgxIY1hmfKiLcjAKn
TLSHT11E11DA7BC38C81297EF15A9A45CEB03E42AE683C0E614A1583CAC4DB168B45D3786F37
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
FileSize300164
MD5B93913D32BFB3DF10E706CE6153354BF
PackageDescriptionESO data reduction pipeline for the AMBER instrument This is the data reduction pipeline for the AMBER instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO). . AMBER is a near-infrared, multi-beam interferometric instrument, combining simultaneously up to 3 telescopes. AMBER can be used in Period 82 and following with UTs or ATs. All possible triplets of UTs are available, and a number of selected AT combinations.
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecpl-plugin-amber
PackageSectionscience
PackageVersion4.3.8+dfsg-1build2
SHA-10FE03E710B5466CF4CDA7440136BD1179BC3D1A7
SHA-2569419FD81FDF34223B754665959B0EE8CA1D67DA87A6F8FF623DE5E7E8FD60884