Result for 2DE0CB2008AC10B0D6335A0671434C1555ECE245

Query result

Key Value
FileName./usr/lib/x86_64-linux-gnu/cpl/plugins/amber-4.3.7/amber_spectral_calibration.la
FileSize1062
MD53CABF57F6ECBB9EAA3ABFE89D8933D3F
SHA-12DE0CB2008AC10B0D6335A0671434C1555ECE245
SHA-256C9008F2331A26F3478FA71621713D75D226FCEB66D4C5200AF2F00CC85CE7EEA
SSDEEP24:KSeSG1bWsmiYRxIY+Ahmfvi4nvD2NGDe5/bAp:KSGVWKgxIY1hmfKiLcbAp
TLSHT1BC11BB7B838CC1293AF1559945CEB03E42AD64380E614A1583CAC4DB168B4593746F37
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
FileSize333778
MD5202ECCC29F7723BEBD40456752899B3B
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
PackageVersion4.3.7+dfsg-1
SHA-151B46F1A2AA397E908F30A31BE9AF52942DD19F9
SHA-256C385F531F45D32A34B7C25AF4A5D80A335F82A857BAF7F60CC2246595601065B