Result for 1C51A8BFD23D650BB46748524EDB89365FF40FEC

Query result

Key Value
FileName./usr/lib/x86_64-linux-gnu/cpl/plugins/kmos-1.3.17/kmo_noise_map.la
FileSize988
MD568FBBAA4AF30135DF0087ACC7780C82A
SHA-11C51A8BFD23D650BB46748524EDB89365FF40FEC
SHA-2562078C2AF789026EE248C196DA099E993E3B1FDDEE37BFA55BDA5B8458D4874B2
SSDEEP24:p1eShxWpvihuucxIK+Ahmfvi4LJvD2NGDe5/bOLI:p3HWpKhuucxIK1hmfKgNLcb/
TLSHT1E811023B9388923B37E00F594B8E316F43D94838461A0E2042CA95DF274B81665E5E37
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
FileSize579916
MD506562B457CC1A73E1FBAA2E29678DA03
PackageDescriptionESO data reduction pipeline for the KMOS instrument This is the data reduction pipeline for the KMOS instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO). . The K-band Multi Object Spectrograph (KMOS) is a second-generation instrument designed for operation on the VLT. The key feature of KMOS is its ability to perform Integral Field Spectroscopy in the near-infrared bands for 24 targets simultaneously.
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecpl-plugin-kmos
PackageSectionscience
PackageVersion1.3.17+dfsg-1
SHA-1F8C56CF45D847A412E24F68FB1A7598486CDEB06
SHA-256FE9BC68AA752B7CB593008328A2F0F8D62A5C3867EC2094B989E7094BD85E16A