Result for 0DBFABB6D0CE6E4E4671350F9E68FFBC49F728C4

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/cpl/plugins/kmos-1.3.17/kmo_noise_map.so
FileSize14908
MD5E96D30520F362361911F830A0A21E93C
SHA-10DBFABB6D0CE6E4E4671350F9E68FFBC49F728C4
SHA-2563D674109DF87B1E7C99DEDA22E63FD49333A5C5EB33FC8B185927E3F18755D47
SSDEEP192:+8pI7cz5HPpX3Qgc2EwjH7Encmy32l8hgsG9gNlbJTNrXHyXQP:GixxggTj9JpF7X
TLSHT17462A30AFF86C9B1D1A0D3F6004B5769D2384014FB67FB63784D9A9ABB0535AC42D336
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
FileSize610416
MD544FA0A1C0C19269B5B2EA11B38540EDA
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-16B4577088E823A12EC620A52682D54DD9878E2BF
SHA-25635FF66FBDE8FC1A092410C408CE392EB2EAD800546E14982106D0113628336D9