Result for 0E8F8777596D36E67BEF392289352BB0927D8417

Query result

Key Value
FileName./usr/lib/x86_64-linux-gnu/cpl/plugins/kmos-2.0.2/kmo_noise_map.la
FileSize983
MD5021A7B0DD3FE6985F61681330321B14A
SHA-10E8F8777596D36E67BEF392289352BB0927D8417
SHA-25637CF15C3DDB2A5DB95993A7678DF98E5B12CFA9C8663B384D730477C56374CF1
SSDEEP24:p1eSG1bWpvihuucxIY+Ahmfvi4LJvD2NGDe5/boc:p3GVWpKhuucxIY1hmfKgNLcbR
TLSHT10311023A9388813F3BE00F494A8E317F43E94838071A0E2046CA95DF374B41625E5F37
hashlookup:parent-total1
hashlookup:trust55

Network graph view

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
FileSize615044
MD5B5225B731ABEA5F82102DF9C51EC9E86
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
PackageVersion2.0.2+dfsg-1
SHA-1514B556170FF20CC66D91F15AE408C369D9A02B1
SHA-256DB7C65BA400DCCBAC930C139061AA774FE0F0BFF562719DB4F000B9E2659A522