Result for 070727BEDC323514A37D592BFA1981D22427CC85

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabihf/cpl/plugins/kmos-2.0.2/kmo_noise_map.so
FileSize10728
MD5CF129458B6696DB6FE102DC928AAA9BD
SHA-1070727BEDC323514A37D592BFA1981D22427CC85
SHA-256B346EF4075F372C07CA16FC6411918F835C19D5AC5CEB3DE45A55C2436B3CA2A
SSDEEP192:Bn832RnlZnHpnRy+d/yP8n2xnQ+cV9mhy395brXHyXm:BjRnlZnHptd/yP42yB
TLSHT1BA22838AFE824A33D8E8DB3854874E07EF75C0886B1E5B13714D22A83F116788D6DF46
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
FileSize596736
MD576704A6E98FF40E94522D6CFE74B3FCB
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-13BAF7A9632D8C1FB465126E77ADFD91F2E318D11
SHA-256738849B7639228B04870B95186753EAE578729301ED26C54B2999B2DD8172EEE