Result for 010E63B23FE620B21190D12D6FB7807824391CFC

Query result

Key Value
FileName./usr/lib/aarch64-linux-gnu/cpl/plugins/hawki-1.8.21/hawki_step_stats.so
FileSize15232
MD564274EF0BBDDBD9E6FD775345B400E97
SHA-1010E63B23FE620B21190D12D6FB7807824391CFC
SHA-256E1590F9D2C148195F575158AF61F2C7DC4C8E6F55453B53C75AB78824D5AE9C3
SSDEEP96:YhFiBWBP36N3Vr4l/WwqrfJVBWRbC048PWRk3B2diOzP/T9VgoF0hGjlzYAG3yQY:Ii8p36MnqtVBUOAWiB2diK1jlzM3yQ5
TLSHT15D626199ED98D93FCDD022794CCB0F3CB7A14419A716838B221D09686F437AE4E3A55E
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
FileSize166042
MD5B97749A724F73C32C3325C17663564D8
PackageDescriptionESO data reduction pipeline for the HAWK-I instrument This is the data reduction pipeline for the HAWK-I instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO). . HAWK-I is a near-infrared (0.85-2.5 μm ) wide-field imager. It is being offered for the first time in Period 81. The instrument is cryogenic (120 K, detectors at 80 K) and has a full reflective design. The light passes four mirrors and two filter wheels before hitting a mosaic of four Hawaii 2RG 2048 * 2048 pixels detectors. The final F-ratio is F/4.36 ( 1 arcsec on the sky corresponds to 169 μm on the detector).
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion1.8.21+dfsg-1build1
SHA-11A54E42B7554DE056107B4700225D916C9932974
SHA-2560E51D833B4411CD82D6A2A5FE156078517284A85462E8AC7D767EF137DF6136F