Result for 2EDEA56B82D7FB0DA49CED7DC05E7A74A2E3C8DB

Query result

Key Value
FileName./usr/lib/s390x-linux-gnu/cpl/plugins/hawki-2.4.9/hawki_tec_filtchk.so
FileSize10704
MD51AE4B55C2C9CC43068C8BB0F5A70B2DC
SHA-12EDEA56B82D7FB0DA49CED7DC05E7A74A2E3C8DB
SHA-256E3BFF31295044F5E1CD9B3692CCF00A17881EEB24379BF225B8A1F56F6546DDF
SSDEEP96:RxQXpmBWBA3wQmVs/VYxnojV9Jisgi4U/cqCSG40qSUj52yuQ0CR+Ar9crF:gXc8quV+kkV94tUNxow52yuQ0Cowc
TLSHT10322624F6F7A8CA9C6F43B34458F4378627A5910F3464F027BDC43505D13B905ABAE92
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
FileSize447560
MD5313F0A8BE77EE12C7AF31C26CE90DC22
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).
PackageMaintainerDebian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion2.4.9+dfsg-1
SHA-13807DF06BE1E959160FCB49D785AAEE6751E71BE
SHA-25636FAFBF666EB029A87DADFC2A4503881FB8C4DF4DA5FAE8B9768C2EE810AC74C