Result for 1880521DAED79A40CD79B17604E00A0282395588

Query result

Key Value
FileName./usr/lib/s390x-linux-gnu/cpl/plugins/hawki-2.4.9/hawki_detector_noise.so
FileSize23832
MD5D51ADCA923557B920408547A724DDF7E
SHA-11880521DAED79A40CD79B17604E00A0282395588
SHA-256497380062FD2135B2A229E2BCB0E6F5C973C0F04FE35EB8727F4E5BB30C9D503
SSDEEP384:eCRuverYSAXx2fslyhwrcOck/GYcnLeG8H0fCknbCW:eCRuverYSQ8EyhFOcCsaoCkn
TLSHT116B2C69BEF769E9BC0F8BA32804F93B9E2774530B6854A05375C83140D17B904A3DAE7
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
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