Result for 094B43C789833BD2FBB884E4198109EFBC892B30

Query result

Key Value
FileName./usr/lib/s390x-linux-gnu/cpl/plugins/hawki-2.4.9/hawki_linearity_analyse.so
FileSize27864
MD5D25FBA15C542AC4D63907ACCE69A8609
SHA-1094B43C789833BD2FBB884E4198109EFBC892B30
SHA-256BDECE0AD6685EAA556F8840DA8FA4FBC819B0A03B74E6AA71E6978388024480B
SSDEEP384:GPCoczHQXGceRp0bsFkHgunpTVrpNquY+0W8LE9WNu/TB:G65zHt9vJ2FphbquYW7EurB
TLSHT15EC2B8CFBE31CAAAD5F4F632509F8B76D77B1435B2454A14B39C83201D13B845A2E9B2
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