Result for 075A41B4B7CD7D455EE9C80316195C9BA23DA782

Query result

Key Value
FileName./usr/lib/powerpc64le-linux-gnu/cpl/plugins/hawki-2.4.3/hawki_dark_combine.so
FileSize69136
MD5D481C01412B4BF8C4DA72D5D5914D6AB
SHA-1075A41B4B7CD7D455EE9C80316195C9BA23DA782
SHA-2568F3AFF655E59F9276A6928C1D7B6667022FBC217A02DB7092F58EECE0B76BFC1
SSDEEP384:1CAFfwkMsMqVHl3Dk67BmBhS2YxWCBHemJ01zDqVid45tVDu+JGp:1CWfwkMsM4FTk8XWy+31zDpz
TLSHT17A63B7A3772D6B09DF51E035D1FE1531B2A26E0F47304303A914932A2EDAB1C8B25E5B
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
FileSize547580
MD5B18CA767A1199AA5AF489CE17CD7BB65
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
PackageVersion2.4.3+dfsg-1
SHA-1F236FEA9C8FD567B3682BBF6658FCD7300D6B0E0
SHA-256F686E8D97B34E3D32A5A43F84F58708D1760617E24A4B37F15023F1F5FB5E51F