Result for 145ACB970CBF31EB095A8271D1F2326E532E19EB

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/cpl/plugins/hawki-2.2.0/hawki_util_gendist.so
FileSize18272
MD5266B843F8A439B56A7349D78D4DF8298
SHA-1145ACB970CBF31EB095A8271D1F2326E532E19EB
SHA-256F85FD368A807A49AF839FC2EE10DD937AB129FD1D2DD6A7B79B69B02EA61E407
SSDEEP384:4fBywxy/MUzggTjNltlCQANch6tSWy/4SJ7+Z5Nry:4fBywYPzfTRlHCQA6/Wy/85Nry
TLSHT15682B64EFA52E7F1C1C231F4640B063EAE608900F61BD7137A9C62C463526A8FB66739
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
FileSize510596
MD5C3A8598255D089A56D7555D54E939763
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
PackageVersion2.2.0+dfsg-1+b1
SHA-126EC7B533367155E98EE1068CED505920F9DD102
SHA-256AE2F773418C6EAFE9CB8230F334D27A87C21AD03F9D91B92A96859FA35E55D2F