Result for 140CE62BD7DDCEE9A6AD274318625E80058A9C34

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/cpl/plugins/hawki-2.4.3/hawki_step_subtract_bkg.la
FileSize1044
MD5DF9AFAEB18CB06596BD3CA8645D8A5FB
SHA-1140CE62BD7DDCEE9A6AD274318625E80058A9C34
SHA-256A93D5B50D1F0EFE16241592ABE7C55853D656BA5B42E81ED4B3B800680146B3A
SSDEEP24:1eSGsWJEOiw5xIY+Ahmfvi4HvD2NGDe5/o0:3GsWJc2xIY1hmfKQLco0
TLSHT13911203A839B9125BAD40B5D8ACF303E429948790B265F0053C798DF128B43B1567E23
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
FileSize548756
MD57B774D5D5C690C1AD50BAFC43FDDB0C4
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-1B6C87AC7CEF51846AD1962434E51181D948F75F9
SHA-2564BB11E9B6BA556172558877F98E9B23702C96254E0C6CD3DF42D3C2B65C795F7