Result for 009E96BDECB0ACEB7310020423E7F37A4C6E1984

Query result

Key Value
FileName./usr/lib/mipsel-linux-gnu/cpl/plugins/hawki-2.4.9/hawki_step_subtract_bkg.la
FileSize1045
MD5151798B359990DBB9B29E85E7D3B6F6E
SHA-1009E96BDECB0ACEB7310020423E7F37A4C6E1984
SHA-2567B4D0CDFBA5D30B9B6D5D6FE32D875294073BE8C175A89EAF2EA67DF24A0D0F3
SSDEEP24:1eSG5WJEOiw5xIY+Ahmfvi4HvD2NGDe5/YS:3G5WJc2xIY1hmfKQLcYS
TLSHT1D511203A839A8125BAD40B5D8EDF303E429948790B2A4F1043C798DF128B43B1557E23
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
FileSize451748
MD5071B9F4695EF80D6D86B48ECB848BDB1
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-12EFAE4DCB62A49CB19F7510008CFF9C14342BE11
SHA-256ABAE21EFC2A432D5D37BD2D33604B5CE713A35277F7F34E80A7E278641E8009B