Result for 1725BD2B260A9FE7DFE142FD72A7ED76524D460F

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabi/cpl/plugins/hawki-2.4.11/hawki_step_subtract_bkg.la
FileSize1046
MD5F4A27EBC839BE0FF47CFAE0F6A44C0F4
SHA-11725BD2B260A9FE7DFE142FD72A7ED76524D460F
SHA-256B794BA0EEDEB67A75E19AD0BF71658DDC8E8965C96A8EF565880AB9D7A6877CC
SSDEEP24:1eSHOWJEOiw5xIY+Ahmfvi4HvD2NGDe5/AjI:3uWJc2xIY1hmfKQLcAk
TLSHT1B011203AC3DB8525BAD4065D8ADF703E425948790B274F1043C798DF128B42B115BE23
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
FileSize460432
MD5C4C5EBB37D7DBB8298549F3C6954D382
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
PackageVersion2.4.11+dfsg-1
SHA-1CD3572D24E59B9C5CC2677F15ACDA24FFDA85C4C
SHA-2564ACCFB4EC42FBCD04415B3421FF1F11B47DE7CE1669F475BEC1727F12E938654