Result for 16E70F6BDF8AC5AE6754F61F04C539F4E52A54B1

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabi/cpl/plugins/hawki-2.4.9/hawki_step_apply_dist.so
FileSize14432
MD5FF1E349AC793442EAD13AA4FC31D5B5B
SHA-116E70F6BDF8AC5AE6754F61F04C539F4E52A54B1
SHA-2562F0C008FB4C6734329BFDEBE451A58816A5C1544B879B145BF9BD445E08495BA
SSDEEP192:AUwdT8+ooO7oXc533pb1LfAlB4a3CS2wf2Q:bwdtooOMM53zLfg2i
TLSHT1D152648FF6A6CF67C0C13234319B0F1A5131859DC29B6753256D52983F192AECF16F8A
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
FileSize453352
MD55CFC0CB5C37652E14DA39B16073327E6
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-109AD28C108CC2A32C4F9E9E6E17CB27DA90FFD5E
SHA-2567A78D83C1E6E73EB9D53CA7D68B3C5EB49076AFE08652C402C0E2888B970DE64