Result for 0B274ED4992591A9E2F46B429B3EE6276E745C3B

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabi/cpl/plugins/hawki-1.8.21/hawki_step_photom_2mass.la
FileSize1048
MD5B4E05B2CB744D80243FA7D26E0B4094D
SHA-10B274ED4992591A9E2F46B429B3EE6276E745C3B
SHA-2567DC9061C5ACF256FBE19642781475998C9B11257E54DFE59AFD5F8F2332A7673
SSDEEP24:ueSGWWJNmifRxIY+Ahmfvi4qvD2NGDe5/Ajsn:mGWWJNZxIY1hmfKPLcAA
TLSHT15911423BC39A052AAFE405466E8F347F43898539037E2E0442C7C4EF220B42932A6E22
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
FileSize228074
MD5CE29F2691A6DA88FF83D73C679596827
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
PackageVersion1.8.21+dfsg-1
SHA-1FFAB13A4EB060F369871AD9885635F1D6BDEAB73
SHA-2568D0D52E213F4C1B1787D5035FF57338A5A51EE8C5F408362A01B3492A2590DA5