Result for 0EC15D80B5CA0D4AC50380D411907D2FD891AD51

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabi/cpl/plugins/hawki-1.8.21/hawki_step_compute_bkg.so
FileSize22956
MD5486281A1E83705FDA03E54DE00AFE523
SHA-10EC15D80B5CA0D4AC50380D411907D2FD891AD51
SHA-256364511C8F26BE2F62B0370280F271328A44A23ABEB535D5B6F9AD19B9B0997E5
SSDEEP384:IcXQnB8swHRuUzJvJX5Gtz/81Z4yaP2fUVMjsH5kIOj4P7/GGfl0yx:Icgn+swX5eb83k7Zvoc7n
TLSHT148A2E8E7B4C27B37C5C02376325F8F0612221FB4869F6B23548C48745A22B6F9D76E4A
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