Result for 13F47EBE2DE6AA3ED57045745D8396AA8FA33583

Query result

Key Value
FileName./usr/lib/mips-linux-gnu/cpl/plugins/hawki-2.4.3/hawki_step_compute_bkg.so
FileSize23476
MD57CDCAABABAE9BEB456D04961F1C11179
SHA-113F47EBE2DE6AA3ED57045745D8396AA8FA33583
SHA-2561B82360B1C6CFD6D5C8970A9BEAD707C9543A9140F92D1FA96D5746754BFCA03
SSDEEP384:H1onq8/wo2DYPl9bo22RNRR7Kvqls4jQjSP7/GG+t0yi:HenB/wOMjRIdt67V
TLSHT1B7B2C94B23518E4DF1E2C3B4B15B86E611A025616EC54B63D4BDF0633588F1E783BEBA
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
FileSize471088
MD5B8FD83D2BD28D19D4560F9F25976C8F4
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
PackageVersion2.4.3+dfsg-1
SHA-11C8FE32120734D45F159CF07A89DF8F4AE4700E1
SHA-25633B192C73AF4F5B97638210C15508D770F5731F4969E5D34D0864DB81751A269