Result for 02058622F1E0C6FE367C1219822560E076FD065E

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabi/cpl/plugins/hawki-2.2.0/hawki_step_detect_obj.la
FileSize1033
MD5029EE5223DFF8242D3C52B6F5BA462EB
SHA-102058622F1E0C6FE367C1219822560E076FD065E
SHA-256643CD0C6E4C7AAB833EC3DECF73D1EAC276D56598AE39A376EAA8D675C46AC4A
SSDEEP24:PeSG1bWJU2icBxIY+Ahmfvi45vD2NGDe5/AjO:lGVWJUzcBxIY1hmfKqLcAK
TLSHT18711F03FD3DD317AAFD4154596CF303E4289887907322E5063C784DB224B81911A7E27
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
FileSize442062
MD5E779873E6D359675CEDBC17AC57E9320
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
PackageVersion2.2.0+dfsg-1+b1
SHA-13C5CD869CACE89525DD780CA8081A8C6802AEDE3
SHA-256EB202A58AA0E86581745FF06F55E29A9F37826AF733B571458392DCD61AAD19D