Result for 15F2C4A7DAEA3E4727F1EAFDE9DC5779D34D3D84

Query result

Key Value
FileName./usr/lib/x86_64-linux-gnu/cpl/plugins/hawki-2.4.11/hawki_step_detect_obj.la
FileSize1033
MD5C5DA291CD3898A97D062CA581B3E5AAB
SHA-115F2C4A7DAEA3E4727F1EAFDE9DC5779D34D3D84
SHA-2560C71D1D1741146E16E900BC6D08AE93D9F93C4BB3C8CE6BB5B31445B9E670076
SSDEEP24:PeSHOWJU2icBxIY+Ahmfvi45vD2NGDe5/b1:luWJUzcBxIY1hmfKqLcb1
TLSHT15011C03FE3DE753AAFD4294596CF303E4289847947322E5063CB95DB224B81911A7E37
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
FileSize494108
MD502A3A726877552855F37063639962D69
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
PackageVersion2.4.11+dfsg-1
SHA-1F0C3B24956A696442FCB32E293471A377BAA1960
SHA-256B278D9B2C829C63930C1DD03871AC2A331689C9689B54528681565BE256BB13C