Result for 13F54E2E47B71AD247FB0732081B0AA39D270BDF

Query result

Key Value
FileName./usr/lib/x86_64-linux-gnu/cpl/plugins/hawki-1.8.14/hawki_step_detect_obj.la
FileSize1036
MD5BA4A8C0B525E6F942E439F2EC423EBF3
SHA-113F54E2E47B71AD247FB0732081B0AA39D270BDF
SHA-2564F5BDDEDAC4E0B9743FDEA6D1C026D778760C30656199912BBBEED756EBFF79F
SSDEEP24:PeShuWJU2icBxIK+Ahmfvi45vD2NGDe5/bh:l8WJUzcBxIK1hmfKqLcbh
TLSHT19F110D3BD3DA713AAFD416458ACF303E42C5883907312E1063C785DB224B80911A7E27
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
FileSize235558
MD5B07F1716E526AC3171FDD3D19B6361F7
PackageDescriptionESO data reduction pipeline for HAWK-I 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
PackageVersion1.8.14+dfsg-2
SHA-1FF4A18E1FFAB4BD4D31FE1BE2C866401316953B6
SHA-256FF0CE99CD7E6398A4E477532FD9D5B3A7D05EA786069F1522624BC3E1B406AAA