Result for 11250B61DCAE3EE1E8B5A8E6E05F11C06D8A8271

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabihf/cpl/plugins/hawki-2.4.3/hawki_step_detect_obj.la
FileSize1037
MD589360AD2614B3080BB3347F6E498341F
SHA-111250B61DCAE3EE1E8B5A8E6E05F11C06D8A8271
SHA-2566D0AAB599A784F0BAF2FAC08F209E6FDC646CF29F831DAADDB05DBF5DFEA732B
SSDEEP24:PeSGsWJU2icBxIY+Ahmfvi45vD2NGDe5/Ajd:lGsWJUzcBxIY1hmfKqLcAp
TLSHT13B11C03FD3DE753AAFD4154596CF303E42C9887907312E5063C795DB224B81911A7E27
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
FileSize471024
MD5948CB92838A4404E1AA12023641CDAB5
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-12E3B1A4071995F103CF47F407CA4EF4591C36C9F
SHA-256382F8A1605747E26EE33758BD402E6C71DCB38950105E0EEF9E246951EF5205A