Result for 1C6306C56140CFC1240DE88AAC26E6DE49EE22FB

Query result

Key Value
FileName./usr/lib/s390x-linux-gnu/cpl/plugins/hawki-1.8.21/hawki_step_detect_obj.so
FileSize27864
MD53C261C8788F02C9C064D86FAA8295082
SHA-11C6306C56140CFC1240DE88AAC26E6DE49EE22FB
SHA-256AA17CEB7C89D542CEC9E64E56A68A34D1BBA4E42ACAD648636723D25C12ABF45
SSDEEP384:NcxJ3nwwWoOkHfA3+cPSk4WPLVjxDu2N9647tMyG:NcxJ3nwwWYBaVbxG
TLSHT1C7C2A4CFAE32A3E6D8F87731D54F8636977A4A31B3495A04B7BC83500E17F544A39862
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
FileSize220720
MD5E4E92A0B8190448093C1085FB0D1AB85
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
PackageVersion1.8.21+dfsg-1
SHA-15F53BAE9EC1154ED30C70C9E236D9A12E80D8EED
SHA-2567104AFD5FC486C6AD3216BF94DBBF5645F48AF5AA637F090A9BBBDD4D0A7C17C