Result for 050E50B17AE66E693BDF2F5B833DCB63D4073D6F

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabi/cpl/plugins/hawki-2.2.0/hawki_sci_jitter.la
FileSize1003
MD5B885A9FA668D1262EA16F71772F00C55
SHA-1050E50B17AE66E693BDF2F5B833DCB63D4073D6F
SHA-256567F38D8A9138E35010F30E83EF01C3EF9E5217ADB6E35F47BCAA64BC4A10DBF
SSDEEP24:neSG1bWJniaxIY+Ahmfvi431vD2NGDe5/AjO:NGVWJiaxIY1hmfKSpLcAK
TLSHT1EE11327BC3DA89277BD40E4546CE382F428AC83D0B620E5052CEC5DB6247C1EA167F2B
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