Result for 05574A6E653A8F878C13A269A7AC0E13DDB906FA

Query result

Key Value
FileName./usr/lib/powerpc64le-linux-gnu/cpl/plugins/hawki-1.8.14/hawki_util_stdstars.so
FileSize10216
MD53ACF5A8CC3B19B8909030F46086A184F
SHA-105574A6E653A8F878C13A269A7AC0E13DDB906FA
SHA-256656662146D7E4CFB7DB75861BEE724C2D5B47BE77D6A8F1193BBB1D67B753107
SSDEEP96:TlDUZBWBPJx7XTxgsHjP02lB5p3utinpMZkvEeeTN9K7ajkKISqx+p8Mil+qI:WZ8p/XT3H42lB5p3duZk9eRRY+uMj
TLSHT1762262A3767D9E6FD7C4223B599F03703321AF4203510317561853193F8A7AE8F7A986
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
FileSize191810
MD5F94E1EDE633CCEDCBE31E09724D85AA3
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).
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion1.8.14+dfsg-2
SHA-1DC1833126CD4314E1C140EAE317204641EC0C86B
SHA-25687DAF936BC5231E6477B366A7A32736D2E8ECF099140D10468051527FE345A49