Result for 0F7C5762352677D864A4D8D95CDBBFF8FE3C4647

Query result

Key Value
FileName./usr/lib/aarch64-linux-gnu/cpl/plugins/hawki-2.4.3/hawki_util_stdstars.so
FileSize10472
MD5F8BF2A081EA94C0ABDED39F51EBF257D
SHA-10F7C5762352677D864A4D8D95CDBBFF8FE3C4647
SHA-256AEE56E893B2594975299DC84B38501FACC54A1401AB1A162FA1B8B4DCA9A730F
SSDEEP96:x3HL7SM6BWBiSHwi7LEaiXjEl9OH1ZV6j2Pz2EyoHkKunrZtEGMwxvWWFq+ArVc5:tr7SM689HwWIh+yTsS6RWut4wxvdF5
TLSHT1DE226289BE449D3FC9D857B14C9B1B30B372DA8C9B29435B3908A3241F523DF0E6658E
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
FileSize470896
MD504E6CDD5BC92409B9B8ACCDBDA45598D
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-11AB820B4CF5A53A38486A13C3E51A928A2FE694D
SHA-256F4E93FD2283238717114016AB9CA5CDBD1B98D37FDA6784152CB5222AD3B3867