Result for 1F66A0DE0E3B16C16D7E5C160880EFCBC18458A1

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/cpl/plugins/hawki-2.4.11/hawki_util_gendist.so
FileSize18404
MD59447A5C362F0A5A03A188165A1D33C36
SHA-11F66A0DE0E3B16C16D7E5C160880EFCBC18458A1
SHA-2562DC31961F9392AEECA29921BE89F792FE80ADE123FAA50C1F44F9EAEA4861D25
SSDEEP192:Ip8UVJBWg1af71XfzX3Qgc2EwjHtltlCUV3/bORPN9r3WTulSeol/Ox0sM8Wvqjv:IvfBWgkJvzggTjNltlCCOxjcTOx0UKV
TLSHT12A82D85FFA92D7F1E1C231F4240B073EAE718401F507C753BA5C2285AA925E8FB2A756
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
FileSize527876
MD51EDF8496263A6ADC7FA6A5315429C69F
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
PackageVersion2.4.11+dfsg-1
SHA-1B819EEA56280AD4ABCC44E5D419874F364EF861F
SHA-256591F4DC68AFEC363D198CBB54130A8FFCC76FF7F0F3FEE4034C8C6347C8CD4E0