Result for 0E39004C98CDF8DF6FEB2EA9BA7AE3E7496ACBE5

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/cpl/plugins/hawki-2.4.9/hawki_util_stdstars.so
FileSize14072
MD50DA9F9AA86F85E91705AF98CD9685CF1
SHA-10E39004C98CDF8DF6FEB2EA9BA7AE3E7496ACBE5
SHA-25639C5D267FB9BF91C8111D116B1F683E1C39342A3825B4C69E490A340BFBC1D6E
SSDEEP192:wWP8Gymt+S+HTX3Qgc2E31xk/zXYfRtyv2L+PqtcZej:wWRySogg0bkGXyv2L+i
TLSHT12752C65BBB85D8B2E2D552B4941BC33CC271843197A3C7237E48239C2D36BD8D9163AA
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
FileSize524536
MD53FC8B3C34A65DF11F4044DD0DED779E6
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
PackageVersion2.4.9+dfsg-1
SHA-170C4037CF07C67D800F6A6916A4412B35AFD6356
SHA-256A4615C80DE8B1365075BBBC5B4DEDF45435016BCDC59F1DE203D83F86568C5FA