Result for 2258567CBF13B38FBBE501F66A529A4B20E85B99

Query result

Key Value
FileName./usr/lib/aarch64-linux-gnu/cpl/plugins/hawki-1.8.21/hawki_cal_dark.so
FileSize23656
MD5B0401860229CBDEA6A42C57A58BA9169
SHA-12258567CBF13B38FBBE501F66A529A4B20E85B99
SHA-2568476EA59A1F69E56C1B7EDE8FF7401F77AFC1200642D5832D8B603C2B1E8A45B
SSDEEP192:qZwTgP8p9cUgwdTGAtEX1hxbZQ6IZRFaW6H1vV1f2WrJobvvvJAFUFSxw9dabhIR:UUgwdTFEli60/kV1AbvDSF6L
TLSHT1A4B2B7B8F60C9A2FCC91F7B9599F1B70B25405446718CB83754C09E46F493AECE3A98E
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
FileSize203830
MD50217B24BC288D83D67B33CC086B6DC72
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
PackageVersion1.8.21+dfsg-1
SHA-1A3D2F47DDC44170E6E18F65F24ECF6BC5365A200
SHA-2568BAD397247F133240BFF3538BA243E921F9D81B6F302F0F295AE0F28FE15DF22