Result for 19DBDFAA331C39F24C733EFBD12F5A0DEE555FF6

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabi/cpl/plugins/hawki-2.2.0/hawki_dark_combine.so
FileSize27104
MD5134B038A1310BD67B0F42621700DB226
SHA-119DBDFAA331C39F24C733EFBD12F5A0DEE555FF6
SHA-2565A2DD14B75A262ADA856EC2352B7563D383BC52F5B2E291D0F074D5A5B9D95EB
SSDEEP384:05HUF9wu8l9GmdIgm3t3cxbE4Jdl7UTLsvs3MHYyF9lr:05HK9wR9ddIgmSbE4YY6GYyJ
TLSHT11BC229C6B9624F97C4C0A731225F0B09726157B4E39E2303528C4DA63B86A5D5D3BFBE
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
FileSize442062
MD5E779873E6D359675CEDBC17AC57E9320
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
PackageVersion2.2.0+dfsg-1+b1
SHA-13C5CD869CACE89525DD780CA8081A8C6802AEDE3
SHA-256EB202A58AA0E86581745FF06F55E29A9F37826AF733B571458392DCD61AAD19D