Result for 03A1FF0A21D3FB46A3DDCDAB08454B674046E5BD

Query result

Key Value
FileName./usr/lib/x86_64-linux-gnu/cpl/plugins/hawki-1.8.21/hawki_step_subtract_bkg.so
FileSize15248
MD50E161E93E62A48FE636905B57190A491
SHA-103A1FF0A21D3FB46A3DDCDAB08454B674046E5BD
SHA-256F6CB50AA2682691FBDAC56484390006F8F9832F2F12C07EF75496892ECE888E3
SSDEEP192:RGJEfSy8pNWV4+Fje1e5CozMgCo5f0BHDxx0OUvoDqg+ZM3yZi:4JEfS1WRFjFd/C4fGjxlqg13y
TLSHT10262C60BA7A5DD7EC4E4533884CB0234A970A885FF25DB17255C64B54E027AC4B3F7AB
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
FileSize200196
MD555DAFFDB7A8ADAEB25B360D7AD3A2159
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).
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion1.8.21+dfsg-1build1
SHA-15604971B6C39DB285290AA6F1E48D23EE6AEBB28
SHA-256104611200EAA2B4F7482B543F9B2A05BC611FD705EDF92FD5DD80228BAA3DB55