Result for 17E5F9F2133BAE4EC9B8BF8ED53E3054895DD7DB

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabihf/cpl/plugins/hawki-2.4.11/hawki_step_subtract_bkg.so
FileSize67732
MD511B97E70398E9C492617A600E1325081
SHA-117E5F9F2133BAE4EC9B8BF8ED53E3054895DD7DB
SHA-256655AE62FA72FDBB5B84534ECB2CA773B6A00A1D26C397380E130D535F9931830
SSDEEP96:sR4ZDEBWBRmWlYVs4DNpgNCriI8AY1G+1BVf8xAq89fzc2L+ZM3C4nz4y2O/:cKo8mWuppgNWiu5AfUxmdzcg+ZM3C4P
TLSHT1C36395CBBBD35F5FD8C12738584F0F28562187A9DB178F33995C40F01D02AE9892AAD6
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
FileSize451432
MD5806CB6A07D053F721A8E675196114EB6
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-1D4EE6BE1F295CE3F05E675E4F234B3A20BF3B199
SHA-256E2F48D24F4D2E931655F871957B4718228B438460887A47BEAC55B6C6D323744