Result for 28BA7B384FE4DE7573613F30A7BDD5003630032B

Query result

Key Value
FileName./usr/lib/x86_64-linux-gnu/cpl/plugins/hawki-1.8.14/hawki_step_subtract_bkg.so
FileSize15216
MD557C55D3ADCD0E1E5EDD04B6E82A6B36F
SHA-128BA7B384FE4DE7573613F30A7BDD5003630032B
SHA-256499119D3D16F3D66F5F639068AF747CE8AD2867E3F7189EED07F4984E26FCA1E
SSDEEP192:RLPUfS+8pNWVwyPFLyvCyJdBHDxxkWqDDBg+ZM3Mw:ZUfSBW9FLyJ7jxOBg13
TLSHT16362C80BA6E1CE7DC1D4533890CB473499706885FB31DB171658A2B85E023AC4B2F7AB
hashlookup:parent-total1
hashlookup:trust55

Network graph view

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
FileSize195760
MD5AD2C0CE7BFA6DD0C55A03053260B56BB
PackageDescriptionESO data reduction pipeline for HAWK-I 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
PackageVersion1.8.14+dfsg-2
SHA-1086A952CA52A913571A4B157A2FACE4144827EDA
SHA-2562D7C4EE843C799609FC589F29F835C883F9AA2BE52375FA434E627D2452C14C0