Result for 11A32D96C18FA8AA32E6860C44609C43D9BF0B3D

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/cpl/plugins/hawki-1.8.18/hawki_step_subtract_bkg.so
FileSize14428
MD5777E7379FF14B88A533E74E302482693
SHA-111A32D96C18FA8AA32E6860C44609C43D9BF0B3D
SHA-256ADF2279A7293901EDA6B44128B4320A65EE8E03332054E91519863316910A247
SSDEEP384:yQWx8v2M8ggTjNVGuE6y8DpM+AvA/AvAcATAZJ9so/g13A:1WSOM8fTRV9mceI4IvsZXscj
TLSHT104528403A7D2DFB5E1A22278118B072C95704520DE17CF43BD9C66D8A96539CBD233AB
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
FileSize221550
MD57CA8C8F751AC49CD58D14D76DA00B8B5
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
PackageVersion1.8.18+dfsg-4
SHA-1BA8CEACF21DD0E05B10A5C496CD082AD9365547E
SHA-256949029E1EA39C0BBA2A85405157D2B6E9179DF9FAFA1E585C720E7DE40B0B7D9