Result for 1D97AA23F1F85BC4DC9669F8DB720D4D8D474FB4

Query result

Key Value
FileName./usr/lib/x86_64-linux-gnu/cpl/plugins/hawki-1.8.18/hawki_tec_filtchk.so
FileSize10728
MD573D5EC14F1E42A35450148FD9F5616BC
SHA-11D97AA23F1F85BC4DC9669F8DB720D4D8D474FB4
SHA-2567CCCDF4249D0F48DCA1EF475B3213750E3084577675A10558E4EA89DB1A38A39
SSDEEP96:RTyJTBWBPh3wXE1m0eOhb6nTYbDY6/JNYuEHUZfhK6qQV+iSiA08j:RTy18phIE11hyTYbDY6/JWucU1wDQsi
TLSHT1D122A64BB2A8DD7AC4D86334509B427536B05850EF20CB1B354869B8AD03B9C477BFAF
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
FileSize199012
MD5B01C49B7C03387D9F4FEB6040374C806
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-5
SHA-13471E1B68664943242AD6077ADE94A6DCD742EE6
SHA-256318E3CDF027B1088E2BD10A59D696200CE37664D96E4CE2F5D0C6A0BDC7F1631