Result for 1E3AC73C38944C0E7320354A1A1370FF699C5B7B

Query result

Key Value
FileName./usr/lib/mips64el-linux-gnuabi64/cpl/plugins/hawki-2.4.9/hawki_science_postprocess.la
FileSize1064
MD5797ED3367EB1F19764627B12019123B3
SHA-11E3AC73C38944C0E7320354A1A1370FF699C5B7B
SHA-25699D4C67B1F29D4D07F984B429EACAA448B5C0F364A8CAB68E6B74840647F9FEE
SSDEEP12:JHK4fWgxGb/r5WFKmH3LiBH1W1WoxIha+AAmBB7Szf77ixCF7tvT3RTZ/9IMCKbO:TeSG5WJ7icxIY+Ahmfvi45vD2NGDe5/5
TLSHT13011DDF6C3C95D7A6BD01945A6CE302F4A8A843C0B190A3493C6E5EB278742A1157E3B
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
FileSize432820
MD5C12CBBEF48D8105D146F3F56E4FC6A80
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
PackageVersion2.4.9+dfsg-1
SHA-1E41BD0569D8F9C390A871D226FEBCF087EAA5725
SHA-2561645C1BA99874DEA41DB29C0692F68499585F6E8E7C1FA36686DA058B91EFAFC