Result for 0DE799C4EE1A0824AF7939E2082E3BE8316C4D36

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabihf/cpl/plugins/hawki-2.4.11/hawki_linearity_analyse.la
FileSize1048
MD53E943855CA38360993F8D4E93E82D257
SHA-10DE799C4EE1A0824AF7939E2082E3BE8316C4D36
SHA-2562576FC61250696645C9C151AF46780AD5745CBD2F57878225336CD627312B521
SSDEEP24:cDeSHOWJe9iUXXKxIY+Ahmfvi4ybvD2NGDe5/Ajy:cRuWJesUXXKxIY1hmfK/vLcAW
TLSHT16611423BE39A093A27E4074616CE346F47994079C3530E9C82CAA6DF3183929335BF22
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