Result for 21B6364CF5D939E94B0A8DCE0BFDECE3495DD988

Query result

Key Value
FileName./usr/lib/mips-linux-gnu/cpl/plugins/hawki-2.4.3/hawki_sci_jitter.so
FileSize44512
MD5067978A168CCEF3982FCEEAD4EA1D41D
SHA-121B6364CF5D939E94B0A8DCE0BFDECE3495DD988
SHA-2566789D0CD2F243BAD1DE91C6D2552080F004383F87CEA7C3113745DE19C8CFDA7
SSDEEP768:p6tNwrYKWULkoJf0giiuFgUd3hfYZbrHVHn8cKSXonr52egkh9uIqPy:wTwEKWGko+ggdRwtpcuXzp3y
TLSHT15C13C86B63608F2EF0D2C1B8B81789E224B350A262E48553D07DF11539C5F6AE737A1F
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
FileSize471088
MD5B8FD83D2BD28D19D4560F9F25976C8F4
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
PackageVersion2.4.3+dfsg-1
SHA-11C8FE32120734D45F159CF07A89DF8F4AE4700E1
SHA-25633B192C73AF4F5B97638210C15508D770F5731F4969E5D34D0864DB81751A269