Result for 2196C20B873E14F19327AC440CE05FE77966BD27

Query result

Key Value
FileName./usr/lib/mips-linux-gnu/cpl/plugins/hawki-2.4.3/hawki_science_postprocess.so
FileSize44508
MD5B3D4B6E043858895DF4B7771A81FF37A
SHA-12196C20B873E14F19327AC440CE05FE77966BD27
SHA-2566CECCCD0FD7F68A70253950326A06DF58E4C7CF5F4090FF50FC8C9DFF5E02531
SSDEEP768:PVXvHpq2w9ID/tEwpealYGfLn+aBWxkhLZjClt/IwSqy4EUFm0Y/CaUyo+IZytov:dXv3w9ID/tEwpealYGfLn+aBVVAt/IeR
TLSHT1EB13B86BA7104F4EF0E2C674F843CAE23570C06365C88663C47DFB253AD5B5AA82B657
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