Result for 015F7A3B3346A5D2D7811BB2525573B1967BC1A3

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabihf/cpl/plugins/hawki-2.2.0/hawki_linearity_analyse.so
FileSize22664
MD5EDCAC75C33C234EC09CDAF17DEE278FE
SHA-1015F7A3B3346A5D2D7811BB2525573B1967BC1A3
SHA-256456966F6DD1758233968A6AFB88FAD03446CADA85DF8921C4570CA04EE84123A
SSDEEP384:3IWzHewimcpDVG136yTSWEEOV8jOGdx3qH8Ml/JOr:YWzHew6xGZDPEEXjOG/k8Kxg
TLSHT142A2D5E7AC116977C0D49375246F8A8A72216BB0C3DF1B23904C4E243A9674E5F7BF4A
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
FileSize426848
MD5C8FC8B61CFE578FB387193CC0948C4CE
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
PackageVersion2.2.0+dfsg-1+b1
SHA-10D7A9C3BDB5386D1AD3C03E278B8A26A53117B63
SHA-256E99CF0D36C035AAC0C944D8858B13809B9E0F719118FEA0D5165C368314DEA9E