Result for 1C96A697FA3B899323529284716083F55FAF9663

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabihf/cpl/plugins/hawki-2.4.3/hawki_step_subtract_bkg.so
FileSize10248
MD5B947FAE1B3D15F775C464D0A1D0D2F19
SHA-11C96A697FA3B899323529284716083F55FAF9663
SHA-25689EF3C90B99B28C14A80882B377057BB910891CE6F81F5BB3271BDE05FDB567F
SSDEEP192:iVotm+8mWNwdxXsdafP5TyFsxX5ANBhg+ZM3:6d4WNwdxXEaoazALhg13
TLSHT1052263CBE7E25A37D0D1363D59CF4E2C1764C4898A2B4F17154C22A43B122B98D6AE97
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
FileSize471024
MD5948CB92838A4404E1AA12023641CDAB5
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-12E3B1A4071995F103CF47F407CA4EF4591C36C9F
SHA-256382F8A1605747E26EE33758BD402E6C71DCB38950105E0EEF9E246951EF5205A