Result for 00E3D00E497C3A3BF25D0CD11BDE47D5A3BAB77F

Query result

Key Value
FileName./usr/lib/x86_64-linux-gnu/cpl/plugins/hawki-2.2.0/hawki_linearity_analyse.so
FileSize27808
MD5B639991FDD479DD559498579F2464527
SHA-100E3D00E497C3A3BF25D0CD11BDE47D5A3BAB77F
SHA-2561EF96553B90DE97F2C14E00E7C001810F3E5EAB49B929C30587ABE8318F23F67
SSDEEP384:mRcHzHewMtszPE8NAO/pZ4IGqjHunNDi:GcHzHewCKM8dFjHQNDi
TLSHT112C2098FEA7189BEC0D0D73018CF64239A747655E630932F138462727B45B68572FB6B
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
FileSize479446
MD505163626569370830CB4BA3492E0B092
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-1CEDE6337214FC45AF5F212D7F8B8F84CD8EDCD55
SHA-25689D9D055F1AB77CD76E039FA4BC12C013BD5702025C1FA292279C2316B1D1BB8