Result for 051F35E15CC057719CD37C572B9AA6AD984A8504

Query result

Key Value
FileName./usr/lib/mipsel-linux-gnu/cpl/plugins/hawki-1.8.21/hawki_step_photom_2mass.so
FileSize23096
MD56CBFE8047212AB9D46D3E4B6EAC311AD
SHA-1051F35E15CC057719CD37C572B9AA6AD984A8504
SHA-256CF3FCB43142933D4C5D388FF5FE28B9628A1822A6010D0E8E0EB0206053C35EB
SSDEEP384:7HS5Ol8fMwtWAbl6gsqmx1JSBpgJhzE0l7GDK9KuPLwcKcBknEGjZD08wIyUECHp:7y5Ol8fMwYWl6gsq01JSBpgJhzE0l7Gz
TLSHT10BA2B4B3AF541E07D5D1DD309C6FD910A0FF4E1CA29CE263F82DD8852A4AA691CF7948
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
FileSize227748
MD5B2ACC305E3A6F4603A32574AC2FA46EC
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
PackageVersion1.8.21+dfsg-1
SHA-1FAFAFF50844AC69EF126AC054E01E64C67733705
SHA-256129BF7506968CEB0DAF1299EEF863D41B29E5AA4EBA5505D0C3DBD8CAD911A64