Result for 10E33F41A37DDFD2FA48C47D3AA7C001D43EC783

Query result

Key Value
FileName./usr/lib/mipsel-linux-gnu/cpl/plugins/hawki-2.4.8/hawki_detector_noise.so
FileSize19228
MD5B955AC99905B0AFA0A4E976823132B0A
SHA-110E33F41A37DDFD2FA48C47D3AA7C001D43EC783
SHA-256F023FB176D327EEE6F6C70A59937041F34B62C9B313C158502F5F18A2A628021
SSDEEP384:rtverAZnaO7rrEPPbYiTcRVASGmPPea9sl6nEiIKAa0CdyxoQbdwEgH45v0ht1cd:RverAZaO7rrEPPbYiTcRVASGmPPea9sJ
TLSHT18C825167AF141E57D8C2DC71189FC24292BF8E4DF198EA03E11DD9842707B4C6EABA4D
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
FileSize451824
MD51F48F63051D9F44902CAF24A014F7EA7
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
PackageVersion2.4.8+dfsg-4
SHA-11F8850C8DF01377F7D9588E80BA2C9DB502D4044
SHA-2560A8C64809D35D4085A35B94D11899977427986C005708D095B5B089F504E52EE