Result for 0E8E911E8D30DF8A3E8D0634AAB3F4ED2D649FE9

Query result

Key Value
FileName./usr/lib/mipsel-linux-gnu/cpl/plugins/hawki-2.4.8/hawki_step_subtract_bkg.la
FileSize1045
MD54786A739D9902A6A5EBA011B61E7493B
SHA-10E8E911E8D30DF8A3E8D0634AAB3F4ED2D649FE9
SHA-2568DEC3BDCFE6406190D345513F4350C83DF2F8CECF3F29E7808C500C4EA9634D0
SSDEEP24:1eSG5WJEOiw5xIY+Ahmfvi4HvD2NGDe5/Yr:3G5WJc2xIY1hmfKQLcYr
TLSHT14411F03A839A9125BAD40B5D8ADF703E429948790B2A5F1053C799DF128B43B1557E23
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