Result for 138DAFCEB732205C7B2CA366FCA9F4B0435B7CB0

Query result

Key Value
FileName./usr/lib/mipsel-linux-gnu/cpl/plugins/hawki-2.4.9/hawki_step_compute_bkg.la
FileSize1039
MD5CED6599740E1AEEEF6F8E9E67CA8D1D5
SHA-1138DAFCEB732205C7B2CA366FCA9F4B0435B7CB0
SHA-25665F1DA88ECAC16765EA66E8C15782EB81FA5504294B0C94B63FA480B7EBBCF91
SSDEEP24:0ReSG5WJmyOicJJy5xIY+Ahmfvi4C1vD2NGDe5/YS:0LG5WJmmcJJwxIY1hmfK7pLcYS
TLSHT13111E23A93C95125ABE04A865B9F303F428B487C07266E6052C7D9FB114B82B3156F22
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
FileSize451748
MD5071B9F4695EF80D6D86B48ECB848BDB1
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
PackageVersion2.4.9+dfsg-1
SHA-12EFAE4DCB62A49CB19F7510008CFF9C14342BE11
SHA-256ABAE21EFC2A432D5D37BD2D33604B5CE713A35277F7F34E80A7E278641E8009B