Result for 0E54FCAA015B677698644FD5F700AEECD8E75860

Query result

Key Value
FileName./usr/lib/aarch64-linux-gnu/cpl/plugins/hawki-2.4.3/hawki_step_subtract_bkg.so
FileSize15088
MD5A62989AE8A20EF255472D208E6AFFB11
SHA-10E54FCAA015B677698644FD5F700AEECD8E75860
SHA-2564DF39B7E929C7C1C0855B9B21464745F1333DE6F03F75DD426DFFDB28C332C3F
SSDEEP192:2+G8DW2w1CvVBUOfJm6Ettyjlk3s4JnGwaxXJQK9lg+ZM3Q:1W2w1E+mF0tyxYs4lajQKg13
TLSHT1D862B586F698C83FD9E12379889F437CB352840DA32A5B83250D4B646F477BA5D3918F
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
FileSize470896
MD504E6CDD5BC92409B9B8ACCDBDA45598D
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
PackageVersion2.4.3+dfsg-1
SHA-11AB820B4CF5A53A38486A13C3E51A928A2FE694D
SHA-256F4E93FD2283238717114016AB9CA5CDBD1B98D37FDA6784152CB5222AD3B3867