Result for 14F18BF7CD8ADFE622BF3CC6D65C8CDDE5C0E902

Query result

Key Value
FileName./usr/lib/aarch64-linux-gnu/cpl/plugins/hawki-2.2.0/hawki_cal_flat.so
FileSize36800
MD5AD5CB745CC397B83CB91B775B41AA1BA
SHA-114F18BF7CD8ADFE622BF3CC6D65C8CDDE5C0E902
SHA-256BA02F2D0294B79475D96AC7A703E68ABE66711206FB31377B10F2CB988D4FC3B
SSDEEP768:jb60G+UwX9EdMx3hB6oLTnwF6bGx/EomaYUZ:j+0QwudMFh5L726bLa7Z
TLSHT1A4F2F9DDEB2DA937C996773D1DDE4768B1112E89A211CFC2216F80485B8077E8C3A5CE
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
FileSize412076
MD508B3CE36677FB07D89A49E60A807357C
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
PackageVersion2.2.0+dfsg-1+b1
SHA-1EDDFA8E4D2940474F63B25AC9BDAB2C9340BD1C7
SHA-256F5CDE157AB1385847031F916C70B8A0015D5F3794F32164E289FACCEFEA462DA