Result for 1395E56AE3C63085C61632DDBC94F28DBB59E31A

Query result

Key Value
FileName./usr/lib/aarch64-linux-gnu/cpl/plugins/hawki-2.4.3/hawki_dark_combine.so
FileSize28136
MD52C1EAAA8FD3F6F19BFFC0C7956A23C24
SHA-11395E56AE3C63085C61632DDBC94F28DBB59E31A
SHA-256D6F5436E9C6D7A0ECC698EE8FE0CA48BE1BB50FC7179C4C807F8504FC4882618
SSDEEP384:+5sZfw0hwLA7tReQObAOVGrbpJWBm4Y+uA41:C+fw0T5RRZbpgs3F1
TLSHT1D3C2C6ADFF18C953C89BE23155CF1650F3225A88B13047A3756C0B1A2F4A7AE4D3E64E
hashlookup:parent-total1
hashlookup:trust55

Network graph view

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