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Package: cpl-plugin-hawki (2.4.6+dfsg-1build1)

ESO 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).

Other Packages Related to cpl-plugin-hawki

  • depends
  • recommends
  • suggests
  • dep: libc6 (>= 2.29)
    GNU C Library: Shared libraries
    also a virtual package provided by libc6-udeb
  • dep: libcplcore26 (>= 6.3)
    Fundamental CPL data types and functions
  • dep: libcpldfs26 (>= 6.0)
    CPL functions for Data Flow System compatibility
  • dep: libcpldrs26 (>= 6.4)
    CPL higher level data processing algorithms
  • dep: libcplui26 (>= 6.4)
    CPL framework interface library
  • dep: libgcc-s1 (>= 3.0) [amd64]
    GCC support library
    dep: libgcc-s1 (>= 3.5) [armhf]
  • dep: libgomp1 (>= 4.9)
    GCC OpenMP (GOMP) support library
  • dep: libgsl23 (>= 2.5)
    GNU Scientific Library (GSL) -- library package
  • dep: libstdc++6 (>= 4.1.1) [amd64]
    GNU Standard C++ Library v3
    dep: libstdc++6 (>= 4.3.0) [armhf]
  • rec: esorex
    Execution Tool for European Southern Observatory pipelines
    or python3-cpl
    Control pipeline recipes from the ESO (Python3)

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Download for all available architectures
Architecture Package Size Installed Size Files
amd64 432.1 kB1915 kB [list of files]
armhf 391.6 kB1328 kB [list of files]