cpl-plugin-hawki-dbgsym 1.8.18+dfsg-5 (ppc64el binary) in ubuntu xenial

 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).