Abstract
Cophasing six telescopes from the CHARA array, the CHARA-Michigan
Phasetracker (CHAMP) and Michigan Infrared Combiner (MIRC) are pushing
the frontiers of infrared long-baseline interferometric imaging in key
scientific areas such as star- and planet-formation. Here we review our
concepts and recent improvements on the CHAMP and MIRC control
interfaces, which establish the communication to the real-time data
recording & fringe tracking code, provide essential performance
diagnostics, and assist the observer in the alignment and flux
optimization procedure. For fringe detection and tracking with MIRC, we
have developed a novel matrix approach, which provides predictions for
the fringe positions based on cross-fringe information.
Original language | English |
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Title of host publication | Optical and Infrared Interferometry III |
Subtitle of host publication | Proceedings of SPIE |
Publisher | SPIE |
Volume | 8445 |
ISBN (Print) | 9780819491466 |
Publication status | Published - 1 Jul 2012 |