The Michigan Infrared Beam Combiner (MIRC) combines the light from all six CHARA telescopes simultaneously. It disperses light across 8 spectral channels in the near infrared H-band (1.6 microns). It was developed by John Monnier and his optical interferometry group in the Astronomy Department at the University of Michigan. MIRC has produced the first images of a main sequence star other than the sun and has measured starpots on the surface of magnetically active stars.
MIRC Photometric Channels --- Che et al. 2010, SPIE, 7734, 2
MIRC 6T Combination --- Che et al. 2012, SPIE, 8445, 0