We present the design of the Michigan Infra-Red Combiner (MIRC). MIRC is planned for deployment at the Georgia State University CHARA array to simultaneously combine all six telescope beams in an image-plane combiner. The novel design incorporates spatial-filtering with single-mode fiber optics, a synthetic (densified) pupil, and a low-resolution spectrometer to allow good calibration and efficient aperture synthesis imaging in the near-infrared. In addition, the focalization and spectrometer optics can accommodate an integrated optics component with minimal re-alignment. The MIRC concept can be scaled-up for interferometer arrays with more telescopes
MIRC-X is a six telescope beam combiner at the CHARA array that works in J and H wavelength bands an...
Cophasing six telescopes from the CHARA array, the CHARA-Michigan Phasetracker (CHAMP) and Michigan ...
We describe the layout and unique features of the focal plane system for MIRI. We begin with the det...
The Michigan Infrared Combiner (MIRC) has been designed for two primary goals: 1) imaging with all s...
International audienceMichigan InfraRed Combiner-eXeter (MIRC-X) is a new highly sensitive six-teles...
Michigan InfraRed Combiner (MIRC) is a near-infrared image-plane combiner at the CHARA array which c...
Based on the success of four-telescope imaging with the Michigan Infrared Combiner (MIRC) on the CHA...
We report the first scientific results from the Michigan Infrared Combiner (MIRC), including the fir...
The CHARA Array possesses the longest baselines in the world for infrared and visible interferometry...
This is the final version of the article. Available from Society of Photo Optical Instrumentation En...
This is the final version of the article. Available from SPIE via the DOI in this recordMIRC-X is a ...
The very long baseline interferometer (VLBI) can achieve the highest angular resolution imaging of a...
This is the final version of the article. Available from SPIE via the DOI in this record.We present ...
An overview of integrated infrared (IR) array technology is presented. Although the array pixel form...
Long baseline optical inerferometers now have the power to resolve objects as small as 0.5 milliarcs...
MIRC-X is a six telescope beam combiner at the CHARA array that works in J and H wavelength bands an...
Cophasing six telescopes from the CHARA array, the CHARA-Michigan Phasetracker (CHAMP) and Michigan ...
We describe the layout and unique features of the focal plane system for MIRI. We begin with the det...
The Michigan Infrared Combiner (MIRC) has been designed for two primary goals: 1) imaging with all s...
International audienceMichigan InfraRed Combiner-eXeter (MIRC-X) is a new highly sensitive six-teles...
Michigan InfraRed Combiner (MIRC) is a near-infrared image-plane combiner at the CHARA array which c...
Based on the success of four-telescope imaging with the Michigan Infrared Combiner (MIRC) on the CHA...
We report the first scientific results from the Michigan Infrared Combiner (MIRC), including the fir...
The CHARA Array possesses the longest baselines in the world for infrared and visible interferometry...
This is the final version of the article. Available from Society of Photo Optical Instrumentation En...
This is the final version of the article. Available from SPIE via the DOI in this recordMIRC-X is a ...
The very long baseline interferometer (VLBI) can achieve the highest angular resolution imaging of a...
This is the final version of the article. Available from SPIE via the DOI in this record.We present ...
An overview of integrated infrared (IR) array technology is presented. Although the array pixel form...
Long baseline optical inerferometers now have the power to resolve objects as small as 0.5 milliarcs...
MIRC-X is a six telescope beam combiner at the CHARA array that works in J and H wavelength bands an...
Cophasing six telescopes from the CHARA array, the CHARA-Michigan Phasetracker (CHAMP) and Michigan ...
We describe the layout and unique features of the focal plane system for MIRI. We begin with the det...