The CHARA Michigan Phase-tracker (CHAMP) is a real-time fringe tracker for the CHARA Array, a six-telescope long baseline optical interferometer on Mount Wilson, California. CHAMP has been optimized for tracking sensitivity at J, H, or K bands and is not meant as a science instrument itself. This ultimately results in maximum sensitivity for all the science beam combiners that benefit from stabilized fringes. CHAMP was designed, built, and tested in the laboratory at the University of Michigan and will be delivered to the CHARA Array in 2008. We present the final design of CHAMP, highlighting some its key characteristics, including a novel post-combination transport and imaging system. We also discuss testing and validation studies and pres...
The CHARA Array is the longest baseline optical interferometer in the world. Operated with natural s...
This is the final version. Available on open access from SPIE via the DOI in this recordData, Materi...
International audienceMichigan InfraRed Combiner-eXeter (MIRC-X) is a new highly sensitive six-teles...
The CHARA Michigan Phase-tracker (CHAMP) is a real-time fringe tracker for the CHARA Array, a six-te...
We present the design for a near-infrared (JHK) fringe tracker to be used at the CHARA Array, a long...
The CHARA-Michigan Phasetracker (CHAMP) successfully tracks fringes in 4-telescope and 6-telescope m...
Cophasing six telescopes from the CHARA array, the CHARA-Michigan Phasetracker (CHAMP) and Michigan ...
Based on the success of four-telescope imaging with the Michigan Infrared Combiner (MIRC) on the CHA...
The Michigan Infrared Combiner (MIRC) has been designed for two primary goals: 1) imaging with all s...
The CHARA Array is the longest baseline optical interferometer in the world. Operated with natural s...
This is the final version. Available from SPIE via the DOI in this recordSPIE Astronomical Telescope...
The CHARA Array is a six telescope optical/IR interferometer run by the Center for High Angular Reso...
This is the final version of the article. Available from Society of Photo Optical Instrumentation En...
International audienceThe CHARA array is an optical/near infrared interferometer consisting of six 1...
The CHARA Array is the longest baseline optical interferometer in the world. Operated with natural s...
This is the final version. Available on open access from SPIE via the DOI in this recordData, Materi...
International audienceMichigan InfraRed Combiner-eXeter (MIRC-X) is a new highly sensitive six-teles...
The CHARA Michigan Phase-tracker (CHAMP) is a real-time fringe tracker for the CHARA Array, a six-te...
We present the design for a near-infrared (JHK) fringe tracker to be used at the CHARA Array, a long...
The CHARA-Michigan Phasetracker (CHAMP) successfully tracks fringes in 4-telescope and 6-telescope m...
Cophasing six telescopes from the CHARA array, the CHARA-Michigan Phasetracker (CHAMP) and Michigan ...
Based on the success of four-telescope imaging with the Michigan Infrared Combiner (MIRC) on the CHA...
The Michigan Infrared Combiner (MIRC) has been designed for two primary goals: 1) imaging with all s...
The CHARA Array is the longest baseline optical interferometer in the world. Operated with natural s...
This is the final version. Available from SPIE via the DOI in this recordSPIE Astronomical Telescope...
The CHARA Array is a six telescope optical/IR interferometer run by the Center for High Angular Reso...
This is the final version of the article. Available from Society of Photo Optical Instrumentation En...
International audienceThe CHARA array is an optical/near infrared interferometer consisting of six 1...
The CHARA Array is the longest baseline optical interferometer in the world. Operated with natural s...
This is the final version. Available on open access from SPIE via the DOI in this recordData, Materi...
International audienceMichigan InfraRed Combiner-eXeter (MIRC-X) is a new highly sensitive six-teles...