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A network of three longitudinally-spaced robotic imaging telescopes is described. So far planets have been
found only around bright stars (m < 1Om). Employment of the network and the photometric method for the detection of extrasolar planets will lead to the discovery of planets around stars of much fainter magnitudes
(m < 19m).
Charles H. McGruder III,Mark E. Everett,Steve B. Howell, andDavid P. Barnaby
"Detection of extrasolar planets via a network of robotic imaging telescopes", Proc. SPIE 4137, Instruments, Methods, and Missions for Astrobiology III, (29 December 2000); https://doi.org/10.1117/12.411611
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Charles H. McGruder III, Mark E. Everett, Steve B. Howell, David P. Barnaby, "Detection of extrasolar planets via a network of robotic imaging telescopes," Proc. SPIE 4137, Instruments, Methods, and Missions for Astrobiology III, (29 December 2000); https://doi.org/10.1117/12.411611