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Coronagraphs are bandwidth limited. BLOCT takes the approach of "divide and conquer" with a front end that is dispersive. Wavelengths are addressed in exquisitely narrow bands using a process of double dispersion. First the wavefront is broken into a spectrum and then it is collimated. A matched pair of wavefronts that have been split form the basis of a long baseline interferometer. Notably this telescope draws from the entire history of astronomical optics. The initial afocal mirror telescope is a Mersenne (1636). The double dispersion traces its roots to Newton's Dual Prism Experiment (1666). The division of light into its spectrum by diffraction was first demonstrated by Rittenhouse (1785). The division of star light into wavelengths derives from von Fraunhofer (1819). The ruled plane grating was developed by Rowland (1880). The interferometric beam splitter and resulting beat pattern was developed by Michelson who measured the diameter of Betelgeuse on the Wilson telescope (1920).
Thomas D. Ditto,Heidi J. Newberg, andLeaf Swordy
"BLOCT: the bifurcated light optical coronagraphic telescope", Proc. SPIE 12680, Techniques and Instrumentation for Detection of Exoplanets XI, 1268029 (5 October 2023); https://doi.org/10.1117/12.2676842
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Thomas D. Ditto, Heidi J. Newberg, Leaf Swordy, "BLOCT: the bifurcated light optical coronagraphic telescope," Proc. SPIE 12680, Techniques and Instrumentation for Detection of Exoplanets XI, 1268029 (5 October 2023); https://doi.org/10.1117/12.2676842