Nanometer-level path-length control scheme for nulling interferometry

Applied Optics

Volumn 38, Issue 19, 1999, Pages 4213-4216

  Serabyn, E ^a  

^a CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0001138241     PISSN: 1559128X     EISSN: 21553165     Source Type: Journal    
DOI: 10.1364/AO.38.004213     Document Type: Article

References (7)

1. R. N. Bracewell, “Detecting nonsolar planets by spinning infrared interferometer,” Nature 274, 780-781 (1978).
2. M. Shao and M. M. Colavita, “Long-baseline optical and infrared stellar interferometry,” Ann. Rev. Astron. Astrophys. 30, 457-498 (1992).
3. N. Woolf and J. R. Angel “Astronomical searches for Earth-like planets and signs of life,” Ann. Rev. Astron. Astrophys. 36, 507-537 (1998).
4. C. A. Beichman, “A roadmap for the exploration of neighboring planetary systems,” JPL Rep. 96-22 (Jet Propulsion Laboratory, Pasadena, Calif., 1996).
5. M. Shao, “Hubble extra solar planet interferometer,” in Space Astronomical Telescopes and Instrumentation, P. Y. Bely and J. B. Breckinridge, eds., Proc. SPIE 1494, 347-352 (1991).
6. D. J. Diner, E. F. Tubbs, S. L. Gaiser, and R. P. Korechoff, “Infrared imaging of extrasolar planets,” J. Br. Interplanetary Soc. 44, 505-512 (1991).
7. P. Baudoz, J. Gay, and Y. Rabbia, “Interfero-coronagraphy: a tool for detection of faint companions,” in Vol. 134 of the ASP Conference Series, Brown Dwarfs and Extrasolar Planets, R. Rebolo, E. L. Martin, and M. R. Zapatero Osorio, eds. (Astronomical Society of the Pacific, San Francisco, 1998), pp. 254-261.