Post-coronagraph wavefront sensor for Gemini planet imager

Proceedings of SPIE - The International Society for Optical Engineering

Volumn 7015, Issue , 2008, Pages

  Wallace, J Kent ^a   Angione, John ^a   Bartos, Randall ^a   Best, Paul ^a   Burruss, Rick ^a   Fregoso, Felipe ^a   Levine, B Martin ^a   Nemati, Bijan ^a   Shao, Michael ^a   Shelton, Chris ^a  

^a CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

Coronagraphy; Interferometry; Planet detection; Wavefront sensing

Indexed keywords

AMPLITUDE ERRORS; APODIZER; CALIBRATION WAVEFRONT SENSORS; COMMON PATH; CORONAGRAPHY; DIRECT DETECTION; HIGH CONTRAST; HIGH-ORDER; MITIGATE ERRORS; PLANET DETECTION; SLOW PHASE; WAVE FRONT SENSORS; WAVEFRONT SENSING;

ARCTIC ENGINEERING; CALIBRATION; ERRORS; IMAGE SENSORS; INTERFEROMETERS; INTERFEROMETRY; STARS;

WAVEFRONTS;

EID: 66949129941     PISSN: 0277786X     EISSN: None     Source Type: Conference Proceeding    
DOI: 10.1117/12.787258     Document Type: Conference Paper

References (4)

1. Bruce Macintosh, et. al., "The Gemini Planet Imager: from science to design to construction", Proc SPIE, Astronomical Telescopes and Instrumentation, these proceedings.
2. S. Shaklan and J.J. Green, "Low-order Aberration Sensitivity of eighth-order coronagraphic masks", ApJ, 628, 474-477 (2005). (Pubitemid 41273242)
3. R. Soummer, C. Aime, and P.E. Falloon, , "Stellar coronagraph with prolate apodization", A&A 397, 1161-1171 (2003).
4. Matthew C. Britton, "Arroyo", Proc. SPIE, Integrated Modeling of Extremely Large Telescopes, Vol.5497, 290 (2004)