The shaped pupil coronagraph for planet finding coronagraphy: optimization, sensitivity, and laboratory testing
Author(s) -
N. Jeremy Kasdin,
Robert J. Vanderbei,
Michael G. Littman,
Michael Carr,
David N. Spergel
Publication year - 2004
Publication title -
proceedings of spie, the international society for optical engineering/proceedings of spie
Language(s) - English
Resource type - Conference proceedings
SCImago Journal Rank - 0.192
H-Index - 176
eISSN - 1996-756X
pISSN - 0277-786X
DOI - 10.1117/12.552273
Subject(s) - coronagraph , apodization , pupil , exoplanet , sensitivity (control systems) , contrast (vision) , optics , throughput , computer science , planet , physics , electronic engineering , engineering , astronomy , telecommunications , wireless
This paper summarizes our work designing optimal shaped pupils for high-contrast imaging. We show how any eective apodization can be created using shaped pupils and present a variety of both one-dimensional and azimuthally symmetric pupil shapes. Each pupil has its own performance advantage and we discuss the tradeos among various designs. Optimizations are typically performed by maximizing a measure of system throughput under constraints on contrast and inner working angle. We mention the question of sensitivity to aberrations. Controlling aberrations will be critical for any implementation of a planet-finding coronagraph. Finally, we present our first laboratory results testing a shaped pupil coronagraph.
Accelerating Research
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom
Address
John Eccles HouseRobert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom