Planet detectability by an adaptive optics stellar coronagraph

• 1 April 1994
• journal article
• Published by American Astronomical Society in The Astrophysical Journal
• Vol. 425, 348
• https://doi.org/10.1086/173990

Abstract

Keywords

• MONTE CARLO SIMULATION
• EXTRASOLAR PLANET
• POINT SPREAD FUNCTION
• INFRARED
• SIGNAL TO NOISE RATIO
• MONTE CARLO METHOD
• DETECTION LIMIT
• SYSTEM PERFORMANCE
• NEAR INFRARED
• PLANETARY SYSTEMS
• ADAPTIVE OPTICS