LOWER LIMITS ON APERTURE SIZE FOR AN EXOEARTH DETECTING CORONAGRAPHIC MISSION
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[1] Stuart Bowyer,et al. The 1997 reference of diffuse night sky brightness , 1998 .
[2] Robert A. Brown. Single-Visit Photometric and Obscurational Completeness , 2005, astro-ph/0503077.
[3] N. Jeremy Kasdin,et al. Linear and bayesian planet detection algorithms for the Terrestrial planet finder , 2006 .
[4] Stuart B. Shaklan,et al. The lighter side of TPF-C: evaluating the scientific gain from a smaller mission concept , 2007, SPIE Optical Engineering + Applications.
[5] Andrew Cumming,et al. The Keck Planet Search: Detectability and the Minimum Mass and Orbital Period Distribution of Extrasolar Planets , 2008, 0803.3357.
[6] Remi Soummer,et al. NEW COMPLETENESS METHODS FOR ESTIMATING EXOPLANET DISCOVERIES BY DIRECT DETECTION , 2010 .
[7] N. J. Kasdin,et al. Analyzing the Designs of Planet-Finding Missions , 2009, 0903.4915.
[8] Drake Deming,et al. Earth as an extrasolar planet: Earth model validation using EPOXI earth observations. , 2011, Astrobiology.
[9] D. Ciardi,et al. The exoplanet eccentricity distribution from Kepler planet candidates , 2012, 1203.1631.
[10] Zhaohuan Zhu,et al. FAST RISE OF “NEPTUNE-SIZE” PLANETS (4–8 R⊕) FROM P ∼ 10 TO ∼250 DAYS—STATISTICS OF KEPLER PLANET CANDIDATES UP TO ∼0.75 AU , 2012, 1212.4853.
[11] M. R. Haas,et al. PLANET OCCURRENCE WITHIN 0.25 AU OF SOLAR-TYPE STARS FROM KEPLER , 2011, 1103.2541.
[12] Aki Roberge,et al. The Search for Habitable Worlds. 1. The Viability of a Starshade Mission , 2012 .
[13] G. Marcy,et al. A PLATEAU IN THE PLANET POPULATION BELOW TWICE THE SIZE OF EARTH , 2013, 1304.0460.
[14] G. Marcy,et al. Prevalence of Earth-size Planets Orbiting Sun-like Stars , 2015, 1510.03902.
[15] Ryan C. Terrien,et al. HABITABLE ZONES AROUND MAIN-SEQUENCE STARS: NEW ESTIMATES , 2013, 1301.6674.
[16] Luis Marchen,et al. The AFTA coronagraph instrument , 2013, Optics & Photonics - Optical Engineering + Applications.
[17] Timothy D. Brandt,et al. Prospects for detecting oxygen, water, and chlorophyll on an exo-Earth , 2014, Proceedings of the National Academy of Sciences.
[18] R. Soummer,et al. APODIZED PUPIL LYOT CORONAGRAPHS FOR ARBITRARY APERTURES. IV. REDUCED INNER WORKING ANGLE AND INCREASED ROBUSTNESS TO LOW-ORDER ABERRATIONS , 2014, 1412.2751.
[19] William C. Danchi,et al. CONSTRAINING THE EXOZODIACAL LUMINOSITY FUNCTION OF MAIN-SEQUENCE STARS: COMPLETE RESULTS FROM THE KECK NULLER MID-INFRARED SURVEYS , 2014 .
[20] G. Marcy,et al. THE MASS–RADIUS RELATION FOR 65 EXOPLANETS SMALLER THAN 4 EARTH RADII , 2013, 1312.0936.
[21] Ari Silburt,et al. A STATISTICAL RECONSTRUCTION OF THE PLANET POPULATION AROUND KEPLER SOLAR-TYPE STARS , 2014, 1406.6048.
[22] D. Hogg,et al. EXOPLANET POPULATION INFERENCE AND THE ABUNDANCE OF EARTH ANALOGS FROM NOISY, INCOMPLETE CATALOGS , 2014, 1406.3020.