WFIRST-AFTA Coronagraph Science Yield Modeling with EXOSIMS
arXiv:1511.02869 · doi:10.1117/1.JATIS.2.1.011006
Abstract
We present and discuss the design details of an extensible, modular, open source software framework called EXOSIMS, which creates end-to-end simulations of space-based exoplanet imaging missions. We motivate the development and baseline implementation of the component parts of this software with models of the WFIRST-AFTA coronagraph, and present initial results of mission simulations for various iterations of the WFIRST-AFTA coronagraph design. We present and discuss two sets of simulations: The first compares the science yield of completely different instruments in the form of early competing coronagraph designs for WFIRST-AFTA. The second set of simulations evaluates the effects of different operating assumptions, specifically the assumed post-processing capabilities and telescope vibration levels. We discuss how these results can guide further instrument development and the expected evolution of science yields.
43 pages, 14 figures; accepted for publication in WFIRST Coronagraph special issue of JATIS
References in corpus (10)
- The false positive rate of Kepler and the occurrence of planets
- Wide-Field InfrarRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA 2015 Report
- The Gemini Planet Imager: First Light
- The Occurrence Rate of Small Planets around Small Stars
- The Occurrence and Mass Distribution of Close-in Super-Earths, Neptunes, and Jupiters
- Synthetic Spectra and Colors of Young Giant Planet Atmospheres: Effects of Initial Conditions and Atmospheric Metallicity
- A Plateau in the Planet Population Below Twice the Size of Earth
- Maximizing the ExoEarth Candidate Yield from a Future Direct Imaging Mission
- Wide-Field InfraRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA Final Report
- Parameter distributions of Keplerian orbits
Cited by in corpus (18)
- Orbits for the Impatient: A Bayesian Rejection Sampling Method for Quickly Fitting the Orbits of Long-Period Exoplanets
- Characterizing Earth Analogs in Reflected Light: Atmospheric Retrieval Studies for Future Space Telescopes
- The Habitable Exoplanet Observatory (HabEx) Mission Concept Study Interim Report
- Characterization of Exoplanet Atmospheres with the Optical Coronagraph on WFIRST
- Analytical tolerancing of segmented telescope co-phasing for exo-Earth high-contrast imaging
- Planet occurrence rate density models including stellar effective temperature
- Prospects for Directly Imaging Young Giant Planets at Optical Wavelengths
- Sensitivity of the Roman Coronagraph Instrument to Exozodiacal Dust
- HWO Target Stars and Systems: A Prioritized Community List of Potential Stellar Targets for the Habitable Worlds Observatory's ExoEarth Survey
- A Simple Depth of Search Metric for Exoplanet Imaging Surveys
- Identifying Exo-Earth Candidates in Direct Imaging Data through Bayesian Classification
- A review of simulation and performance modeling for the Roman coronagraph instrument
- The Roman coronagraph community participation program: observation planning
- Model of the Search For Extraterrestrial Intelligence with Coronagraphic Imaging
- Flight masks of the Roman Space Telescope Coronagraph Instrument
- Apodized Pupil Lyot Coronagraphs with arbitrary aperture telescopes: novel designs using hybrid focal plane masks
- Consequences of Non-Gaussian Instrumental Noise in Perturbed Nulling Interferometers
- Starshade Rendezvous: Exoplanet Sensitivity and Observing Strategy