Exoplanet Exploration Program Analysis Group (ExoPAG) Report to Paul Hertz Regarding Large Mission Concepts to Study for the 2020 Decadal Survey
B. Scott Gaudi, Eric Agol, Daniel Apai, Eduardo Bendek, Alan Boss,, James B. Breckinridge, David R. Ciardi, Nicolas B. Cowan, William C. Danchi,, Shawn Domagal-Goldman, Jonathan J. Fortney, Thomas P. Greene, Lisa, Kaltenegger, James F. Kasting, David T. Leisawitz, Alain Leger

TL;DR
This report summarizes consensus among astrophysics program analysis groups on studying four large mission concepts for the 2020 Decadal Survey, emphasizing community support and the need for detailed maturation of these missions.
Contribution
It provides a coordinated recommendation to study four specific large mission concepts and supports the development of probe-class missions within the astrophysics portfolio.
Findings
Consensus on studying four large mission concepts
Strong community support for mission maturation via STDTs
Support for probe-class missions within the portfolio
Abstract
This is a joint summary of the reports from the three Astrophysics Program Analysis Groups (PAGs) in response to the "Planning for the 2020 Decadal Survey" charge given by the Astrophysics Division Director Paul Hertz. This joint executive summary contains points of consensus across all three PAGs. Additional findings specific to the individual PAGs are reported separately in the individual reports. The PAGs concur that all four large mission concepts identified in the white paper as candidates for maturation prior to the 2020 Decadal Survey should be studied in detail. These include the Far-IR Surveyor, the Habitable-Exoplanet Imaging Mission, the UV/Optical/IR Surveyor, and the X-ray Surveyor. This finding is predicated upon assumptions outlined in the white paper and subsequent charge, namely that 1) major development of future large flagship missions under consideration are to…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Gamma-ray bursts and supernovae
