Enabling Exoplanet Demographics Studies with Standardized Exoplanet Survey Meta-Data
Abstract
Goal 1 of the National Academies of Science, Engineering and Mathematics Exoplanet Science Strategy is "to understand the formation and evolution of planetary systems as products of the process of star formation, and characterize and explain the diversity of planetary system architectures, planetary compositions, and planetary environments produced by these processes", with the finding that "Current knowledge of the demographics and characteristics of planets and their systems is substantially incomplete." One significant roadblock to our ongoing efforts to improve our demographics analyses is the lack of comprehensive meta-data accompanying published exoplanet surveys. The Exoplanet Program Analysis Group (ExoPAG) Science Interest Group 2: Exoplanet Demographics has prepared this document to provide guidance to survey architects, authors, referees and funding agencies as to the most valuable such data products for five different exoplanet detection techniques - transit, radial velocity, direct imaging, microlensing and astrometry. We find that making these additional data easily available would greatly enhance the community's ability to perform robust, reproducible demographics analyses, and make progress on achieving the most important goals identified by the exoplanet and wider astronomical community.
Keywords
Cite
@article{arxiv.2304.12442,
title = {Enabling Exoplanet Demographics Studies with Standardized Exoplanet Survey Meta-Data},
author = {Prepared by the ExoPAG Science Interest Group and 2 on Exoplanet Demographics and Jessie L. Christiansen and David P. Bennett and Alan P. Boss and Steve Bryson and Jennifer A. Burt and Rachel B. Fernandes and Todd J. Henry and Wei-Chun Jao and Samson A. Johnson and Michael R. Meyer and Gijs D. Mulders and Susan E. Mullally and Eric L. Nielsen and Ilaria Pascucci and Joshua Pepper and Peter Plavchan and Darin Ragozzine and Lee J. Rosenthal and Eliot Halley Vrijmoet},
journal= {arXiv preprint arXiv:2304.12442},
year = {2023}
}
Comments
21 pages, final report after community feedback addressed