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Extreme Precision Radial Velocity Working Group Final Report

Authors :
Crass, Jonathan
Gaudi, B. Scott
Leifer, Stephanie
Beichman, Charles
Bender, Chad
Blackwood, Gary
Burt, Jennifer A.
Callas, John L.
Cegla, Heather M.
Diddams, Scott A.
Dumusque, Xavier
Eastman, Jason D.
Ford, Eric B.
Fulton, Benjamin
Gibson, Rose
Halverson, Samuel
Haywood, Raphaëlle D.
Hearty, Fred
Howard, Andrew W.
Latham, David W.
Löhner-Böttcher, Johannes
Mamajek, Eric E.
Mortier, Annelies
Newman, Patrick
Plavchan, Peter
Quirrenbach, Andreas
Reiners, Ansgar
Robertson, Paul
Roy, Arpita
Schwab, Christian
Seifahrt, Andres
Szentgyorgyi, Andy
Terrien, Ryan
Teske, Johanna K.
Thompson, Samantha
Vasisht, Gautam
Publication Year :
2021

Abstract

Precise mass measurements of exoplanets discovered by the direct imaging or transit technique are required to determine planet bulk properties and potential habitability. Furthermore, it is generally acknowledged that, for the foreseeable future, the Extreme Precision Radial Velocity (EPRV) measurement technique is the only method potentially capable of detecting and measuring the masses and orbits of habitable-zone Earths orbiting nearby F, G, and K spectral-type stars from the ground. In particular, EPRV measurements with a precision of better than approximately 10 cm/s (with a few cm/s stability over many years) are required. Unfortunately, for nearly a decade, PRV instruments and surveys have been unable to routinely reach RV accuracies of less than roughly 1 m/s. Making EPRV science and technology development a critical component of both NASA and NSF program plans is crucial for reaching the goal of detecting potentially habitable Earthlike planets and supporting potential future exoplanet direct imaging missions such as the Habitable Exoplanet Observatory (HabEx) or the Large Ultraviolet Optical Infrared Surveyor (LUVOIR). In recognition of these facts, the 2018 National Academy of Sciences (NAS) Exoplanet Science Strategy (ESS) report recommended the development of EPRV measurements as a critical step toward the detection and characterization of habitable, Earth-analog planets. In response to the NAS-ESS recommendation, NASA and NSF commissioned the EPRV Working Group to recommend a ground-based program architecture and implementation plan to achieve the goal intended by the NAS. This report documents the activities, findings, and recommendations of the EPRV Working Group.<br />Comment: Full report: 103 pages. Executive summary: 7 pages. More information about the NASA-NSF Exoplanet Observational Research (NN-EXPLORE) program, including the NASA-NSF Extreme Precision Radial Velocity Initiative, can be found here: https://exoplanets.nasa.gov/exep/NNExplore/

Details

Database :
arXiv
Publication Type :
Report
Accession number :
edsarx.2107.14291
Document Type :
Working Paper