Published February 2019 | Version Submitted
Journal Article Open

Detecting exoplanets with FAST?

  • 1. ROR icon Laboratory of Space Studies and Instrumentation in Astrophysics
  • 2. ROR icon National Astronomical Observatories
  • 3. ROR icon University of Chinese Academy of Sciences
  • 4. ROR icon University of Paris
  • 5. ROR icon Jet Propulsion Lab
  • 6. ROR icon California Institute of Technology

Abstract

We briefly review the various proposed scenarios that may lead to nonthermal radio emissions from exoplanetary systems (planetary magnetospheres, magnetosphere-ionosphere and magnetosphere-satellite coupling, and star-planet interactions), and the physical information that can be drawn from their detection. The latter scenario is especially favorable to the production of radio emission above 70 MHz. We summarize the results of past and recent radio searches, and then discuss FAST characteristics and observation strategy, including synergies. We emphasize the importance of polarization measurements and a high duty-cycle for the very weak targets that radio-exoplanets prove to be.

Additional Information

© 2019 National Astronomical Observatories, CAS and IOP Publishing Ltd. Received 2018 February 6; accepted 2018 June 5. This work is supported by the National Key R&D Program No. 2017YFA0402600, the CAS International Partnership Program No. 14A11KYSB20160008, and the NSFC grant No. 11725313. Part of this research (TJWL) was carried out at JPL/Caltech under a contract with NASA.

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Additional details

Identifiers

Eprint ID
92853
DOI
10.1088/1674-4527/19/2/23
Resolver ID
CaltechAUTHORS:20190212-153233039

Funding

National Program on Key Research and Development Project
2017YFA0402600
Chinese Academy of Sciences
14A11KYSB20160008
National Natural Science Foundation of China
11725313
NASA/JPL/Caltech

Dates

Created
2019-02-13
Created from EPrint's datestamp field
Updated
2021-11-16
Created from EPrint's last_modified field

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Caltech groups
Astronomy Department