The Exo-Jupiter Candidate FL Lyr b in Data of Kepler and TESS Space Missions
- Authors: Kozyreva V.S.1, Bogomazov A.I.1, Demkov B.P.2, Zotov L.V.1,3, Tutukov A.V.4
- 
							Affiliations: 
							- M. V. Lomonosov Moscow State University, P.K. Sternberg State Astronomical Institute
- Individual enterpreneur
- Higher School of Economics, A.N. Tikhonov Moscow Institute of Electronics and Mathematics
- Institute of Astronomy of Russian Academy of Sciences
 
- Issue: Vol 100, No 5 (2023)
- Pages: 441-451
- Section: Articles
- URL: https://rjpbr.com/0004-6299/article/view/647527
- DOI: https://doi.org/10.31857/S0004629923050067
- EDN: https://elibrary.ru/YWQGEE
- ID: 647527
Cite item
Abstract
We study the light-time effect in the eclipsing binary system FL Lyr using data of the Kepler and TESS space missions. We demonstrate that the system contains a candidate exo-Jupiter FL Lyr b, its probable orbital period being about 22 years.
Keywords
About the authors
V. S. Kozyreva
M. V. Lomonosov Moscow State University, P.K. Sternberg State Astronomical Institute
														Email: a78b@yandex.ru
				                					                																			                												                								Moscow, Russia						
A. I. Bogomazov
M. V. Lomonosov Moscow State University, P.K. Sternberg State Astronomical Institute
														Email: a78b@yandex.ru
				                					                																			                												                								Moscow, Russia						
B. P. Demkov
Individual enterpreneur
														Email: a78b@yandex.ru
				                					                																			                												                								Zelenograd, Moscow, Russia						
L. V. Zotov
M. V. Lomonosov Moscow State University, P.K. Sternberg State Astronomical Institute; Higher School of Economics, A.N. Tikhonov Moscow Institute of Electronics and Mathematics
														Email: a78b@yandex.ru
				                					                																			                												                								Moscow, Russia; Moscow, Russia						
A. V. Tutukov
Institute of Astronomy of Russian Academy of Sciences
							Author for correspondence.
							Email: a78b@yandex.ru
				                					                																			                												                								Moscow, Russia						
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