The Exo-Jupiter Candidate FL Lyr b in Data of Kepler and TESS Space Missions-Reference-Cited by-同舟云学术

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The Exo-Jupiter Candidate FL Lyr b in Data of Kepler and TESS Space Missions

Published:2023-05-01 Issue:5 Volume:100 Page:441-451
ISSN:0004-6299
Container-title:Астрономический журнал
language:
Short-container-title:Astronomičeskij žurnal

Author:

Kozyreva V. S.¹,Bogomazov A. I.¹,Demkov B. P.²,Zotov L. V.¹³,Tutukov A. V.⁴

Affiliation:

1. M. V. Lomonosov Moscow State University, P.K. Sternberg State Astronomical Institute

2. Individual enterpreneur

3. Higher School of Economics, A.N. Tikhonov Moscow Institute of Electronics and Mathematics

4. Institute of Astronomy of Russian Academy of Sciences

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.

Publisher

The Russian Academy of Sciences

Reference15 articles.

1. N. A. Kaib, S. N. Raymond, and M. Duncan, Nature 493, 381 (2013).

2. A. V. Tutukov and A. I. Bogomazov, Astron. Rep. 56, 775 (2012).

3. V. S. Kozyreva, A. I. Bogomazov, B. P. Demkov, L. V. Zotov, and A. V. Tutukov, Astron. Rep. 59, 1036 (2015).

4. V. S. Kozyreva, A. I. Bogomazov, B. P. Demkov, L. V. Zotov, and A. V. Tutukov, Astron. Rep. 60, 534 (2016).

5. K. G. Helminiak, N. Ukita, E. Kambe, S. K. Kozlowski, et al., Monthly Not. Roy. Astron. Soc. 468, 1726 (2017).

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