利用SPIRou与TESS发现并表征TOI-1695周围的亚海王星行星
地球与行星天体物理
2023-02-22 v2
摘要
TOI-1695是一颗位于北半球、距太阳45pc的V星等=13的M型矮星,在TESS测光中识别出由其超级地球候选体产生的3.134天周期凌星信号。凌星深度为1.3mmag,TESS流水线估计候选体TOI-1695.01的半径为1.82R,平衡温度约K。借助SPIRou红外光谱偏振仪对TOI-1695长达一年的视向速度监测,我们成功探测到恒星的反射运动,并确定其由轨道周期与测光凌星周期一致的行星伴星引起。我们使用并比较了不同方法来归约和分析这些数据。我们报告了5.5-的行星信号探测,得出质量为M、半径为R。我们推导出该行星平均平衡温度为K。这颗小行星的平均密度gcm与地球相似(低1.7-)。这导致其大气中挥发性组分不可忽略,其中%或%。TOI-1695b是一颗位于M型矮星半径谷边界的新亚海王星行星,有助于检验超级地球/亚海王星类行星的形成情景。
引用
@article{arxiv.2211.06205,
title = {A sub-Neptune planet around TOI-1695 discovered and characterized with SPIRou and TESS},
author = {F. Kiefer and G. Hébrard and E. Martioli and E. Artigau and R. Doyon and J. -F. Donati and C. Cadieux and A. Carmona and D. R. Ciardi and P. I. Cristofari and L. de Almeida and P. Figueira and E. Gaidos and E. Gonzales and A. Lecavelier and K. G. Stassun and L. Arnold and B. Benneke and I. Boisse and X. Bonfils and N. J. Cook and P. Cortés-Zuleta and X. Delfosse and J. Dias do Nascimento and M. Fausnaugh and W. Fong and P. Fouqué and T. Forveille and J. Gomes da Silva and K. Hesse and Á. Kóspál and H. Lewis and C. -F. Liu and J. H. C. Martins and M. Paegert and S. Seager and H. Shang and J. D. Twicken and T. Vandal and S. Vinatier and T. Widemann and J. N. Winn},
journal= {arXiv preprint arXiv:2211.06205},
year = {2023}
}
备注
15 pages (+9 appendix pages), 19 figures, 8 tables, accepted for publication in A&A