Exoplanet Imitators: A Test of Stellar Activity Behavior in Radial Velocity Signals

Exoplanet Imitators: A Test of Stellar Activity Behavior in Radial Velocity Signals
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系外行星模仿者:径向速度信号中恒星活动行为的测试

DOI:
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发表时间:
2019
影响因子:
5.3
通讯作者:
H. Giles
H. Giles
中科院分区:
物理与天体物理2区
文献类型:
--
作者:
C. Nava;M. L'opez;R. Haywood;H. Giles

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Accurately modeling effects from stellar activity is a key step in detecting radial velocity (RV) signals of low-mass and long-period exoplanets. RVs from stellar activity are dominated by magnetic active regions that move in and out of sight as the star rotates, producing signals with timescales related to the stellar rotation period. Methods to characterize RV periodograms assume that peaks from magnetic active regions will typically occur at the stellar rotation period or a related harmonic. However, with surface features unevenly spaced and evolving over time, signals from magnetic activity are not perfectly periodic, and the effectiveness of characterizing them with sine curves is unconfirmed. With a series of simulations, we perform the first test of common assumptions about signals from magnetic active regions in RV periodograms. We simulate RVs with quasi-periodic signals that account for evolution and migration of magnetic surface features. As test cases, we apply our analysis to two exoplanet hosts, Kepler-20 and K2-131. Simulating observing schedules and uncertainties of real RV surveys, we find that magnetic active regions commonly produce maximum periodogram peaks at spurious periods unrelated to the stellar rotation period: 81% and 72% of peaks, respectively, for K2-131 and Kepler-20. These unexpected peaks can potentially lead to inaccuracies in derived planet masses. We also find that these spurious peaks can sometimes survive multiple seasons of observation, imitating signals typically attributed to exoplanet companions.
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发表时间: 2019
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影响因子: --
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