Planets around young active solar-type stars: assessing detection capabilities from a non-stabilized spectrograph

Autor: Stephen C. Marsden, Matthew W. Mengel, Alexis Heitzmann, Mathieu Clerte, Ian A. Waite, Robert A. Wittenmyer, C. P. Folsom, Duncan J. Wright, I. Millburn, Brett C. Addison, Pascal Petit
Přispěvatelé: Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS)
Rok vydání: 2021
Předmět:
planets and satellites: detection
FOS: Physical sciences
stars: pre-main-sequence
01 natural sciences
Planet
techniques: radial velocities
stars: activity
0103 physical sciences
planets and satellites: formation
Instrumentation and Methods for Astrophysics (astro-ph.IM)
010303 astronomy & astrophysics
Spectrograph
Solar and Stellar Astrophysics (astro-ph.SR)
stars: individual: HD 141943
Earth and Planetary Astrophysics (astro-ph.EP)
Physics
010308 nuclear & particles physics
Astronomy
Astronomy and Astrophysics
Stars
Astrophysics - Solar and Stellar Astrophysics
[SDU]Sciences of the Universe [physics]
Space and Planetary Science
Active solar
Astrophysics::Earth and Planetary Astrophysics
Astrophysics - Instrumentation and Methods for Astrophysics
Astrophysics - Earth and Planetary Astrophysics
Zdroj: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2021, 505, pp.4989-5011. ⟨10.1093/mnras/stab1586⟩
ISSN: 1365-2966
0035-8711
DOI: 10.1093/mnras/stab1586
Popis: Short-orbit gas giant planet formation/evolution mechanisms are still not well understood. One promising pathway to discriminate between mechanisms is to constrain the occurrence rate of these peculiar exoplanets at the earliest stage of the system's life. However, a major limitation when studying newly born stars is stellar activity. This cocktail of phenomena triggered by fast rotation, strong magnetic fields and complex internal dynamics, especially present in very young stars, compromises our ability to detect exoplanets. In this paper, we investigated the limitations of such detections in the context of already acquired data solely using radial velocity data acquired with a non-stabilised spectrograph. We employed two strategies: Doppler Imaging and Gaussian Processes and could confidently detect Hot Jupiters with semi-amplitude of 100 $m.s^{-1}$ buried in the stellar activity. We also showed the advantages of the Gaussian Process approach in this case. This study serves as a proof of concept to identify potential candidates for follow-up observations or even discover such planets in legacy datasets available to the community.
Comment: 16 pages, 13 figures, 11 pages appendix, accepted for publication in MNRAS
Databáze: OpenAIRE