Radial-velocity Searches for Planets Around Active Stars

Raphaëlle D. Haywood (Autor)

Buch | Softcover

XV, 140 Seiten

2018 | 1. Softcover reprint of the original 1st ed. 2016
Springer International Publishing (Verlag)
978-3-319-82310-2 (ISBN)

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This thesis develops new and powerful methods for identifying planetary signals in the presence of "noise" generated by stellar activity, and explores the physical origin of stellar intrinsic variability, using unique observations of the Sun seen as a star. In particular, it establishes that the intrinsic stellar radial-velocity variations mainly arise from suppression of photospheric convection by magnetic fields. With the advent of powerful telescopes and instruments we are now on the verge of discovering real Earth twins in orbit around other stars. The intrinsic variability of the host stars themselves, however, currently remains the main obstacle to determining the masses of such small planets. The methods developed here combine Gaussian-process regression for modeling the correlated signals arising from evolving active regions on a rotating star, and Bayesian model selection methods for distinguishing genuine planetary signals from false positives produced by stellar magnetic activity.
The findings of this thesis represent a significant step towards determining the masses of potentially habitable planets orbiting Sun-like stars.

Raphaëlle D. Haywood studied Physics at Imperial College London, UK, where she obtained her MSci degree in 2011. She went on to do her PhD in Astrophysics on the detection of Neptune- and Earth-mass exoplanets under the supervision of Prof. Andrew Collier Cameron at the University of St Andrews, UK, where she recently graduated in fall 2015. She is now a postdoctoral fellow at Harvard College Observatory, working with Prof. David Charbonneau and his group, where she is pursuing her investigations on the magnetic variability of the Sun and other stars and pushing the magnetic activity barrier in exoplanet mass determinations ever further.

Introduction: the Hunt for Extra-solar Planets.- A Toolkit to Detect Planets Around Active Stars.- Application to Observations of Planet-hosting Stars.- An Exploration into the Radial-velocity Variability of the Sun.- Conclusion.

Erscheinungsdatum	05.03.2022
Reihe/Serie	Springer Theses
Zusatzinfo	XV, 140 p. 60 illus., 57 illus. in color.
Verlagsort	Cham
Sprache	englisch
Maße	155 x 235 mm
Gewicht	2467 g
Themenwelt	Naturwissenschaften ► Physik / Astronomie ► Astronomie / Astrophysik
Schlagworte	Exoplanet Characterisation • Exoplanet (extra-solar planet) Detection • Exoplanet Mass Determination • Low-mass Exoplanets • Radial-velocity Searches • Search for Other Earths • Starspots • Stellar Activity • Stellar Radial-velocity Variability • Sun-like Stars
ISBN-10	3-319-82310-8 / 3319823108
ISBN-13	978-3-319-82310-2 / 9783319823102
Zustand	Neuware