STELLAR SURFACE MAGNETO-CONVECTION AS A SOURCE OF ASTROPHYSICAL NOISE. I. MULTI-COMPONENT PARAMETERIZATION OF ABSORPTION LINE PROFILES
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C. A. Watson | H. M. Cegla | M. Mathioudakis | S. Shelyag | C. Watson | H. Cegla | S. Shelyag | M. Mathioudakis | M. Mathioudakis
[1] S. Solanki,et al. Stokes diagnostics of simulated solar magneto-convection , 2007, astro-ph/0703490.
[2] F. Keenan,et al. Vorticity in the solar photosphere , 2010, 1010.5604.
[3] C. Schrijver,et al. Solar and Stellar Magnetic Activity: Mechanisms of atmospheric heating , 2000 .
[4] Christophe Lovis,et al. Planetary detection limits taking into account stellar noise - I. Observational strategies to reduce stellar oscillation and granulation effects , 2010, 1010.2616.
[5] C. Watson,et al. Stellar jitter from variable gravitational redshift: implications for radial velocity confirmation of habitable exoplanets , 2011, 1112.1553.
[6] V. Makarov. VARIABILITY OF SURFACE FLOWS ON THE SUN AND THE IMPLICATIONS FOR EXOPLANET DETECTION , 2010, 1004.1383.
[7] M. Schuessler,et al. A solar surface dynamo , 2007, astro-ph/0702681.
[8] D. Dravins. 'Ultimate' information content in solar and stellar spectra: Photospheric line asymmetries and wavelength shifts , 2008, 0810.2533.
[9] T. Emonet,et al. Simulations of magneto-convection in the solar photosphere Equations, methods, and results of the MURaM code , 2005 .
[10] F. Bouchy,et al. An Earth-mass planet orbiting α Centauri B , 2012, Nature.
[11] D. Queloz,et al. The HARPS search for Earth-like planets in the habitable zone - I. Very low-mass planets around HD 20794, HD 85512, and HD 192310 , 2011, 1108.3447.
[12] S. Aigrain,et al. Correction to: A simple method to estimate radial velocity variations due to stellar activity using photometry , 2011, Monthly Notices of the Royal Astronomical Society.
[13] S. Criscuoli. COMPARISON OF PHYSICAL PROPERTIES OF QUIET AND ACTIVE REGIONS THROUGH THE ANALYSIS OF MAGNETOHYDRODYNAMIC SIMULATIONS OF THE SOLAR PHOTOSPHERE , 2013, 1309.5494.