activity
20112026
most citedModelling the Rossiter-McLaughlin Effect: Impact of the Convective Centre-to-Limb Variations in the Stellar Photosphere

49 citations · 119 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2026

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum

Cis Lagae, Ginger Frame, Heather M. Cegla +5

Detecting the radial velocity signal of Earth-mass exoplanets requires the characterisation and removal of granulation-induced radial velocity variability from spectroscopic observ…

astro-ph.SR2026

Synthetic disk-integrated absorption lines isolating stellar granulation for high-precision RV studies

Ginger Frame, Heather Cegla, Cis Lagae +6

We present a novel method for constructing high-accuracy, time-varying disk-integrated stellar absorption line profiles that isolate the effects of granulation alone. This framewor…

astro-ph.SR2025

Towards understanding stellar variability at the sub m/s level: Isolating granulation signals in synthetic spectral lines

Ginger Frame, Heather M. Cegla, Veronika Witzke +5

Granulation in the photospheres of FGK-type stars induces variability in absorption lines, complicating exoplanet detection via radial velocities and characterisation via transmiss…

astro-ph.EP2016★ 49 cited

Modelling the Rossiter-McLaughlin Effect: Impact of the Convective Centre-to-Limb Variations in the Stellar Photosphere

H. M. Cegla, M. Oshagh, C. A. Watson +3

Observations of the Rossiter-McLaughlin (RM) effect provide information on star-planet alignments, which can inform planetary migration and evolution theories. Here, we go beyond t…

astro-ph.SR2014★ 2 cited

Understanding Astrophysical Noise from Stellar Surface Magneto-Convection

H. M. Cegla, C. A. Watson, S. Shelyag +1

To obtain cm/s precision, stellar surface magneto-convection must be disentangled from observed radial velocities (RVs). In order to understand and remove the convective signature,…

astro-ph.SR2012★ 43 cited

Stellar Surface Magneto-Convection as a Source of Astrophysical Noise. I. Multi-component Parameterisation of Absorption Line Profiles

H. M. Cegla, S. Shelyag, C. A. Watson +1

We outline our techniques to characterise photospheric granulation as an astrophysical noise source. A four component parameterisation of granulation is developed that can be used…

astro-ph.EP2011★ 25 cited

Stellar jitter from variable gravitational redshift: implications for RV confirmation of habitable exoplanets

H. M. Cegla, C. A. Watson, T. R. Marsh +6

A variation of gravitational redshift, arising from stellar radius fluctuations, will introduce astrophysical noise into radial velocity measurements by shifting the centroid of th…