activity
20142023
most citedStellar magnetism: empirical trends with age and rotation

446 citations · 611 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.EP20231 cited

Identification of the Top TESS Objects of Interest for Atmospheric Characterization of Transiting Exoplanets with JWST

Benjamin J. Hord, Eliza M. -R. Kempton, Thomas Mikal-Evans +142

JWST has ushered in an era of unprecedented ability to characterize exoplanetary atmospheres. While there are over 5,000 confirmed planets, more than 4,000 TESS planet candidates a…

astro-ph.SR201657 cited

Magnetic fields on young, moderately rotating Sun-like stars II. EK Draconis (HD 129333)

Ian Waite, Stephen Marsden, Brad Carter +6

The magnetic fields, activity and dynamos of young solar-type stars can be empirically studied using time-series of spectropolarimetric observations and tomographic imaging techniq…

astro-ph.SR201695 cited

The connection between stellar activity cycles and magnetic field topology

V. See, M. Jardine, A. A. Vidotto +14

Zeeman Doppler imaging has successfully mapped the large-scale magnetic fields of stars over a large range of spectral types, rotation periods and ages. When observed over multiple…

astro-ph.SR20151 cited

Winds of Planet Hosting Stars

B. A. Nicholson, M. W. Mengel, L. Brookshaw +6

The field of exoplanetary science is one of the most rapidly growing areas of astrophysical research. As more planets are discovered around other stars, new techniques have been de…

astro-ph.SR201411 cited

Doppler images and the underlying dynamo. The case of AF Leporis

S. P. Järvinen, R. Arlt, T. Hackman +6

The (Zeeman-)Doppler imaging studies of solar-type stars very often reveal large high-latitude spots. This also includes F stars that possess relatively shallow convection zones, i…

astro-ph.SR2014446 cited

Stellar magnetism: empirical trends with age and rotation

A. A. Vidotto, S. G. Gregory, M. Jardine +12

We investigate how the observed large-scale surface magnetic fields of low-mass stars (~0.1 -- 2 Msun), reconstructed through Zeeman-Doppler imaging (ZDI), vary with age t, rotatio…