activity
20192021
most citedHARPS-N Solar Radial-Velocity Variations Are Dominated By Large, Bright Magnetic Regions

85 citations · 260 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2021★ 15 cited

Estimating Magnetic Filling Factors From Simultaneous Spectroscopy and Photometry: Disentangling Spots, Plage, and Network

T. W. Milbourne, D. F. Phillips, N. Langellier +21

State of the art radial velocity (RV) exoplanet searches are limited by the effects of stellar magnetic activity. Magnetically active spots, plage, and network regions each have di…

astro-ph.EP2020★ 8 cited

Identifying Exoplanets with Deep Learning. IV. Removing Stellar Activity Signals from Radial Velocity Measurements Using Neural Networks

Zoe L. de Beurs, Andrew Vanderburg, Christopher J. Shallue +24

Exoplanet detection with precise radial velocity (RV) observations is currently limited by spurious RV signals introduced by stellar activity. We show that machine learning techniq…

astro-ph.EP2020★ 35 cited

Detection Limits of Low-mass, Long-period Exoplanets Using Gaussian Processes Applied to HARPS-N Solar RVs

N. Langellier, T. W. Milbourne, D. F. Phillips +29

Radial velocity (RV) searches for Earth-mass exoplanets in the habitable zone around Sun-like stars are limited by the effects of stellar variability on the host star. In particula…

astro-ph.SR2020★ 24 cited

The spectral impact of magnetic activity on disk-integrated HARPS-N solar observations: exploring new activity indicators

A. P. G. Thompson, C. A. Watson, R. D. Haywood +21

Stellar activity is the major roadblock on the path to finding true Earth-analogue planets with the Doppler technique. Thus, identifying new indicators that better trace magnetic a…

astro-ph.EP2020★ 29 cited

An ultra-short period rocky super-Earth orbiting the G2-star HD 80653

G. Frustagli, E. Poretti, T. Milbourne +26

Ultra-short period (USP) planets are a class of exoplanets with periods shorter than one day. The origin of this sub-population of planets is still unclear, with different formatio…

astro-ph.SR2019★ 17 cited

Testing the Spectroscopic Extraction of Suppression of Convective Blueshift

M. Miklos, T. W. Milbourne, R. D. Haywood +21

Efforts to detect low-mass exoplanets using stellar radial velocities (RVs) are currently limited by magnetic photospheric activity. Suppression of convective blueshift is the domi…

astro-ph.SR2019★ 7 cited

Sensitivity of low-degree solar p modes to active and ephemeral regions: frequency shifts back to the Maunder Minimum

William J. Chaplin, Rachel Howe, Sarbani Basu +7

We explore the sensitivity of the frequencies of low-degree solar p-modes to near-surface magnetic flux on different spatial scales and strengths, specifically to active regions wi…

astro-ph.SR2019★ 40 cited

Temporal evolution and correlations of optical activity indicators measured in Sun-as-a-star observations

J. Maldonado, D. F. Phillips, X. Dumusque +29

(Abridged) We perform a detailed study of the main optical activity indicators (Ca II H & K, Balmer lines, Na I D D, and He I D) measured for the Sun…

astro-ph.SR2019★ 85 cited

HARPS-N Solar Radial-Velocity Variations Are Dominated By Large, Bright Magnetic Regions

T. W. Milbourne, R. D. Haywood, D. F. Phillips +37

State of the art radial-velocity (RV) exoplanet searches are currently limited by RV signals arising from stellar magnetic activity. We analyze solar observations acquired over a 3…