activity
20032026
most citedState of the Field: Extreme Precision Radial Velocities

369 citations · 1.3k across the 31 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

6 papers · 1 filter

astro-ph.SR2024★ 5 cited

Precise and efficient modeling of stellar-activity-affected solar spectra using SOAP-GPU

Yinan Zhao, Xavier Dumusque, Michael Cretignier +4

One of the main obstacles in exoplanet detection when using the radial velocity (RV) technique is the presence of stellar activity signal induced by magnetic regions. In this conte…

astro-ph.SR2023

Scaling and Evolution of Stellar Magnetic Activity

Emre Işık, Jennifer L. van Saders, Ansgar Reiners +1

Magnetic activity is a ubiquitous feature of stars with convective outer layers, with implications from stellar evolution to planetary atmospheres. Investigating the mechanisms res…

astro-ph.SR2020★ 25 cited

The CARMENES search for exoplanets around M dwarfs: Rubidium abundances in nearby cool stars

C. Abia, H. M. Tabernero, S. A. Korotin +25

In this study, abundances of the neutron-capture elements Rb, Sr, and Zr are derived, for the first time, in a sample of nearby M dwarfs. We focus on stars in the metallicity range…

astro-ph.SR2020★ 8 cited

Inflection point in the power spectrum of stellar brightness variations III: Faculae vs. Spot dominance on stars with known rotation periods

E. M. Amazo-Gomez, A. I. Shapiro, S. K. Solanki +4

Stellar rotation periods can be determined by observing brightness variations caused by active magnetic regions transiting visible stellar disk as the star rotates. The successful…

astro-ph.SR2020★ 7 cited

The CARMENES search for exoplanets around M dwarfs. The He I infrared triplet lines in PHOENIX models of M2-3 V stars

D. Hintz, B. Fuhrmeister, S. Czesla +25

The He I infrared (IR) line at a vacuum wavelength of 10833 A is a diagnostic for the investigation of atmospheres of stars and planets orbiting them. For the first time, we study…

astro-ph.SR2020★ 15 cited

Rotation periods from the inflection point in the power spectrum of stellar brightness variations: II. The Sun

E. M. Amazo-Gómez, A. I. Shapiro, S. K. Solanki +5

Young and active stars generally have regular, almost sinusoidal, patterns of variability attributed to their rotation, while the majority of older and less active stars, including…