activity
20202026
most citedStellar impact on disequilibrium chemistry and on observed spectra of hot Jupiter atmospheres

22 citations · 73 across the 6 of their papers we have counts for

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6 papers · 1 filter

astro-ph.SR2026

Decoding the Radial Velocity Signatures of Solar Faculae with 3D MHD Simulations

Florian Kröll, Sowmya Krishnamurthy, Alexander Shapiro +8

We model the solar radial velocity (RV) signal induced by faculae, the dominant contributor to RV variability in Sun-like stars. We use a representative case of a facular patch tra…

astro-ph.SR202120 cited

Predictions of Astrometric Jitter for Sun-like Stars. II. Dependence on Inclination, Metallicity, and Active-Region Nesting

K. Sowmya, N. -E. Nèmec, A. I. Shapiro +5

Ultra-precise astrometry from the Gaia mission is expected to lead to astrometric detections of more than 20,000 exoplanets in our Galaxy. One of the factors that could hamper such…

astro-ph.SR2021

Modeling stellar Ca II H & K emission variations. I. Effect of inclination on the S-index

K. Sowmya, A. I. Shapiro, V. Witzke +5

The emission in the near ultraviolet Ca II H & K lines is modulated by stellar magnetic activity. Although this emission, quantified via the S-index, has been serving as a prime pr…

astro-ph.SR202116 cited

Where have all the solar-like stars gone? Rotation period detectability at various inclinations and metallicities

Timo Reinhold, Alexander I. Shapiro, Veronika Witzke +3

The plethora of photometric data collected by the Kepler space telescope has promoted the detection of tens of thousands of stellar rotation periods. However, these periods are not…

astro-ph.SR202014 cited

Connecting measurements of solar and stellar brightness variations

N. -E. Nèmec, E. Işık, A. I. Shapiro +3

Comparing solar and stellar brightness variations is hampered by the difference in spectral passbands used in observations as well as by the possible difference in the inclination…

astro-ph.SR2020

Power spectra of solar brightness variations at different inclinations

N. -E. Nèmec, A. I. Shapiro, N. A. Krivova +4

Magnetic features on the surfaces of cool stars cause variations of their brightness. Such variations have been extensively studied for the Sun. Recent planet-hunting space telesco…