activity
20172021
most citedHARPS-N Solar Radial-Velocity Variations Are Dominated By Large, Bright Magnetic Regions

85 citations · 259 across the 10 of their papers we have counts for

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Showing astro-ph.SRShow all

6 papers · 1 filter

astro-ph.SR2021

Star-disk interaction in the T Tauri star V2129 Oph: An evolving accretion-ejection structure

A. P. Sousa, J. Bouvier, S. H. P. Alencar +16

Classical T Tauri stars are young low-mass systems still accreting material from their disks. These systems are dynamic on timescales of hours to years. The observed variability ca…

astro-ph.SR202025 cited

The GAPS Programme at TNG -- XXV. Stellar atmospheric parameters and chemical composition through GIARPS optical and near-infrared spectra

M. Baratella, V. D'Orazi, K. Biazzo +20

The detailed chemical composition of stars is important in many astrophysical fields, among which the characterisation of exoplanetary systems. Previous studies seem to indicate an…

astro-ph.SR201917 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.SR201940 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.SR201985 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…

astro-ph.SR20176 cited

The GAPS Programme with HARPS-N at TNG XV. A substellar companion around a K giant star identified with quasi-simultaneous HARPS-N and GIANO measurements

E. González - Álvarez, L. Affer, G. Micela +34

Context. Identification of planetary companions of giant stars is made difficult because of the astrophysical noise, that may produce radial velocity (RV) variations similar to tho…