The California Legacy Survey. V. Chromospheric Activity Cycles in Main-sequence Stars

Abstract We present optical spectroscopy of 710 solar neighborhood stars collected over 20 years to catalog chromospheric activity and search for stellar activity cycles. The California Legacy Survey stars are amenable to exoplanet detection using precise radial velocities, and we present their Ca ii H and K time series as a proxy for stellar and chromospheric activity. Using the High Resolution Echelle Spectrometer at Keck Observatory, we measured stellar flux in the cores of the Ca ii H and K lines to determine S -values on the Mount Wilson scale and the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mi>log</mml:mi> <mml:mo stretchy="false">(</mml:mo> <mml:msubsup> <mml:mi>R</mml:mi> <mml:mi>HK</mml:mi> <mml:mo>′</mml:mo> </mml:msubsup> <mml:mo stretchy="false">)</mml:mo> </mml:math> metric, which is comparable across a wide range of spectral types. From the 710 stars, with 52,372 observations, 285 stars were sufficiently sampled to search for stellar activity cycles with periods of 2–25 yr, and 138 stars showed stellar cycles of varying length and amplitude. S -values can be used to mitigate stellar activity in the detection and characterization of exoplanets. We used them to probe stellar dynamos and to place the Sun's magnetic activity into context among solar neighborhood stars. Using precise stellar parameters and time-averaged activity measurements, we found tightly constrained cycle periods as a function of stellar temperature between <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mi>log</mml:mi> <mml:mo stretchy="false">(</mml:mo> <mml:msubsup> <mml:mi>R</mml:mi> <mml:mi>HK</mml:mi> <mml:mo>′</mml:mo> </mml:msubsup> <mml:mo stretchy="false">)</mml:mo> </mml:math> of −4.7 and −4.9, a range of activity in which nearly every star has a periodic cycle. These observations present the largest sample of spectroscopically determined stellar activity cycles to date.

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Publication Details

Journal
The Astrophysical Journal Supplement Series
Published
2024-09-30
DOI
https://doi.org/10.3847/1538-4365/ad676c
Citations
12
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
3.98

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article

The California Legacy Survey. V. Chromospheric Activity Cycles in Main-sequence Stars

Howard Isaacson, Jack Lubin, Andrew W. Mayo, Stephen R. Kane et al.
12 citations
The Astrophysical Journal Supplement Series
Stellar, planetary, and galactic studies
3.98
article

The California Legacy Survey. V. Chromospheric Activity Cycles in Main-sequence Stars

Howard Isaacson, Jack Lubin, Andrew W. Mayo, Stephen R. Kane, Andrew W. Howard, Steven Giacalone, Corey Beard, Dakotah Tyler, Malena Rice, Samuel W. Yee, Michelle L. Hill, Ian J. M. Crossfield, Casey L. Brinkman, Daria Pidhorodetska, Benjamin J. Fulton, Aida Behmard, Erik A. Petigura, Sarah Blunt, Ashley Chontos, Judah Van Zandt, Alex S. Polanski, Joseph M. Akana Murphy, Luke G. Bouma, Emma V. Turtelboom, Ryan A. Rubenzahl, Mason G. MacDougall, Isabel Angelo, Lauren M. Weiss, Rae Holcomb, Paul A. Dalba, Nicholas Saunders, Jingwen Zhang, Brad Carter, Fei Dai
article en
12 citations

Abstract

Abstract We present optical spectroscopy of 710 solar neighborhood stars collected over 20 years to catalog chromospheric activity and search for stellar activity cycles. The California Legacy Survey stars are amenable to exoplanet detection using precise radial velocities, and we present their Ca ii H and K time series as a proxy for stellar and chromospheric activity. Using the High Resolution Echelle Spectrometer at Keck Observatory, we measured stellar flux in the cores of the Ca ii H and K lines to determine S -values on the Mount Wilson scale and the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mi>log</mml:mi> <mml:mo stretchy="false">(</mml:mo> <mml:msubsup> <mml:mi>R</mml:mi> <mml:mi>HK</mml:mi> <mml:mo>′</mml:mo> </mml:msubsup> <mml:mo stretchy="false">)</mml:mo> </mml:math> metric, which is comparable across a wide range of spectral types. From the 710 stars, with 52,372 observations, 285 stars were sufficiently sampled to search for stellar activity cycles with periods of 2–25 yr, and 138 stars showed stellar cycles of varying length and amplitude. S -values can be used to mitigate stellar activity in the detection and characterization of exoplanets. We used them to probe stellar dynamos and to place the Sun's magnetic activity into context among solar neighborhood stars. Using precise stellar parameters and time-averaged activity measurements, we found tightly constrained cycle periods as a function of stellar temperature between <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mi>log</mml:mi> <mml:mo stretchy="false">(</mml:mo> <mml:msubsup> <mml:mi>R</mml:mi> <mml:mi>HK</mml:mi> <mml:mo>′</mml:mo> </mml:msubsup> <mml:mo stretchy="false">)</mml:mo> </mml:math> of −4.7 and −4.9, a range of activity in which nearly every star has a periodic cycle. These observations present the largest sample of spectroscopically determined stellar activity cycles to date.

The Astrophysical Journal Supplement SeriesVol. 274(2)
Planetary Science Institute (US)
National Science Foundation, National Aeronautics and Space Administration, W. M. Keck Foundation, California Institute of Technology, NASA Exoplanet Science Institute
Openalex Percentile: Top 6%
Stellar, planetary, and galactic studies
3.98
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