Testing the Limits of Precise Subgiant Characterization with APOGEE and Gaia: Opening a Window to Unprecedented Astrophysical Studies-Reference-Cited by-同舟云学术

Testing the Limits of Precise Subgiant Characterization with APOGEE and Gaia: Opening a Window to Unprecedented Astrophysical Studies

Published:2021-06-29 Issue:1 Volume:915 Page:19
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Godoy-Rivera Diego^ORCID,Tayar Jamie^ORCID,Pinsonneault Marc H.^ORCID,Rodríguez Martínez Romy^ORCID,Stassun Keivan G.^ORCID,van Saders Jennifer L.^ORCID,Beaton Rachael L.^ORCID,García-Hernández D. A.^ORCID,Teske Johanna K.

Funder

National Aeronautics and Space Administration

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/abf8ba/pdf

Reference144 articles.

1. The 16th Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2 Southern Survey and Full Release of eBOSS Spectra

2. Gaia Data Release 2

3. The Chemical Composition of the Sun

4. Estimating Distance from Parallaxes. IV. Distances to 1.33 Billion Stars in Gaia Data Release 2

5. On the Rotational Evolution of Solar‐ and Late‐Type Stars, Its Magnetic Origins, and the Possibility of Stellar Gyrochronology

Cited by 13 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Magnetic activity of red giants: Correlation between the amplitude of solar-like oscillations and chromospheric indicators;Astronomy & Astrophysics;2024-06

2. Kepler main-sequence solar-like stars: surface rotation and magnetic-activity evolution;Frontiers in Astronomy and Space Sciences;2024-03-15

3. The breakdown of current gyrochronology as evidenced by old coeval stars;Monthly Notices of the Royal Astronomical Society;2023-06-16

4. A Reanalysis of the Composition of K2-106b: An Ultra-short-period Super-Mercury Candidate;The Astronomical Journal;2023-02-10

5. Revised Extinctions and Radii for 1.5 Million Stars Observed by APOGEE, GALAH, and RAVE;The Astrophysical Journal Supplement Series;2023-02-01