Asteroseismically Inferred Ages of 132,000 Red Giants with TESS
arXiv:2505.08109 · doi:10.3847/1538-4365/ae315a
Abstract
NASA's TESS mission has identified at least 158,000 oscillating red giants, increasing the known sample by roughly an order of magnitude. After validating that these measurements are reliable to 5% for up to 90% of red giants (Theodoridis & Tayar 2023), we make custom stellar evolution models using MESA in order to estimate ages for ~132,794 of these stars to an average uncertainty of 23%. We show that these ages follow similar distributions to those observed in other samples such as Kepler with small differences likely resulting in the galactic volume probed. We provide these ages to the community to enable future galactic archaeology analyses.
14 pages, 9 figures. For all data, please visit https://zenodo.org/records/18050974
References in corpus (39)
- The Gaia mission
- Modules for Experiments in Stellar Astrophysics (MESA)
- Modules for Experiments in Stellar Astrophysics (MESA): Pulsating Variable Stars, Rotation, Convective Boundaries, and Energy Conservation
- Modules for Experiments in Stellar Astrophysics (MESA): Time-Dependent Convection, Energy Conservation, Automatic Differentiation, and Infrastructure
- Painting a portrait of the Galactic disc with its stellar clusters
- APOGEE Data and Spectral Analysis from SDSS Data Release 16: Seven Years of Observations Including First Results from APOGEE-South
- A million binaries from Gaia eDR3: sample selection and validation of Gaia parallax uncertainties
- Structure and Evolution of Nearby Stars with Planets II. Physical Properties of ~1000 Cool Stars from the SPOCS Catalog
- Asteroseismology and Gaia: Testing Scaling Relations Using 2200 Kepler Stars with TGAS Parallaxes
- Standing on the shoulders of Dwarfs: the asteroseismic LEGACY sample I - oscillation mode parameters
- A time-resolved picture of our Milky Way's early formation history
- A Guide to Realistic Uncertainties on Fundamental Properties of Solar-Type Exoplanet Host Stars
- Coulomb tunneling for fusion reactions in dense matter: Path integral Monte Carlo versus mean field
- Robust Data-driven Metallicities for 175 Million Stars from Gaia XP Spectra
- Oscillating K giants with the WIRE satellite: determination of their asteroseismic masses
- StarHorse results for spectroscopic surveys + Gaia DR3: Chrono-chemical populations in the solar vicinity, the genuine thick disk, and young-alpha rich stars
- Age dating of an early Milky Way merger via asteroseismology of the naked-eye star Indi
- The first all-sky view of the Milky Way stellar halo with Gaia+2MASS RR Lyrae
- APOKASC-3: The Third Joint Spectroscopic and Asteroseismic catalog for Evolved Stars in the Kepler Fields
- Spectroscopic age estimates for APOGEE red-giant stars: Precise spatial and kinematic trends with age in the Galactic disc
- Mass loss along the red giant branch in 46 Globular Clusters and their multiple populations
- Stellar Rotation in the Gaia Era: Revised Open Clusters Sequences
- Chemical Evolution in the Milky Way: Rotation-based ages for APOGEE-Kepler cool dwarf stars
- How accurate are stellar ages based on stellar models ? I. The impact of stellar models uncertainties
- Discovery of post-mass-transfer helium-burning red giants using asteroseismology
- Prospects for Galactic and stellar astrophysics with asteroseismology of giant stars in the Continuous Viewing Zones and beyond
- The Absolute Age of M92
- TESS Giants Transiting Giants II: The hottest Jupiters orbiting evolved stars
- The Ages of Galactic Bulge Stars with Realistic Uncertainties
- Integrated Mass Loss of Evolved Stars in M4 using Asteroseismology
- Asteroseismology of the multiple stellar populations in the Globular Cluster M4
- Asteroseismic Signatures of Core Magnetism and Rotation in Hundreds of Low-Luminosity Red Giants
- Why Machine Learning Models Systematically Underestimate Extreme Values
- A Unified Exploration of the Chronology of the Galaxy
- Connecting integrated RGB mass loss from asteroseismology and globular clusters
- Red giants evolutionary status determination: the complete Kepler catalog
- Identifying Uncertainties in Stellar Evolution Models Using the Open Cluster M67
- Assessing the Accuracy of TESS Asteroseismology with APOGEE
- The highest mass Kepler red giants -- II. Spectroscopic parameters, the amplitude-activity relation, and unexpected halo orbits