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20232026
most citedAsteroseismology of the young open cluster NGC 2516 I: Photometric and spectroscopic observations

28 citations · 47 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2026

Global asteroseismology of 19,000 red giants in the TESS Continuous Viewing Zones

K. R. Sreenivas, Timothy R. Bedding, Daniel Huber +5

TESS (Transiting Exoplanet Survey Satellite) has produced long-term photometry for millions of stars across the sky. In this work, we present an asteroseismic catalogue of 19,151 r…

astro-ph.SR2026

Asteroseismic Diagnostics for Red Giants with Kepler: Measuring epsilon and Small Frequency Separations in 16,000 Stars

Yingxiang Wang, Timothy R. Bedding, Yaguang Li +4

Asteroseismic studies of red giants have primarily relied on two global parameters: the large frequency separation (Dnu) and the frequency of maximum power (numax). Meanwhile, the…

astro-ph.SR2025★ 8 cited

Testing the wavelength dependence of oscillations and granulation in red giants using Kepler and TESS

K. R. Sreenivas, Timothy R. Bedding, Daniel Huber +5

Stellar oscillations and granulation in red giants are both powered by convection. Studying the wavelength dependence of their amplitudes can provide useful insights on the driving…

astro-ph.SR2024

Realistic Uncertainties for Fundamental Properties of Asteroseismic Red Giants and the Interplay Between Mixing Length, Metallicity and

Yaguang Li, Timothy R. Bedding, Daniel Huber +8

Asteroseismic modelling is a powerful way to derive stellar properties. However, the derived quantities are limited by built-in assumptions used in stellar models. This work presen…

astro-ph.SR2024

The highest mass Kepler red giants -- I. Global asteroseismic parameters of 48 stars

Courtney L. Crawford, Timothy R. Bedding, Yaguang Li +6

When low- and intermediate-mass stars evolve off the main sequence, they expand and cool into the red giant stages of evolution, which include those associated with shell H burning…

astro-ph.SR2024★ 11 cited

A simple method to measure numax for asteroseismology: application to 16,000 oscillating Kepler red giants

K. R. Sreenivas, Timothy R. Bedding, Yaguang Li +4

The importance of numax (the frequency of maximum oscillation power) for asteroseismology has been demonstrated widely in the previous decade, especially for red giants. With the l…

astro-ph.SR2023★ 28 cited

Asteroseismology of the young open cluster NGC 2516 I: Photometric and spectroscopic observations

Gang Li, Conny Aerts, Timothy R. Bedding +8

Asteroseismic modelling of isolated star presents significant challenges due to the difficulty in accurately determining stellar parameters, particularly the stellar age. These cha…