Oscillation mode lifetimes of red giants observed during the initial and first anticentre long run of CoRoT
S. Hekker, C. Barban, F. Baudin, J. De Ridder, T. Kallinger, T. Morel,, W.J. Chaplin, Y. Elsworth

TL;DR
This study measures the lifetimes of oscillation modes in red giants using long-term CoRoT data, demonstrating the effects of data length and noise, and confirming theoretical predictions about mode lifetime dependencies.
Contribution
It introduces a method to correct mode lifetime measurements for observational biases and provides empirical validation of theoretical models for red giant oscillations.
Findings
Mode lifetimes depend on frequency and mode degree.
Data length, gaps, and noise significantly affect lifetime measurements.
Corrected measurements align with theoretical predictions.
Abstract
Long timeseries of data increase the frequency resolution in the power spectrum. This allows for resolving stochastically excited modes with long mode lifetimes, as well as features that are close together in frequency. The CoRoT fields observed during the initial run and second long run partly overlap, and stars in this overlapping field observed in both runs are used to create timeseries with a longer timespan than available from the individual runs. We aim to measure the mode lifetimes of red giants and compare them with theoretical predictions. We also investigate the dependence of the mode lifetimes on frequency and the degree of the oscillation modes. We perform simulations to investigate the influence of the gap in the data between the initial and second long run, the total length of the run and the signal-to-noise ratio on the measured mode lifetime. This provides us with a…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
