Bibcode
Thiery, S.; Boumier, P.; Gabriel, A. H.; Bertello, L.; Lazrek, M.; García, R. A.; Grec, G.; Robillot, J. M.; Roca-Cortés, T.; Turck-Chièze, S.; Ulrich, R. K.
Bibliographical reference
Astronomy and Astrophysics, v.355, p.743-750 (2000)
Advertised on:
3
2000
Journal
Citations
51
Refereed citations
37
Description
We show here evidence for the necessity of an asymmetric form in
modelling the profile of an acoustic mode in the power spectral density.
The analysis was performed on a 805-day series of GOLF data (l=0 to 3).
The assumptions used for the fits are discussed and their consequences
quantified, in particular for the optimum choice of the fitting spectral
window. Values are given for the bias on the mode parameters (frequency,
width, splitting) when using a Lorentzian fit. The bias depends on the
degree l and on the frequency, and when taken into account leads to
variations in the mode parameters with degree more consistent with
theoretical expectations.