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Issue A&A
Volume 428, Number 3, December IV 2004
Page(s) 1039 - 1042
Section Instruments, observational techniques, and data processing
DOI http://dx.doi.org/10.1051/0004-6361:20041682



A&A 428, 1039-1042 (2004)
DOI: 10.1051/0004-6361:20041682

On detecting short-lived p modes in a stellar oscillation spectrum

T. Appourchaux

Institut d'Astrophysique Spatiale, Université Paris XI - CNRS, Bâtiment 121, 91405 Orsay Cedex, France
    e-mail: Thierry.Appourchaux@ias.u-psud.fr

(Received 16 July 2004 / accepted 26 September 2004 )

Abstract
The false alarm probability for detecting peaks embedded in a power spectrum of noise was given by Scargle (1982). This test has been used in helioseismology to detect long-lived modes such as g modes (Appourchaux et al. 2000). With the development of asteroseismology, there is now a need to define a similar test but for short-lived p modes. In this article, I define a false alarm test for detecting short-lived p modes, and I give the probability of detecting such modes given their signal-to-noise ratio, their linewidths and the duration of observation.


Key words: stars: oscillations -- methods: statistical




© ESO 2004


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