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A&A 428, 1039-1042 (2004)
DOI: 10.1051/0004-6361:20041682
On detecting short-lived p modes in a stellar oscillation spectrum
T. AppourchauxInstitut 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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