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arXiv 0711.0601astro-ph
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在MOST南河三数据中寻找p模:另一种观点

Searching for p-modes in MOST Procyon data: Another view

F. Baudin, T. Appourchaux, P. Boumier, R. Kuschnig, J. W. Leibacher, J. M. Matthews

摘要:

2004年由MOST卫星获得的南河三光度计已经被几个小组搜索了p模式,有时有相互矛盾的解释。我们探讨了两个可能的因素,使分析复杂化,并可能导致这些数据中的p模式的错误报告。两种方法被用来说明的作用,微妙的仪器效应的光度:时间-频率分析,和搜索规则间隔的峰在傅立叶光谱的基础上的阶梯光栅光谱法。我们没有找到令人信服的证据的p模式信号在MOST南河三的数据。我们可以解释一个明显的过剩的功率接近p模式的频率范围和迹象的结构中阶梯光栅的仪器效应。

英文摘要:

Photometry of Procyon obtained by the MOST satellite in 2004 has been searched for p modes by several groups, with sometimes contradictory interpretations. We explore two possible factors that complicate the analysis and may lead to erroneous reports of p modes in these data. Two methods are used to illustrate the role of subtle instrumental effects in the photometry: time-frequency analysis, and a search for regularly spaced peaks in a Fourier spectrum based on the echelle diagramme approach. We find no convincing evidence of a p-mode signal in the MOST Procyon data. We can account for an apparent excess of power close to the p-mode frequency range and signs of structure in an echelle diagramme in terms of instrumental effects.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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