Spectral analysis of stellar light curves by means of neural networks

被引:23
作者
Tagliaferri, R
Ciaramella, A
Milano, L
Barone, F
Longo, G
机构
[1] Univ Salerno, Dipartimento Matemat & Informat, I-84081 Baronissi, SA, Italy
[2] INFM, Unita Salerno, I-84081 Baronissi, SA, Italy
[3] Univ Naples Federico II, Dipartimento Sci Fis, Naples, Italy
[4] Complesso Univ Monte St Angelo, Ist Nazl Fis Nucl, Sez Napoli, I-80126 Naples, Italy
[5] Osservatorio Astron Capodimonte, I-80131 Naples, Italy
来源
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 1999年 / 137卷 / 02期
关键词
methods : data analysis; techniques : radial velocities; stars : binaries : eclipsing;
D O I
10.1051/aas:1999254
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Periodicity analysis of unevenly collected data is a relevant issue in several scientific fields. In astrophysics, for example, we have to find the fundamental period of light or radial velocity curves which are unevenly sampled observations of stars. Classical spectral analysis methods are unsatisfactory to solve the problem. In this paper we present a neural network based estimator system which performs well the frequency extraction in unevenly sampled signals. Pt uses an unsupervised Hebbian nonlinear neural algorithm to extract, from the interpolated signal, the principal components which, in turn, are used by the MUSIC frequency estimator algorithm to extract the frequencies. The neural network is tolerant to noise and works well also with few points in the sequence. We benchmark the system on synthetic and real signals with the Periodogram and with the Cramer-Rao lower bound.
引用
收藏
页码:391 / 405
页数:15
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