Singular Spectrum Analysis for astronomical time series: constructing a parsimonious hypothesis test

التفاصيل البيبلوغرافية
العنوان: Singular Spectrum Analysis for astronomical time series: constructing a parsimonious hypothesis test
المؤلفون: Greco, G., Kondrashov, D., Kobayashi, S., Ghil, M., Branchesi, M., Guidorzi, C., Stratta, G., Ciszak, M., Marino, F., Ortolan, A.
سنة النشر: 2015
المجموعة: Astrophysics
مصطلحات موضوعية: Astrophysics - Instrumentation and Methods for Astrophysics
الوصف: We present a data-adaptive spectral method - Monte Carlo Singular Spectrum Analysis (MC-SSA) - and its modification to tackle astrophysical problems. Through numerical simulations we show the ability of the MC-SSA in dealing with $1/f^{\beta}$ power-law noise affected by photon counting statistics. Such noise process is simulated by a first-order autoregressive, AR(1) process corrupted by intrinsic Poisson noise. In doing so, we statistically estimate a basic stochastic variation of the source and the corresponding fluctuations due to the quantum nature of light. In addition, MC-SSA test retains its effectiveness even when a significant percentage of the signal falls below a certain level of detection, e.g., caused by the instrument sensitivity. The parsimonious approach presented here may be broadly applied, from the search for extrasolar planets to the extraction of low-intensity coherent phenomena probably hidden in high energy transients.
Comment: Refereed Proceeding of the "The Universe of Digital Sky Surveys" conference held at the INAF - Observatory of Capodimonte, Naples, on 25th-28th november 2014, to be published on Astrophysics and Space Science Proceedings, edited by Longo, Napolitano, Marconi, Paolillo, Iodice
نوع الوثيقة: Working Paper
DOI: 10.1007/978-3-319-19330-4_16
URL الوصول: http://arxiv.org/abs/1509.03342
رقم الأكسشن: edsarx.1509.03342
قاعدة البيانات: arXiv
الوصف
DOI:10.1007/978-3-319-19330-4_16