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Author Mohan, Prashanth ♦ Mangalam, A. ♦ Chattopadhyay, S.
Source Indian Institute of Astrophysics
Content type Text
File Format PDF
Language English
Subject Domain (in DDC) Natural sciences & mathematics ♦ Physics
Subject Keyword Astrophysics - Astrophysics of Galaxies ♦ Astrophysics - High Energy Astrophysical Phenomena
Description The maximum likelihood estimator is used to determine fit parameters for various parametric models of the Fourier periodogram followed by the selection of the best fit model amongst competing models using the Akaike information criteria. This analysis, when applied to light curves of active galactic nuclei can be used to infer the presence of quasi-periodicity and break or knee frequencies. The extracted information can be used to place constraints on the mass, spin and other properties of the putative central black hole and the region surrounding it through theoretical models involving disk and jet physics.
ISSN 02506335
Educational Use Research
Education Level UG and PG
Learning Resource Type Article
Publisher Institution Indian Academy of Sciences
Starting Page 1