Astrophysics Group, Cavendish Laboratory, University of Cambridge
Kazan Federal University
53
520
521
523
524
52-1
52-6
41.00
29.35
29.31
29.33
29.27
29.05
03.06.01
03.05.01
03.04.03
2
223
614
6135
SCI004000
SCI005000
We present different methods for analyzing the light curves of active galactic nuclei (AGNs). Based on the example of AGN multiwavelength measurements, features of the following methods are considered: (1) structure functions (SFs)—to search for variability timescales; (2) discrete correlation functions (DCFs)—to search for connections between processes; (3) the Lomb–Scargle (L–S) periodogram—to search for periodicity. We analyze advantages and disadvantages of the methods and discuss their constraints and interpretation.
methods: data analysis, statistical, observational; radiation mechanisms: non-thermal
1. Edelson R.A. and Krolik J.H., 1988, ApJ, 333, p. 646
2. Emmanoulopoulos D., McHardy I.M., Papadakis I.E., 2013, MNRAS, 433, 2, p. 443
3. Emmanoulopoulos D., McHardy I.M., Uttley P., 2010, MNRAS, 404, p. 931
4. Hufnagel B.R. and Bregman J.N., 1992, ApJ, 386, p. 473
5. Lomb N.R., 1976, Ap&SS, 39, 2, p. 447
6. Robertson D.R.S., Gallo L.C., Zoghbi A., et al., 2015, MNRAS, 453, 4, p. 3455
7. Scargle J.D., 1982, ApJ, 262, p. 835
8. Simonetti J.H., Cordes J.M., Heeschen D.S., 1985, ApJ, 296, p. 46
9. White R.J., Peterson B.M., 1994, PASP, 106, p. 879.