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Institut für Astronomie und AstrophysikAbteilung AstronomieSand 1, D-72076 Tübingen, Germany |
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lc_done
Simulate a light-curve with a power-law distributed
periodogram
light curve simulation
lc_done,time,rate,nt=nt,beta=beta,sigma=sigma,mean=mea, $
seed=seed,dt=dt
-
nt: Number of bins of the simulated lightcurve (default:65536)
beta: Power law index of the periodogram (default: 1.5)
mean: Mean count rate of the simulated lightcurve (default: 0.)
sigma: Standard deviation of the lightcurve to be simulated
(default:1.)
seed: Seed for the random number generator (returned if not
defined -- see IDL help for randomu function)
fact: Factor introduced by Merrifield & McHardy 1994, MNRS
271, 899 for the Fourier freq. array dimension to
explore the effects of the low-freq. component in the
PSD. They used fact = 10. If not set, then fact = 1.
dt: time resolution of the lightcurve
time: Time array (trivial :-) )
rate: Array of countrates of length nt
seed: see above
Version 1.0, 2002/01/10, Sara Benlloch, IAAT
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