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Institut für Astronomie und Astrophysik

Abteilung Astronomie

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lc_done Source code in lc_done.pro

lc_done

Name
          lc_done
Purpose
          Simulate a light-curve with a power-law distributed
          periodogram
Category
          light curve simulation
Calling Sequence
          lc_done,time,rate,nt=nt,beta=beta,sigma=sigma,mean=mea, $
            seed=seed,dt=dt
Input Parameters
          -
Optional Input Parameters
          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
Keyword Parameters

Output Parameters
        time: Time array (trivial :-) )
        rate: Array of countrates of length nt
Optional Output
        seed: see above
Restrictions

Procedure

Example

Revision History
        Version 1.0, 2002/01/10, Sara Benlloch, IAAT

Last modified by pro2html on 2005 January 04 at 16:47 UTC

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Jörn Wilms (wilms@astro.uni-tuebingen.de)
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