Institut für Astronomie und AstrophysikAbteilung AstronomieSand 1, D-72076 Tübingen, Germany |
fiterror
compute two-sided, asymmetric error bars for a chi^2 fit
function fitting
result=fiterror(x, y, ww, apar, sigmaa,chi2=cchi2, $ bounds=bounds, delchi=delchi,toldel=toldel, $ debug=debug,intpar=intpar,...)
similar to jwcurvefit, see the documentation of jwcurvefit for an exhaustive explanation. The input-parameter apar is the best-fit vector as returned from jwcurvefit, sigmaa is the "uncertainty" (i.e. the diagonal elements of the Hessian matrix) as returned from jwcurvefit.
chi2= the (reduced) chi^2 value of the best fit as returned from jwcurvefit debug= return tons of debugging information if set. intpar= array containing the indexes of all interesting parameters, i.e., those for which the uncertainty is to be computed (note: although the word interesting is used here, this is not to be confused with the notion of "interesting parameters" in chi^2 minimization) delchi= delta chi^2 to be used for the determination of the uncertainty. default: 1, corresponding to 1 sigma errors. Use 2.71 for 90% uncertainty (in general, delchi=chisqr_dvf(1-prob,1) where prob is the probability that the n dimensional parameter space spanned by the uncertainties contains the real value) maxtry= maximum number of invocations of jwcurvefit in the determination of ONE error (used to determine non-convergence).
a 2 dimensional array containing the error ranges for all fit parameters (lower boundary = upper boundary for the fixed parameters).
a not very stable combination of a secant method and bisection
Version 1.0, 1999.10.21, Joern Wilms (wilms@astro.uni-tuebingen.de), based on previous work by JW and input from Mike Nowak (mnowak@rocinante.colorado.edu). CVS Version 1.4, 2001.02.01, Joern Wilms corrected bug occuring when trial starting value was outside the bounds CVS Version 1.5, 2001.10.07, Joern Wilms corrected bug resulting in the code to loop (logical mistake)
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