[AstroPy] Chi-square problems with lmfit and scipy

Rudolf Baer rbaer25 at gmail.com
Thu May 20 05:11:39 EDT 2021


Hi Peter
thanks for your reply.
I have solved the problem by normalizing the y values as suggested by Ivan.
With my first e mail I provided the python code. I attach the actual data
file.
Your comment on the errors is correct; the file has no errors. I have
introduced a gaussian error,
y_noise=(0.02*y * np.random.normal(size=len(x)))
y=y+y_noise
but it does not affect the results.

with kind regards
Rudolf


On Wed, May 19, 2021 at 10:38 PM Peter Erwin <peter.erwin at gmail.com> wrote:

> Rudolf,
>
> It’s not clear to me what you are doing. You say you are using “lmfit and
> scipy”.
> By “lmfit” do you mean the lmfit package —
> https://lmfit.github.io/lmfit-py/index.html ?
>
> This has nothing to do with scipy (though it assumes numpy exists), so
> maybe you
> are using something else instead?
>
> In any case, I’d guess the chi^2 values are “wrong” because you don’t have
> good error
> estimates (“uncertainties”) for the data values.
>
> Providing examples of the actual Python commands you are using (and maybe
> a few
> sample data values from your NIR spectrum) would be helpful.
>
> cheers,
>
> Peter
>
> > On May 19, 2021, at 5:43 PM, Rudolf Baer <rbaer25 at gmail.com> wrote:
> >
> > I am fitting the continuum of a NIR spectrum with a blackbody plus power
> law using lmfit and scipy. The plot of the fit looks good
> > and the resulting parameters agree reasonably with previous results.
> > T:      1109.29505 +/- 3.08340774 (0.28%) (init = 1100)
> > const:  4.7240e-21 +/- 6.3014e-23 (1.33%) (init = 2e-21)
> > A:      2.4188e-11 +/- 6.3181e-14 (0.26%) (init = 2e-11)
> > p:     -1.06704890 +/- 0.01701493 (1.59%) (init = -1)
> >
> > However the chi-square and reduced chi-square values
> > (chi-square = 1.1268e-20 reduced chi-square = 2.1039e-24)
> > are clearly wrong. The problem is apparently known as the scipy guide
> says Note that the calculation of chi-square and
> > reduced chi-square assume that the returned residual function is scaled
> properly to the uncertainties in the data.
> > For these statistics to be meaningful, the person writing the function
> to be minimized must scale them properly.
> >
> >  I do not know how to do this. Any advice will be appreciated.
> >
> > With kind regards
> > Rudolf Baer
> > Zurich
> >
> >
> >
> > The input data for the code are x: lambda in AA, y: flux density in
> erg/cm^{2}/s/{\AA)
> > Code:
> >
> > x=x_AA/10000. #<---------conversion AA to um
> >
> > y=y*1e4
> >
> > y=y*x
> >
> #=========================================================================================
> >
> > def bb(x, T, const):
> >
> >     from scipy.constants import h,k,c
> >
> >     x = 1e-6 * x # convert to metres from um
> >
> >     return const*2*h*c**2 / (x**5 * (np.exp(h*c / (x*k*T)) - 1))
> #J/s/m2/m
> >
> >
> > def powerlaw(x,A,p):
> >
> >     return A*x**p
> >
> >
> > mod= Model(bb) + Model(powerlaw)
> >
> > pars  = mod.make_params(T=1100,const=2*1e-21,A=2*1e-11,p=-1.0)
> >
> >  result = mod.fit(y,pars,x=x)
> > _______________________________________________
> > AstroPy mailing list
> > AstroPy at python.org
> > https://mail.python.org/mailman/listinfo/astropy
>
> =============================================================
> Peter Erwin                   Max-Planck-Insitute for Extraterrestrial
> erwin at mpe.mpg.de              Physics, Giessenbachstrasse
> tel. +49 (0)176 2481 7713     85748 Garching, Germany
> fax  +49 (0)89 30000 3495     https://www.mpe.mpg.de/~erwin
>
>
>
>
> _______________________________________________
> AstroPy mailing list
> AstroPy at python.org
> https://mail.python.org/mailman/listinfo/astropy
>
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