FaucherKaspi2006¶
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class
gammapy.astro.population.FaucherKaspi2006(amplitude=1, r_0=7.04, sigma=1.83, **kwargs)[source]¶ Bases:
astropy.modeling.Fittable1DModelRadial distribution of the birth surface density of pulsars in the galaxy - Faucher-Giguere & Kaspi 2006.
\[f(r) = A \frac{1}{\sqrt{2 \pi} \sigma} \exp \left(- \frac{(r - r_0)^2}{2 \sigma ^ 2}\right)\]Reference: http://adsabs.harvard.edu/abs/2006ApJ...643..332F (Appendix B)
Parameters: amplitude : float
See model formula
r_0 : float
See model formula
sigma : float
See model formula
See also
CaseBattacharya1998,Paczynski1990,YusifovKucuk2004,Lorimer2006,YusifovKucuk2004B,ExponentialAttributes Summary
amplitudeevolvedparam_namesr_0sigmaMethods Summary
evaluate(r, amplitude, r_0, sigma)One dimensional Faucher-Giguere & Kaspi 2006 model function Attributes Documentation
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amplitude¶
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evolved= False¶
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param_names= ('amplitude', 'r_0', 'sigma')¶
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r_0¶
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sigma¶
Methods Documentation
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