PSF_KING¶
The King function parametrisations for PSFs has been in use in astronomy as an analytical PSF model for many instruments, for example by the Fermi-LAT (see 2013ApJ…765…54A).
The distribution has two parameters GAMMA \(\gamma\) and SIGMA \(\sigma\)
and is given by the following formula:
\[dP/d\Omega(r,\sigma,\gamma) =
\frac{1}{2\pi\sigma^2}
\left(1-\frac{1}{\gamma}\right)
\left(1+\frac{r^2}{2\gamma\sigma^2}\right)^{- \gamma}\]
This formula integrates to 1 (see Introduction).
Columns:
ENERG_LO,ENERG_HI– ndim: 1, unit: TeV- True energy axis
THETA_LO,THETA_HI– ndim: 1, unit: deg- Field of view offset axis (see Field of view)
GAMMA– ndim: 2, unit: none- Model parameter (see formula above)
SIGMA– ndim: 2, unit: deg- Model parameter (see formula above)
Recommended axis order: ENERGY, THETA
Header keywords:
As explained in HDU classes, the following header keyword should be used to declare the type of HDU:
HDUDOC= ‘https://github.com/open-gamma-ray-astro/gamma-astro-data-formats’HDUVERS= ‘0.3’HDUCLASS= ‘GADF’HDUCLAS1= ‘RESPONSE’HDUCLAS2= ‘PSF’HDUCLAS3= ‘FULL-ENCLOSURE’HDUCLAS4= ‘PSF_KING’
Example data file: TODO