agauss, zagauss: gaussian line profile in wavelength space

A simple gaussian line profile. If the width is $\leq 0$ then it is treated as a delta function. The zagauss variant computes a redshifted gaussian.

$\displaystyle A(\lambda) = K {1\over{\sigma\sqrt{2\pi}}}
\exp(-(\lambda-\lambda_l)^2/2\sigma^2)
$

where:

par1 = $\lambda_l$ line wavelength in Angstrom
par2 = $\sigma$ line width in Angstrom
Norm = K total photons/cm$^2$/s in the line

For zagauss the corresponding formula is:

$\displaystyle A(\lambda) = K {(1+z)\over{\sigma\sqrt{2\pi}}}
\exp(-(\lambda/(1+z)-\lambda_l)^2/2\sigma^2)
$

and the parameters are:

par1 = $\lambda_l$ line wavelength in Angstrom
par2 = $\sigma$ line width in Angstrom
par3 = z redshift
Norm = K total photons/cm$^2$/s in the line

The line is truncated at the point that the integrated flux under the line is within a critical value of the total flux. This critical value can be changed using xset LINECRITLEVEL. The default critical value is $1.0\times10^{-6}$.


HEASARC Home | Observatories | Archive | Calibration | Software | Tools | Students/Teachers/Public

Last modified: Friday, 23-Aug-2024 13:20:40 EDT

HEASARC Staff Scientist Position - Applications are now being accepted for a Staff Scientist with significant experience and interest in the technical aspects of astrophysics research, to work in the High Energy Astrophysics Science Archive Research Center (HEASARC) at NASA Goddard Space Flight Center (GSFC) in Greenbelt, MD. Refer to the AAS Job register for full details.