Note
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Gaussian spectral model#
This model parametrises a gaussian spectrum.
It is defined by the following equation:
\[\phi(E) = \frac{N_0}{\sigma \sqrt{2\pi}} \exp{ \frac{- \left( E-\bar{E} \right)^2 }{2 \sigma^2} }\]
Example plot#
Here is an example plot of the model:
from astropy import units as u
import matplotlib.pyplot as plt
from gammapy.modeling.models import GaussianSpectralModel, Models, SkyModel
energy_bounds = [0.1, 100] * u.TeV
model = GaussianSpectralModel(norm="1e-2 cm-2 s-1", mean=2 * u.TeV, sigma=0.2 * u.TeV)
model.plot(energy_bounds)
plt.grid(which="both")
plt.ylim(1e-24, 1e-1)
(1e-24, 0.1)
YAML representation#
Here is an example YAML file using the model:
components:
- name: gaussian-model
type: SkyModel
spectral:
type: GaussianSpectralModel
parameters:
- name: amplitude
value: 1.0e-12
unit: cm-2 s-1
- name: mean
value: 2.0
unit: TeV
- name: sigma
value: 0.2
unit: TeV