Note
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PowerLaw temporal model#
This model parametrises a power-law time model.
\[F(t) = \left( \frac{t - t_{\rm{ref}}}{t_0} \right)^\alpha\]
Example plot#
Here is an example plot of the model:
from astropy import units as u
from astropy.time import Time
import matplotlib.pyplot as plt
from gammapy.modeling.models import (
Models,
PowerLawSpectralModel,
PowerLawTemporalModel,
SkyModel,
)
time_range = [Time.now(), Time.now() + 2 * u.d]
pl_model = PowerLawTemporalModel(alpha=-2.0, t_ref=(time_range[0].mjd - 0.1) * u.d)
pl_model.plot(time_range)
plt.grid(which="both")
plt.yscale("log")
YAML representation#
Here is an example YAML file using the model:
model = SkyModel(
spectral_model=PowerLawSpectralModel(),
temporal_model=pl_model,
name="powerlaw-model",
)
models = Models([model])
print(models.to_yaml())
components:
- name: powerlaw-model
type: SkyModel
spectral:
type: PowerLawSpectralModel
parameters:
- name: index
value: 2.0
- name: amplitude
value: 1.0e-12
unit: cm-2 s-1 TeV-1
- name: reference
value: 1.0
unit: TeV
temporal:
type: PowerLawTemporalModel
parameters:
- name: alpha
value: -2.0
- name: t_ref
value: 60626.720597593274
unit: d
- name: t0
value: 1.0
unit: d
scale: utc
metadata:
creator: Gammapy 2.0.dev2+g10bce85c9
date: '2024-11-12T19:41:39.803680'
origin: null