.. DO NOT EDIT. .. THIS FILE WAS AUTOMATICALLY GENERATED BY SPHINX-GALLERY. .. TO MAKE CHANGES, EDIT THE SOURCE PYTHON FILE: .. "user-guide/model-gallery/spectral/plot_smooth_broken_powerlaw.py" .. LINE NUMBERS ARE GIVEN BELOW. .. only:: html .. note:: :class: sphx-glr-download-link-note :ref:`Go to the end ` to download the full example code. or to run this example in your browser via Binder .. rst-class:: sphx-glr-example-title .. _sphx_glr_user-guide_model-gallery_spectral_plot_smooth_broken_powerlaw.py: .. _smooth-broken-powerlaw-spectral-model: Smooth broken power law spectral model ====================================== This model parametrises a smooth broken power law spectrum. It is defined by the following equation: .. math:: \phi(E) = \phi_0 \cdot \left( \frac{E}{E_0} \right)^{-\Gamma1}\left(1 + \frac{E}{E_{break}}^{\frac{\Gamma2-\Gamma1}{\beta}} \right)^{-\beta} .. GENERATED FROM PYTHON SOURCE LINES 16-19 Example plot ------------ Here is an example plot of the model: .. GENERATED FROM PYTHON SOURCE LINES 19-36 .. code-block:: Python from astropy import units as u import matplotlib.pyplot as plt from gammapy.modeling.models import Models, SkyModel, SmoothBrokenPowerLawSpectralModel energy_bounds = [0.1, 100] * u.TeV model = SmoothBrokenPowerLawSpectralModel( index1=1.5, index2=2.5, amplitude="1e-12 TeV-1 cm-2 s-1", ebreak="1 TeV", reference="1 TeV", beta=1, ) model.plot(energy_bounds) plt.grid(which="both") .. image-sg:: /user-guide/model-gallery/spectral/images/sphx_glr_plot_smooth_broken_powerlaw_001.png :alt: plot smooth broken powerlaw :srcset: /user-guide/model-gallery/spectral/images/sphx_glr_plot_smooth_broken_powerlaw_001.png :class: sphx-glr-single-img .. GENERATED FROM PYTHON SOURCE LINES 37-40 YAML representation ------------------- Here is an example YAML file using the model: .. GENERATED FROM PYTHON SOURCE LINES 40-45 .. code-block:: Python model = SkyModel(spectral_model=model, name="smooth-broken-power-law-model") models = Models([model]) print(models.to_yaml()) .. rst-class:: sphx-glr-script-out .. code-block:: none components: - name: smooth-broken-power-law-model type: SkyModel spectral: type: SmoothBrokenPowerLawSpectralModel parameters: - name: index1 value: 1.5 - name: index2 value: 2.5 - name: amplitude value: 1.0e-12 unit: cm-2 s-1 TeV-1 - name: ebreak value: 1.0 unit: TeV - name: reference value: 1.0 unit: TeV - name: beta value: 1.0 metadata: creator: Gammapy 1.3 date: '2024-11-26T10:08:43.774735' origin: null .. _sphx_glr_download_user-guide_model-gallery_spectral_plot_smooth_broken_powerlaw.py: .. only:: html .. container:: sphx-glr-footer sphx-glr-footer-example .. container:: binder-badge .. image:: images/binder_badge_logo.svg :target: https://mybinder.org/v2/gh/gammapy/gammapy-webpage/v1.3?urlpath=lab/tree/notebooks/1.3/user-guide/model-gallery/spectral/plot_smooth_broken_powerlaw.ipynb :alt: Launch binder :width: 150 px .. container:: sphx-glr-download sphx-glr-download-jupyter :download:`Download Jupyter notebook: plot_smooth_broken_powerlaw.ipynb ` .. container:: sphx-glr-download sphx-glr-download-python :download:`Download Python source code: plot_smooth_broken_powerlaw.py ` .. container:: sphx-glr-download sphx-glr-download-zip :download:`Download zipped: plot_smooth_broken_powerlaw.zip ` .. only:: html .. rst-class:: sphx-glr-signature `Gallery generated by Sphinx-Gallery `_