Sky model from the paper "Prospects for a survey of the Galactic plane with the Cherenkov Telescope Array" by the CTA Consortium
- 1. IRAP, Université de Toulouse, CNRS, CNES, UPS
- 2. Université Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM; FSLAC IRL 2009, CNRS/IAC
- 3. Dublin City University
- 4. INAF - Osservatorio Astronomico di Palermo " G.S. Vaiana"; INAF - Osservatorio Astrofisico di Arcetri
- 5. Max-Planck-Institut für Kernphysik
Description
The main source model definition file is provided in two formats.
- models_gps.xml: readable using GammaLib/ctools, see http://cta.irap.omp.eu/ctools/users/user_manual/models.html
- models_gps.yaml: readable using Gammapy, see https://docs.gammapy.org/1.0.1/tutorials/api/models.html#model-lists-and-serialisation
We provide separately the three alternative interstellar emission models.
- base: IEM_base.fits
- varmin: IEM_varmin.fits.gz
- varmin-rescaled: IEM_varmin_rescaled.fits.gz
To use the interstellar models one can employ:
- GammaLib/ctools, see http://cta.irap.omp.eu/ctools/users/user_manual/models_spatial.html#diffusemapcube
- Gammapy, see https://docs.gammapy.org/dev/tutorials/api/maps.html?highlight=cube%20diffuse#reading-and-writing
Notes
Files
Files
(589.0 MB)
| Name | Size | Download all |
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md5:6dfb033af742aa8e2d581ed2829a8911
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589.0 MB | Download |
Additional details
Related works
- Is described by
- Preprint: arXiv:2310.02828 (arXiv)