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Published October 3, 2023 | Version v2
Dataset Open

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

This work was conducted in the context of the CTA Consortium. We gratefully acknowledge financial support from the agencies and organizations listed here: https://www.cta-observatory.org/consortium_acknowledgments/.

Files

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Additional details

Related works

Is described by
Preprint: arXiv:2310.02828 (arXiv)