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Hello all, |
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Dear Marion, All VHE gamma-ray data are full of cosmic-ray induced events and this is why several algorithms have been developed to estimate the background counts needed for any 2D and 3D analysis (see https://docs.gammapy.org/dev/user-guide/makers/index.html#background-estimation). In the case of the test release of H.E.S.S. (HESS-DL3-DR1) made in 2018, no background IRF has been delivered, as mentioned in the accompanying release note (https://www.mpi-hd.mpg.de/HESS/pages/dl3-dr1/hess_dl3_dr1.pdf). User should build their own background model. A dedicated recipes shows how to make a basic background model: https://gammapy.github.io/gammapy-recipes/_build/html/notebooks/background-model/background_model.html. However, in the case of the HESS-DL3-DR1, the Gammapy dataset contain rather good background models that we have produced ourself. The Gammapy Quickstart page explains how to download them (https://docs.gammapy.org/dev/getting-started/index.html#quickstart-setup). |
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Dear Marion,
All VHE gamma-ray data are full of cosmic-ray induced events and this is why several algorithms have been developed to estimate the background counts needed for any 2D and 3D analysis (see https://docs.gammapy.org/dev/user-guide/makers/index.html#background-estimation).
All these methods are using a background model that are delivered by the experiments with the other 3 IRFs (aeff, edisp, PSF, all made from simulations).
In the case of the test release of H.E.S.S. (HESS-DL3-DR1) made in 2018, no background IRF has been delivered, as mentioned in the accompanying release note (https://www.mpi-hd.mpg.de/HESS/pages/dl3-dr1/hess_dl3_dr1.pdf). User should build their own backgroun…