Fig. 1
MAGIC collection area, estimated for an observational sample in the zenith angle range 70°− 80° with Monte Carlo simulations (see also Mirzoyan et al. 2018), and for comparison the collection area (for 20° zenith angle observations in so-called Production 3 layout) of the future CTA array (see Sect. 4 for details). Also shown is the MAGIC collection area at lower zenith angles from Aleksić et al. (2016a).
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