Performance of the MAGIC telescopes in stereoscopic mode
P. Colin, D. Borla Tridon, E. Carmona, F. De Sabata, M. Gaug, S., Lombardi, P. Majumdar, A. Moralejo, V. Scalzotto, J. Sitarek (for the MAGIC, Collaboration)
TL;DR
The paper evaluates the improved performance of the MAGIC gamma-ray telescopes in stereoscopic mode, demonstrating enhanced resolution, sensitivity, and background rejection through Monte Carlo simulations.
Contribution
It provides the first detailed performance assessment of the MAGIC telescopes operating in stereoscopic mode using Monte Carlo simulations.
Findings
Enhanced angular resolution and energy estimation.
Improved cosmic-ray background rejection.
Significant sensitivity increase across 60 GeV - 20 TeV.
Abstract
The MAGIC gamma-ray observatory has recently been upgraded by a second Cherenkov telescope at a distance of 85 m from the first one. Simultaneous observation of air showers with the two MAGIC telescopes (stereoscopic mode) will improve the reconstruction of the shower axis and solve the ambiguity in the impact point occurring in single-telescope mode. Also, the stereo observation will result in a better angular resolution, energy estimation and cosmic-ray background rejection. It is expected that the sensitivity of MAGIC improves significantly over the full energy range (60 GeV - 20 TeV). Here, we present the performance estimated from Monte Carlo simulations.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsSpacecraft Design and Technology · Adaptive optics and wavefront sensing · Astronomy and Astrophysical Research