Figure 9 from Using Muon Rings for the Calibration of the Cherenkov Telescope Array: A Systematic Review of the Method and Its Potential Accuracy

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

Using Muon Rings for the Calibration of the Cherenkov Telescope Array: A Systematic Review of the Method and Its Potential Accuracy

Authors: M. Gaug, S. Fegan, A.M.W. Mitchell, M.C. Maccarone, T. Mineo, and A. Okumura

2019 The Astrophysical Journal Supplement Series 243 11.

Provider: AAS Journals

Caption: Figure 9.

Distribution of the arc width parameter (equivalent to σ_θ) for a real data sample with bad PSF. The obtained 0.2 quantile of 0.°071 is bigger than the one expected from the rest of the observation period. (Figure courtesy of the MAGIC Collaboration.)

Other Images in This Article

Copyright and Terms & Conditions