Gamma 2022
Revision as of 09:46, 17 June 2022 by AAguascaCabot (talk | contribs) (Created page with "= Overview = The data reduction used for the analysis that will be presented at the Gamma 2022 conference is done using the fixed MC production and the source-dependent analys...")
Overview
The data reduction used for the analysis that will be presented at the Gamma 2022 conference is done using the fixed MC production and the source-dependent analysis. In particular, the same DL3 and MC DL2 obtained by Yukiho are used. A dedicated high-level analysis is done for this conference. Please read the following sections for a detailed description of the data reduction, high level analysis and results:
Low level data reduction (up to DL3)
I refer the reader to RS_Oph_Analysis_Yukiho_v09X .
High level analysis
The following table shows the high-level specifications.
RS Oph Results
- Alpha plot
- Same results as RS_Oph_Analysis_Yukiho_v09X .
- LST-1 and Fermi-LAT Spectral energy distribution (SED)
- For the Fermi-LAT SED, the flux points are the ones shown in RS_Oph_Fermi_Analysis_Mab_Bernardos . Notice that the spectral index is different than Yukiho's analysis because the binning of the true-energy axis is different.
- Comparison LST-1, MAGIC and HESS SEDs
- MAGIC and HESS data from Acciari, V.A., Ansoldi, S., Antonelli, L.A. et al. Nat Astron (2022) and H.E.S.S. Collaboration, Science 376, 77–80 (2022), respectively.
- LST-1 and MAGIC light curve
- MAGIC data from Acciari, V.A., Ansoldi, S., Antonelli, L.A. et al. Nat Astron (2022).