Difference between revisions of "Gamma 2022"
(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...") |
|||
| (One intermediate revision by the same user not shown) | |||
| Line 1: | Line 1: | ||
= Overview = | = 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: | + | 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) = | + | = Low-level data reduction (up to DL3) = |
I refer the reader to [[ RS_Oph_Analysis_Yukiho_v09X ]]. | I refer the reader to [[ RS_Oph_Analysis_Yukiho_v09X ]]. | ||
| − | = High level analysis = | + | = High-level analysis = |
The following table shows the high-level specifications. | The following table shows the high-level specifications. | ||
| Line 29: | Line 29: | ||
<li style="display: inline-block;"> [[File:Fermi LST-1 SED gc09 ac10 Yukiho.png|thumb|none|400px|RS Oph LST-1 and Fermi-LAT SED.]] </li> | <li style="display: inline-block;"> [[File:Fermi LST-1 SED gc09 ac10 Yukiho.png|thumb|none|400px|RS Oph LST-1 and Fermi-LAT SED.]] </li> | ||
</ul></div> | </ul></div> | ||
| − | :For the Fermi-LAT SED, the flux points are the | + | :For the Fermi-LAT SED, the flux points are obtained using the data between August 9 to 12 (after midnight when LST-1 finished run 5704). Notice that the spectral index is different than Yukiho's analysis because the binning of the true-energy axis is different. |
Latest revision as of 14:43, 27 June 2022
Overview[edit]
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)[edit]
I refer the reader to RS_Oph_Analysis_Yukiho_v09X .
High-level analysis[edit]
The following table shows the high-level specifications.
RS Oph Results[edit]
- 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 obtained using the data between August 9 to 12 (after midnight when LST-1 finished run 5704). 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).
