Difference between revisions of "RS Oph paper meetings"
| Line 8: | Line 8: | ||
{{Date|2022-02-23}} | {{Date|2022-02-23}} | ||
| − | To be done: LST analysis | + | * To be done: |
| + | :- LST analysis | ||
| + | :- produce MC production with specific NSB parameters, zenith and azimuth angles for RS Oph observation conditions. | ||
{{Date|2022-03-09}} | {{Date|2022-03-09}} | ||
Revision as of 18:26, 10 March 2022
2022-02-09
Kick off meeting, division of the work. We decided that we should To be done: LST analysis, Fermi analysis, we decided not to go for optical analysis => will use the data that will be published by MAGIC
2022-02-23
- To be done:
- - LST analysis
- - produce MC production with specific NSB parameters, zenith and azimuth angles for RS Oph observation conditions.
2022-03-09
- Discussion
- - Runs in dark conditions present similar pixel charge distribution. We exclude the ones with runs affected by moon or strange distribution.
- Presented
- - First results using the IRFs computed by lstmcpipe.
- - First result analysis RS Oph with Fermi data
- To be done:
- - Several checks on Crab, using 3 different datasets: 20201120, September 2021 and March 2022.
- - Compare sensitivity plots
2022-03-30
