Difference between revisions of "RS Oph paper meetings"
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{{Date|2022-03-09}} | {{Date|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. | ||
− | To be done: Several checks on Crab, | + | * 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 | ||
{{Date|2022-03-30}} | {{Date|2022-03-30}} |
Revision as of 18:22, 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
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