Difference between revisions of "RS Oph paper meetings"

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{{Date|2022-03-09}}
 
{{Date|2022-03-09}}
First results using the IRFs computed by lstmcpipe.
+
* 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, etc...
+
* 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