Difference between revisions of "Boomerang SNR"

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== Analysis webpages ==
 
== Analysis webpages ==

Revision as of 09:08, 30 May 2023

Back to Data Analysis

General information

The Boomerang SNR as seen by MAGIC [A&A 658, A60 (2022)]
  • Name of the source: SNR 106.3+2.7
  • Brief description of the source: Strong hadronic PeVatron candidate with TeV emission both from the head and the tail of the SNR
  • Reference coordinated:
- MAGIC Tail: RA, Dec (ICRS): 36.72 deg, 60.84 deg
- MAGIC head: RA, Dec (ICRS): 337.13 deg, 61.10 deg


Proposals

  • MAGIC Cycle XVII (GAL 346)
  • LST Cycle I (GAL 07)

People involved

  • Franca Cassol (PI)
  • Heide Costantini
  • Gabriel Emery
  • Marie-Sophie Carrasco
  • Marine Pihet
  • Takayuki Saito (co-PI)

Data available

There are three set of data :

- Mono-LST-1
- LST+MAGIC
- MAGIC

Monte Carlo Data

Monte Carlo data have been produced with successive productions in order to increase the node density.

- First production has been performed standardly with uniform training nodes on the declination line
- Second production has been performed asking a node with with step cos(zenith)=0.04, for zenith angles > 60 deg (see here)
- Third production has been performed in order to further increase the node density with step cos(zenith)=0.02, for zenith angles > 60 deg (see here)

We asked also to have test nodes on the declination line. The figures below show the present simulated nodes, to be found in

- /fefs/aswg/data/mc/DL0/LSTProd2/TrainingDataset/Protons/dec_6166
- /fefs/aswg/data/mc/DL0/LSTProd2/TrainingDataset/GammaDiffuse/dec_6166
- /fefs/aswg/data/mc/DL0/LSTProd2/TestDataset
Produced node in line May 2023.png
Produced nodes in dec line above 55 deg.png

Analysis webpages

Mono-LST-1

-RF improvement

Stereo LST-1+MAGIC

-Standard analysis check

Main results

- Coming

Internal group meetings

- 2023

External presentations

- 27-03-2023: Random Forest optimization for LZA observations¶ (M. Carrasco, LST analysis meeting)

Conferences

- Coming