Boomerang SNR

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
• Cornelia Arcaro
• 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 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

Analysis webpages

Mono-LST-1

-RF improvement

Stereo LST-1+MAGIC

-Standard analysis check

Main results

- Coming

Internal group meetings

- 2023

Meetings on Background Model estimation (GAL Center and Boomerang groups joint activity)

- 18-10-2023

- 02-11-2023 (coming meeting)

External presentations

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

Conferences

- Coming