Difference between revisions of "Boomerang SNR"

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== Proposals==
 
== Proposals==
* [MAGIC Cycle XVII] (GAL 346)
+
* [[File:MAGIC_Cycle18_draft_GAL00346_Cassol.pdf MAGIC Cycle XVII (GAL 346)]]
 
* [LST Cycle I] (GAL 07)
 
* [LST Cycle I] (GAL 07)
  
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== External presentations ==
 
== External presentations ==
:- 27-03-2023: [https://indico.cta-observatory.org/event/4791/contributions/38892/attachments/23381/33603/20230327_LST_Analysis_Call_RFoptimizationLZA.pdf  
+
:- 27-03-2023: [https://indico.cta-observatory.org/event/4791/contributions/38892/attachments/23381/33603/20230327_LST_Analysis_Call_RFoptimizationLZA.pdf Random Forest optimization for LZA observations¶] (M. Carrasco, LST analysis meeting)
Random Forest optimization for LZA observations] (M. Carrasco, LST analysis meeting)
 
  
 
== Conferences ==
 
== Conferences ==
 
:- Coming
 
:- Coming

Revision as of 14:26, 18 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

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
- LST+MAGIC
- MAGIC

Monte Carlo Data

- To be completed

Analysis webpages

Mono-LST-1

-RF improvement

Stereo LST-1+MAGIC

-Standard analysis check

Main results

- Coming

Internal group meetings

- 11-05-2023


External presentations

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

Conferences

- Coming