Difference between revisions of "Boomerang SNR"

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(Internal group meetings)
(Internal group meetings)
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== Internal group meetings ==
 
== Internal group meetings ==
* 11-05-2023:
+
:-[[2023]]
:- [https://www.lst1.iac.es/wiki/index.php/File:G106_organisation_11_5_2023.pdf Activities on Boomerang] (F. Cassol)
 
* 23-05-2023:
 
:- [https://www.lst1.iac.es/wiki/index.php/File:20230523_GroupMeeting_Carrasco.pdf Work update] (MS. Carrasco)
 
  
 
== External presentations ==
 
== External presentations ==

Revision as of 15:29, 23 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

- To be completed

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