Difference between revisions of "Boomerang SNR"
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* 11-05-2023: | * 11-05-2023: | ||
:- [https://www.lst1.iac.es/wiki/index.php/File:G106_organisation_11_5_2023.pdf Activities on Boomerang] (F. Cassol) | :- [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 Activities on Boomerang] (MS. Carrasco) | ||
== External presentations == | == External presentations == | ||
Revision as of 13:49, 23 May 2023
Back to Data Analysis
General information
- 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
Stereo LST-1+MAGIC
Main results
- - Coming
Internal group meetings
- 11-05-2023:
- - Activities on Boomerang (F. Cassol)
- 23-05-2023:
- - Activities on Boomerang (MS. Carrasco)
External presentations
- - 27-03-2023: Random Forest optimization for LZA observations¶ (M. Carrasco, LST analysis meeting)
Conferences
- - Coming
