Difference between revisions of "Boomerang SNR"
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== Proposals== | == Proposals== | ||
− | * [MAGIC Cycle XVII | + | * [[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) |
− | |||
== Conferences == | == Conferences == | ||
:- Coming | :- Coming |
Revision as of 14:26, 18 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
- File:MAGIC Cycle18 draft GAL00346 Cassol.pdf 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:
Monte Carlo Data
- - To be completed
Analysis webpages
Mono-LST-1
Stereo LST-1+MAGIC
Main results
- - Coming
Internal group meetings
External presentations
- - 27-03-2023: Random Forest optimization for LZA observations¶ (M. Carrasco, LST analysis meeting)
Conferences
- - Coming