Difference between revisions of "Boomerang SNR"
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| + | '''Back to [[Data_analysis|Data Analysis]]''' <br> | ||
==General information== | ==General information== | ||
[[Image:Boomerang_SNR_Magic.png|thumb|right|350px|The Boomerang SNR as seen by MAGIC [A&A 658, A60 (2022)]]] | [[Image:Boomerang_SNR_Magic.png|thumb|right|350px|The Boomerang SNR as seen by MAGIC [A&A 658, A60 (2022)]]] | ||
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* '''Name of the source''': SNR 106.3+2.7 | * '''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 | * '''Brief description of the source''': Strong hadronic PeVatron candidate with TeV emission both from the head and the tail of the SNR | ||
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* ''' Reference coordinated''': | * ''' Reference coordinated''': | ||
::- MAGIC Tail: RA, Dec (ICRS): 36.72 deg, 60.84 deg | ::- MAGIC Tail: RA, Dec (ICRS): 36.72 deg, 60.84 deg | ||
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| + | == Proposals== | ||
| + | * [MAGIC Cycle XVII] (GAL 346) | ||
| + | * [LST Cycle I] (GAL 07) | ||
==People involved == | ==People involved == | ||
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* Marine Pihet | * Marine Pihet | ||
* Takayuki Saito (co-PI) | * Takayuki Saito (co-PI) | ||
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== Data available == | == Data available == | ||
| − | + | There are three set of data: | |
| − | + | :- [[Mono-LST]] | |
| − | + | :- [[LST+MAGIC]] | |
| − | + | :- [[MAGIC]] | |
== Monte Carlo Data == | == Monte Carlo Data == | ||
| − | + | :- To be completed | |
| − | == Analysis == | + | == Analysis webpages == |
=== Mono-LST-1 === | === Mono-LST-1 === | ||
| − | + | :-[[RF improvement]] | |
=== Stereo LST-1+MAGIC === | === Stereo LST-1+MAGIC === | ||
| − | + | :-[[Standard analysis check ]] | |
== Main results == | == Main results == | ||
| − | + | :- Coming | |
== Internal group meetings == | == Internal group meetings == | ||
| − | ::- | + | :- [[11-05-2023]] |
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| + | == External presentations == | ||
| + | :- 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 == |
| − | + | :- Coming | |
Revision as of 13:50, 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
- [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
Random Forest optimization for LZA observations] (M. Carrasco, LST analysis meeting)
Conferences
- - Coming
