Difference between revisions of "Boomerang SNR"
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== Monte Carlo Data == | == Monte Carlo Data == | ||
| − | [[File:Produced_node_in_line_May_2023.png|thumb| | + | [[File:Produced_node_in_line_May_2023.png|thumb|150px|]] |
| − | [[File:Produced_nodes_in_dec_line_above_55_deg.png|thumb| | + | [[File:Produced_nodes_in_dec_line_above_55_deg.png|thumb|150px|]] |
Monte Carlo data have been produced with successive productions in order to increase the node density. | Monte Carlo data have been produced with successive productions in order to increase the node density. | ||
:- First production has been performed standardly with uniform training nodes on the declination line | :- First production has been performed standardly with uniform training nodes on the declination line | ||
:- Second production has been performed asking a node with with step cos(zenith)=0.04, for zenith angles > 60 deg [https://github.com/cta-observatory/lst-sim-config/issues/50 (see here)] | :- Second production has been performed asking a node with with step cos(zenith)=0.04, for zenith angles > 60 deg [https://github.com/cta-observatory/lst-sim-config/issues/50 (see here)] | ||
:- Third production has been performed in order to further increase the node density with step cos(zenith)=0.02, for zenith angles > 60 deg [https://github.com/cta-observatory/lst-sim-config/issues/53 (see here)] | :- Third production has been performed in order to further increase the node density with step cos(zenith)=0.02, for zenith angles > 60 deg [https://github.com/cta-observatory/lst-sim-config/issues/53 (see here)] | ||
| − | We asked also to have test nodes on the declination line. The figures | + | We asked also to have test nodes on the declination line. The figures show the present simulated nodes, to be found in |
:- /fefs/aswg/data/mc/DL0/LSTProd2/TrainingDataset/Protons/dec_6166 | :- /fefs/aswg/data/mc/DL0/LSTProd2/TrainingDataset/Protons/dec_6166 | ||
:- /fefs/aswg/data/mc/DL0/LSTProd2/TrainingDataset/GammaDiffuse/dec_6166 | :- /fefs/aswg/data/mc/DL0/LSTProd2/TrainingDataset/GammaDiffuse/dec_6166 | ||
Revision as of 09:12, 30 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
Monte Carlo data have been produced with successive productions in order to increase the node density.
- - First production has been performed standardly with uniform training nodes on the declination line
- - Second production has been performed asking a node with with step cos(zenith)=0.04, for zenith angles > 60 deg (see here)
- - Third production has been performed in order to further increase the node density with step cos(zenith)=0.02, for zenith angles > 60 deg (see here)
We asked also to have test nodes on the declination line. The figures show the present simulated nodes, to be found in
- - /fefs/aswg/data/mc/DL0/LSTProd2/TrainingDataset/Protons/dec_6166
- - /fefs/aswg/data/mc/DL0/LSTProd2/TrainingDataset/GammaDiffuse/dec_6166
- - /fefs/aswg/data/mc/DL0/LSTProd2/TestDataset
Analysis webpages
Mono-LST-1
Stereo LST-1+MAGIC
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
