Difference between revisions of "Boomerang SNR"
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== Analysis webpages == | == Analysis webpages == | ||
==== Mono-LST-1 ==== | ==== Mono-LST-1 ==== | ||
| − | :-[[ | + | :-[[Data selection]] |
| + | :-[[Data-MC comparison]] | ||
| + | :-[[DL3 analysis]] | ||
==== Stereo LST-1+MAGIC ==== | ==== Stereo LST-1+MAGIC ==== | ||
| − | :-[[ | + | |
| + | :-[[Data-selection]] | ||
| + | :-[[Data-MC comparison]] | ||
| + | :-[[DL3 analysis]] | ||
| + | ==== MAGIC Only data ==== | ||
| + | :-[[Data-selection]] | ||
| + | :-[[Data-MC comparison]] | ||
| + | :-[[DL3 analysis]] | ||
| + | ==== Joint high level analysis ==== | ||
| + | :- Coming | ||
== Main results == | == Main results == | ||
Revision as of 10:30, 4 July 2024
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
- Cornelia Arcaro
- Ali Baktash
- Marie-Sophie Carrasco
- Franca Cassol (PI)
- Yating Chai
- Heide Costantini
- Gabriel Emery
- 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. We asked also to have test nodes on the declination line. The figures show the present simulated nodes, to be found in
1- First production has been performed standardly with uniform training nodes on the declination line
2- Second production has been performed asking a node with with step cos(zenith)=0.04, for zenith angles > 60 deg (see here)
3- 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)
- - /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
4- Fourth production is based on the concept of a very dense simulation line but each node having a low statistics (see here). The idea and method have been presented in several talks (see below)
- - /fefs/aswg/data/mc/DL0/LSTProd2/TrainingDataset/Protons/dec_6166_high_density
- - /fefs/aswg/data/mc/DL0/LSTProd2/TrainingDataset/GammaDiffuse/dec_6166_high_density
The new RFs and DL2 data are in:
- - Model: /fefs/aswg/data/models/AllSky/20240519_v0.10.11_src4_dense_MC_line/dec_6166_high_density/
- - DL2 test gammas : /fefs/aswg/data/mc/DL2/AllSky/20240519_v0.10.11_src4_dense_MC_line/TestingDataset/dec_6166_high_density/
We these new RFs we have reconstruct the old MC line in order to have protons and diffuse gamma as tests:
- - Diffuse gamma :
- - Protons :
Analysis webpages
Mono-LST-1
Stereo LST-1+MAGIC
MAGIC Only data
Joint high level analysis
- - Coming
Main results
- - Coming
Internal group meetings
External presentations
- - 27-03-2023: Random Forest optimization for LZA observations¶ (M. Carrasco, LST analysis meeting)
- - 15-01-2024: Science with LST : the puzzling case of the Boomerang SNR (F. Cassol, 1st VHEGAM meeting)
Meetings on the Background Model estimation (GAL Center and Boomerang groups joint activity)
- - 18-10-2023
- - 02-11-2023
- - 22-11-2023 (coming meeting)
