Difference between revisions of "Boomerang SNR"
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* Marine Pihet | * Marine Pihet | ||
* Takayuki Saito (co-PI) | * Takayuki Saito (co-PI) | ||
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== Data available == | == Data available == | ||
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| − | + | * [[Mono-LST]] | |
| + | * [[LST+MAGIC]] | ||
| + | * [[MAGIC]] | ||
== Monte Carlo Data == | == Monte Carlo Data == | ||
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*[[RF improvement]] | *[[RF improvement]] | ||
=== Stereo LST-1+MAGIC === | === Stereo LST-1+MAGIC === | ||
| − | *[[Standard analysis check]] | + | *[[Standard analysis check ]] |
| − | == | + | == Main results == |
| + | ::- To be completed | ||
== Internal group meetings == | == Internal group meetings == | ||
Revision as of 12:58, 18 May 2023
Contents
Boomerang SNR spectral and morphological study
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
- Proposals:
- - "Large Zenith Angle observation of the hadronic PeVatron candidate in the Boomerang SNR (G106.3+2.7) with MAGIC and LST-1" MAGIC Cycle 18 (GAL 346)
- - "Large Zenith Angle observation of the hadronic PeVatron candidate in the Boomerang SNR (G106.3+2.7) with LST-1" LST Cycle 1 (GAL07)
- Reference coordinated:
- - MAGIC Tail: RA, Dec (ICRS): 36.72 deg, 60.84 deg
- - MAGIC head: RA, Dec (ICRS): 337.13 deg, 61.10 deg
People involved
- Franca Cassol (PI)
- Heide Costantini
- Gabriel Emery
- Marie-Sophie Carrasco
- Marine Pihet
- Takayuki Saito (co-PI)
Proposals
Data available
Monte Carlo Data
- - To be completed
Analysis
Mono-LST-1
Stereo LST-1+MAGIC
Main results
- - To be completed
Internal group meetings
- -
Presentations
- -
