Difference between revisions of "MAGIC priority proposals for joint observations"
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=Cycle II= | =Cycle II= | ||
+ | * APFP01 - Testing propagation of VHE photons in a gravitational field with the gravitationally lensed blazar B0218+357. | ||
+ | * GAL05 - The periastron passage of the colliding wind binary WR140: the first CWB VHE emitter in the Northern hemisphere? | ||
+ | * GAL06 - Multi-wavelength Campaign of the Impending Historic Recurrent Nova -- T Coronae Borealis | ||
+ | * GAL09 - Large Zenith Angle observation of the hadronic PeVatron candidate in the Boomerang SNR (G106.3+2.7) with MAGIC and LST-1 | ||
+ | * GAL13 - The 1LHAASO J0007+7303u PeVatron candidate: solving the CTA 1 conundrum with MAGIC and LST1 | ||
+ | * GAL15 - HESS J1848-018: a stellar cluster PeVatron? | ||
+ | * TECH01 - Benchmark observations with MAGIC and LST-1 | ||
+ | * TECH02 - Technical observations to optimize and monitor the performance of the MAGIC telescopes | ||
+ | * TRAN03 - Multi-wavelength observations of repeating fast radio bursts | ||
+ | * TRAN04 - Gamma-ray bursts observations with MAGIC | ||
+ | * AGN03 - Long-term monitoring program of radio galaxies | ||
+ | * AGN04 - Highly bent radio-galaxies as potential sources of VHE gamma rays | ||
+ | |||
+ | This results in 526.75 hours including both regular and ToO time. | ||
=Cycle I= | =Cycle I= | ||
+ | |||
+ | * GAL01 - Long-term monitoring of the binary system LS I +61 303 | ||
+ | * GAL03 - Multi-wavelength Campaign of the Historic Recurrent Nova - T Coronae Borealis | ||
+ | * GAL06 - Observation of the Cygnus-x North star- forming complex: unveiling the nature of the Cygnus OB2 star cluster as a cosmic- ray accelerator (continued) | ||
+ | * GAL08 - Galactic Targets of Opportunity | ||
+ | * GAL11 - Identifying the counterpart of the PeVatron candidate LHAASO J1956+2845 | ||
+ | * TECH01 - Technical observations to optimize and monitor the performance of the MAGIC telescopes | ||
+ | * TRAN04 - Gamma-ray burst observations with MAGIC | ||
+ | * AGN04 - Monitoring of classical radio galaxies | ||
+ | * AGN10 - IGMF measurement with joint MAGIC+LST1 observations of 1ES 0229+200 | ||
+ | * AGN17 - ToO observations of flaring AGNs based on optical, X-ray and gamma-ray triggers (MTOO) | ||
+ | |||
+ | This results in ~ 530 hours including both regular and ToO time. |
Revision as of 07:49, 2 April 2024
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In this page, the MAGIC proposals that were given priority by the LST LPPB are listed, for each observation cycle.
Cycle II
- APFP01 - Testing propagation of VHE photons in a gravitational field with the gravitationally lensed blazar B0218+357.
- GAL05 - The periastron passage of the colliding wind binary WR140: the first CWB VHE emitter in the Northern hemisphere?
- GAL06 - Multi-wavelength Campaign of the Impending Historic Recurrent Nova -- T Coronae Borealis
- GAL09 - Large Zenith Angle observation of the hadronic PeVatron candidate in the Boomerang SNR (G106.3+2.7) with MAGIC and LST-1
- GAL13 - The 1LHAASO J0007+7303u PeVatron candidate: solving the CTA 1 conundrum with MAGIC and LST1
- GAL15 - HESS J1848-018: a stellar cluster PeVatron?
- TECH01 - Benchmark observations with MAGIC and LST-1
- TECH02 - Technical observations to optimize and monitor the performance of the MAGIC telescopes
- TRAN03 - Multi-wavelength observations of repeating fast radio bursts
- TRAN04 - Gamma-ray bursts observations with MAGIC
- AGN03 - Long-term monitoring program of radio galaxies
- AGN04 - Highly bent radio-galaxies as potential sources of VHE gamma rays
This results in 526.75 hours including both regular and ToO time.
Cycle I
- GAL01 - Long-term monitoring of the binary system LS I +61 303
- GAL03 - Multi-wavelength Campaign of the Historic Recurrent Nova - T Coronae Borealis
- GAL06 - Observation of the Cygnus-x North star- forming complex: unveiling the nature of the Cygnus OB2 star cluster as a cosmic- ray accelerator (continued)
- GAL08 - Galactic Targets of Opportunity
- GAL11 - Identifying the counterpart of the PeVatron candidate LHAASO J1956+2845
- TECH01 - Technical observations to optimize and monitor the performance of the MAGIC telescopes
- TRAN04 - Gamma-ray burst observations with MAGIC
- AGN04 - Monitoring of classical radio galaxies
- AGN10 - IGMF measurement with joint MAGIC+LST1 observations of 1ES 0229+200
- AGN17 - ToO observations of flaring AGNs based on optical, X-ray and gamma-ray triggers (MTOO)
This results in ~ 530 hours including both regular and ToO time.