Difference between revisions of "MAGIC priority proposals for joint observations"

From my_wiki
Jump to: navigation, search
(Create page.)
 
m (Add priority proposals)
Line 5: Line 5:
 
=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

Back to Main page

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.