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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. - Category A
GAL05 - The periastron passage of the colliding wind binary WR140: the first CWB VHE emitter in the Northern hemisphere? - Category C
GAL06 - Multi-wavelength Campaign of the Impending Historic Recurrent Nova -- T Coronae Borealis - Category A
GAL09 - Large Zenith Angle observation of the hadronic PeVatron candidate in the Boomerang SNR (G106.3+2.7) with MAGIC and LST-1 - Category B
GAL13 - The 1LHAASO J0007+7303u PeVatron candidate: solving the CTA 1 conundrum with MAGIC and LST1 - Category A
GAL15 - HESS J1848-018: a stellar cluster PeVatron? - Category C
TECH01 - Benchmark observations with MAGIC and LST-1 - Category A
TECH02 - Technical observations to optimize and monitor the performance of the MAGIC telescopes - Category A
TRAN03 - Multi-wavelength observations of repeating fast radio bursts - Category B
TRAN04 - Gamma-ray bursts observations with MAGIC - Category A
AGN03 - Long-term monitoring program of radio galaxies - Category C
AGN04 - Highly bent radio-galaxies as potential sources of VHE gamma rays - Category B

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.