1. Utilize the small radio telescope array to survey for fast radio bursts (FRBs) in magnetars, high magnetic field neutron stars, globular clusters, and nearby galaxies. Conduct long-term monitoring of known repeating FRBs to build observational datasets and support future array construction.

2. With the array’s gradual expansion, further investigate scientific targets by combining observations with the Five-hundred-meter Aperture Spherical radio Telescope (FAST) to localize repeating FRBs, while initiating radio studies of exoplanets and other transients.

3. Establish a dedicated FRB research team to systematize long-term monitoring, data processing, and analysis. Regularly observe exoplanetary systems to extract time-domain information, estimate emission region properties, and explore potential links between radio bursts and planets. Promote coordinated multi-band observations of transient sources.

4. Actively engage in major national programs, including deep space exploration, autonomous pulsar navigation, microwave sky surveys, aerospace, and defense applications.