While radio, optical, and IR observations would be coordinated through ground-based telescopes, the high energy regions, i.e., UV, X-ray and visible wavelength, would be covered by the dedicated satellite-borne instrumentation of Astrosat.
The coordination of radio, optical, and infrared observations will occur through ground-based telescopes. In contrast, the high-energy spectrum, including UV, X-rays, and visible light, will be monitored using the specialized space-based equipment of Astrosat.