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.
Radio, optical, and IR observations will be conducted via ground-based telescopes. Conversely, the high-energy range, encompassing UV, X-rays, and visible wavelengths, will be investigated through the satellite-borne equipment of Astrosat.