UCAC4 297-064700 , the SIMBAD biblio

We have developed a new method of multiwavelength data combination for the search of late-type radio dwarfs, and have put it into practice using GLEAM-X DR1 data. The initial sample is selected by cross-matching the Gaia/DR3 objects with the probability of being a star no less than 99%, and removing the extragalactic objects assigned by the SIMBAD database. The late-type dwarf stars are judged according to their location in the (BP - RP)₀/M_G color-magnitude diagram and in the (J - H)₀/(K - W1)₀ near-infrared color-color diagram. Furthermore, stellar activity is searched by ultraviolet excess in the GALEX/NUV band and the Rossby number in the TESS light curves. In total, 12 stars are found to be late-type dwarf stars associated with radio source, which consists of five stars with UV excess and seven stars with a Rossby number less than 0.13. Three of these 12 stars are previously studied to be associated with radio objects. All these 12 stars are considered to be reliable counterparts of radio sources.