Notes. Columns 1–5 correspond to the Galactic name, Galactic longitude ℓ and latitude b, and the right ascension (RA) and declination (Dec) of the GLOSTAR sources. Columns 6 and 7 list the peak flux densities and the errors from GLOSTAR (S_peakG ± dS) and CORNISH (S_peakC ± dS) under the same beam size of 1.5″. Sources with θ_S > 1.5″ (i.e., the beam size) in Column 8 are considered resolved, and their deconvolved sizes θ_dcon are determined in Column 9. Sources with θ_S ≤ 1.5″ (i.e., the beam size) are considered unresolved, and their θ_dcon and diam are considered the upper limit values (flagged with a star ⋆ in Column 1), and the upper limit of θ_dcon is set to be $0_{\cdot }^{\mathrm{\prime }\mathrm{\prime }}32$, which corresponds to one standard deviation of the distribution of beam sizes from the CORNISH survey (Purcell et al. 2013). Column 12 gives the variation fraction, as outlined in Sect. 3. The spectral indices α and their errors dα are listed in Column 13. The symbol “−” in Column 13 means that the α is unreliable. Only the Top7 variables are provided here. The full table of the 38 variables is available in electronic form at CDS.