Comparison of the results of this work with the results obtained by Khan et al. (2019) for the solar-like oscillating giants in the Kepler field and the K2 C3 and C6 fields. The surface gravities were obtained from the ν_max scaling relation, while the distances and extinctions were computed with PARAM (Rodrigues et al. 2017), using the seismic parameters Δν, ν_max, as well as spectroscopic (Kepler) or photometric (K2 effective temperatures and metallicities as an input.