Normalized transmission curves of filters (convolved with the instrument/telescope sensitivities) used in our study. In total, we have 50 filters including 21 optical (includes the two UV filters) and 29 IR filters. For each dataset, the filters are color coded from shorter (blueish) to longer (reddish) wavelengths. Left panel from top to bottom: BP, RP, and G from Gaia, U, B, V, and R from M2002, u, v, g, r, i, and z from SkyMapper, and u, g, r, i, z, and Y from NSC. Middle panel from top to bottom: J, H, K_S from 2MASS, Y, J, K_S from VMC, J, H, K_S from IRSF, and FUV and NUV from GALEX. Right panel from top to bottom: IRAC1, IRAC2, IRAC3, IRAC4, and MIPS24 from Spitzer, WISE1, WISE2, WISE3, and WISE4 from WISE, N3, N4, S7, S11, L15, and L24 from AKARI, and MIPS70 (from Spitzer), PACS100, PACS160, SPIRE250, and SPIRE350 from Herschel.