Clumpy Galaxies in CANDELS. II. Physical Properties of UV-bright Clumps at 0.5 ≤ z < 3 - Guo, Yicheng; Rafelski, Marc; Bell, Eric F.; Conselice, Christopher J.; Dekel, Avishai; Faber, S. M.; Giavalisco, Mauro; Koekemoer, Anton M.; Koo, David C.; Lu, Yu; Mandelker, Nir; Primack, Joel R.; et al. (The Astrophysical journal, 2018)
Keywords: Astronomical models; Astrophysics; Clumps; Color; Computer simulation; Fluxes; Galactic evolution; Galaxies; galaxies: evolution; galaxies: formation; galaxies: star formation; galaxies: starburst; galaxies: structure; Giant stars; Image detection; Physical properties; Red shift; Slope gradients; Slopes; Spectral energy distribution; Star & galaxy formation; Star formation; Star formation rate; Stars & galaxies; Stellar age; Stellar mass; Stellar models; Subtraction; ultraviolet: galaxies