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Using the Subaru very deep K'-band imaging and HST WFPC2/NICMOS archival dataof the Hubble Deep Field North, we investigate the evolution of the stellarmass, color, morphology of galaxies to z ~ 3. We mainly examine the rest-frameU-V color distribution of galaxies as a function of stellar mass. At 0.3<z<2,galaxies seem to be divided into the two populations at around the stellar massof ~5x10^9 M_solar. The low-mass galaxies have relatively bluer rest U-V colorand their color does not show clear correlation with stellar mass over therange of 10^8-5x10^9 M_solar. On the other hand, at higher mass, the moremassive galaxies tend to have the redder U-V color. The average U-V color ofthe low-mass galaxies becomes bluer gradually with redshift, from U-V ~ 0.2 atz ~ 0.5 to U-V ~ -0.2 at z ~ 2. On the contrary, the correlation between thestellar mass and rest U-V color of the high-mass population does not seem tochange significantly between z ~ 0.3 and z ~ 2. At z>2, it is seen that moremassive galaxies tend to have redder U-V color over the range of 10^9-10^10M_solar. These results suggests that the star formation history of galaxiesdepends on their stellar mass very much. The low-mass population is likely tohave relatively long star formation timescale. At the stellar mass larger than~5x10^9 M_solar, there must be some mechanisms which suppress the starformation in galaxies at 0<z<2.Comment: 45 pages, 31 figures, accepted for publication in Ap

Evolution of the Dependence of Rest‐Frame Color and Morphology Distribution on Stellar Mass for Galaxies in the Hubble Deep Field–North