New improved photometric redshifts of galaxies in the Hubble Deep Field

We report new improved photometric redshifts of 1048 galaxies in the Hubble Deep Field. A standard chi(2) minimizing method is applied to recent seven -color UBVIJHK photometry by Fernandez-Soto et al. We use 187 template spec tral energy distributions (SEDs) representing a wide variety of morphology and age of observed galaxies based on a population synthesis model by Kodam a & Arimoto. We introduce two new recipes. First, the amount of the interna l absorption is changed as a free parameter in the range E(B-V) = 0.0-0.5 w ith an interval of 0.1. Second, the absorption due to intergalactic H I clo uds is also changed by a factor of 0.5, 1.0, and 1.5 around the opacity giv en by Madau, The total number of template SEDs is thus 187 x 6 x 3 = 3366, except for the redshift grid. The dispersion sigma(z) of our photometric re dshifts with respect to spectroscopic redshifts is sigma(z) = 0.08 and 0.24 for z < 2 and z > 2, respectively, which are smaller than the correspondin g values (sigma(z) = 0.09 and 0.45) by Fernandez-Soto et al. Improvement is significant, especially in z > 2. This is due to smaller systematic errors which are largely reduced mainly by including three opacities due to inter galactic H I clouds. We discuss redshift distribution N(z) and cosmic star formation rate based on our new photometric redshifts.