Primordial environment of supermassive black holes - II. Deep Y- and J-band images around the z?~?6.3 quasar SDSS J1030+0524

摘要

Many cosmological studies predict that early supermassive black holes (SMBHs) can only form in the most massive dark matter halos embedded within large-scale structures marked by galaxy overdensities that may extend up to ~ 10 physical Mpc. This scenario, however, has not been confirmed observationally, as the search for galaxy overdensities around high- z quasars has returned conflicting results. The field around the z = 6.31 quasar SDSSJ1030+0524 (J1030) is unique for multi-band coverage and represents an excellent data legacy for studying the environment around a primordial SMBH. In this paper we present wide-area ( ~ 25′ × 25′ ) Y - and J -band imaging of the J1030 field obtained with the near infrared camera WIRCam at the Canada-France-Hawaii Telescope (CFHT). We built source catalogs in the Y - and J -band, and matched those with our photometric catalog in the r , z , and i bands presented in our previous paper and based on sources with z _(AB)& 25.2 detected using z -band images from the the Large Binocular Cameras (LBC) at the Large Binocular Telescope (LBT) over the same field of view. We used these new infrared data together with H and K photometric measurements from the MUlti-wavelength Survey by Yale-Chile (MUSYC) and with the Spitzer Infrared Array Camera (IRAC) data to refine our selection of Lyman break galaxies (LBGs), extending our selection criteria to galaxies in the range 25.2 & z _(AB)& 25.7 . We selected 21 robust high redshift candidates in the J1030 field with photometric redshift z ~ 6 and colors i ? z ≥ 1.3 . We found a significant asymmetry in the distribution of the high redshift galaxies in J1030, supporting the existence of a coherent large-scale structure around the quasar. We estimated an overdensity of z ~ 6 galaxies in the field of δ = 2.4 , which is significant at & 4 σ . The overdensity value and its significance are higher than those found in our previous paper and we interpret this as evidence of an improved LBG selection.