We present the analysis of deep HST multi-band imaging of the BDF field specifically designed to identify faint companions around two of the few Ly-alpha emitting galaxies spectroscopically confirmed at z~7 (Vanzella et al. 2011). Although separated by only 4.4 proper Mpc these galaxies cannot generate HII regions large enough to explain visibility of their Ly-alpha line, thus requiring a population of fainter ionizing sources in their vicinity. We use deep HST and VLT-Hawk-I data to select z~7 Lyman break galaxies around the emitters. We select 6 new robust z~7 LBGs at Y~26.5-27.5 whose average spectral energy distribution is consistent with the objects being at the redshift of the close-by Ly-alpha emitters. The resulting number density of z~7 LBGs in the BDF field is a factor ~3-4 higher than expected in random pointings of the same size. We compare these findings with cosmological hydrodynamic plus radiative transfer simulations of a universe with a half neutral IGM: we find that indeed Ly-alpha emitter pairs are only found in completely ionized regions characterized by significant LBG overdensities. Our findings match the theoretical prediction that the first ionization fronts are generated within significant galaxy overdensities and support a scenario where faint, "normal" star-forming galaxies are responsible for reionization.
@article{arxiv.1601.03442,
title = {First observational support for overlapping reionized bubbles generated by a galaxy overdensity},
author = {M. Castellano and P. Dayal and L. Pentericci and A. Fontana and A. Hutter and G. Brammer and E. Merlin and A. Grazian and S. Pilo and R. Amorin and S. Cristiani and M. Dickinson and A. Ferrara and S. Gallerani and E. Giallongo and M. Giavalisco and L. Guaita and A. Koekemoer and R. Maiolino and D. Paris and P. Santini and L. Vallini and E. Vanzella and J. Wagg},
journal= {arXiv preprint arXiv:1601.03442},
year = {2016}
}
Comments
Accepted for publication in The Astrophysical Journal Letters. 6 pages, 5 figures