http://arxiv.org/abs/1806.08798
We use deep F275W imaging from the $Hubble$ Deep UV Legacy Survey (HDUV) and G280 grism spectroscopy from $HST$/WFC3, along with new and archival optical spectra from Keck/DEIMOS, to search for candidate ionizing sources in the GOODS-N field at z ~ 2.5 – 3. Spectroscopic identification of our UV-selected sources are 99% complete to F275W = 25.5 in the region of the UV imaging, and we identify 6 potential ionizing galaxies or AGNs at z ~ 3. By far the brightest of these is a z = 2.583 AGN that totally dominates the ionizing flux in the region, with a specific ionizing volume emissivity at $912~ \AA$ of $\epsilon_{912}$ = $8.3^{27}{1.4} \times 10^{24}$ erg s$^{-1}$ Hz$^{-1}$ Mpc$^{-3}$. Based on our spectroscopic data, we find four candidates are contaminated by foreground galaxies at z ~ 0.5 – 0.7. At $\epsilon{912}$ = $2.2^{7.2}_{0.4} \times 10^{23}$ erg s$^{-1}$ Hz$^{-1}$ Mpc$^{-3}$, the remaining candidate galaxy’s contribution to the ionizing background lies well below the flux required to ionize the intergalactic medium at z ~ 2.5 – 3, consistent with previous observations that show AGNs provide the bulk of the ionizing background at these redshifts.
L. Jones, A. Barger, L. Cowie, et. al.
Tue, 26 Jun 18
67/71
Comments: 14 pages, 11 figures. Accepted for publication in ApJ