Infrared Confirmation of z> 5.5 Quasar Candidates

Details Infrared Confirmation of z> 5.5 Quasar Candidates Infrared Confirmation of z> 5.5 Quasar Candidates

Aug 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002noao.prop..292h&link_type=abstract

NOAO Proposal ID #2002B-0292

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Scientific paper

A Gunn-Peterson trough (neutral hydrogen absorption) has been discovered in the spectrum of a z=6.28 quasar from the Sloan Digital Sky Survey. The lack of such troughs in the four other known z> 5.5 quasars suggests that z~6 could be the tail end of the reionization epoch, when the spheres of ionized hydrogen around quasars and star- forming galaxies finally overlap. To better determine the timescale over which reionization occurred - and how the distribution of neutral hydrogen evolved during that epoch - requires more quasars at z> 5.5. We have in hand 90 deg^2 of CFHT and CTIO Rz imaging which enables us to select candidate z> 5.5 quasars and L/T type stars and brown dwarfs as objects with very red (R-z)_AB colors. Here we propose KPNO near-IR imaging to efficiently and accurately separate the quasars among our equatorial and northern candidates from the more numerous L and T dwarfs %class stars and brown dwarfs (which are scientifically interesting in their own right). Our survey reaches two magnitudes fainter than the SDSS, providing a tighter constraint on the quasar contribution to the UV flux needed for reionization (and enabling the discovery of more distant L and T dwarfs). The surface density of z> 5.5 quasars is estimated to be 0.1 deg^-2 %unknown in the 20< z_AB< 22 magnitude range of our survey, but could be as high as 1 deg^-2.

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