Surveying the Post-Reionization Universe with Quasar Spectroscopy III

Details Surveying the Post-Reionization Universe with Quasar Spectroscopy III Surveying the Post-Reionization Universe with Quasar Spectroscopy III

Feb 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011noao.prop..262w&link_type=abstract

NOAO Proposal ID #2011A-0262

Computer Science

Scientific paper

We propose to obtain GMOS-N spectroscopy of 33 quasars as part of a multi-semester endeavor to study the z>4.4 IGM with Gemini (a related 2011A GMOS-S proposal is submitted). This request completes our 3-semester program that will ultimately provide 160 R 850 spectra of z>4.4 quasars, the largest homogeneous sample of science-grade high-redshift quasar spectra in existence. This sample will yield the first statistically meaningful measurements of the neutral gas content, the number density of optically thick absorbers, and the mean hydrogen absorption at z>4.5. In particular, spectral stacks will enable the first direct measurement of the mean free path to ionizing radiation at these redshifts, and probe its expected strong evolution near the epoch of reionization. This novel route to constrain reionization with the Lyman forest requires a large, homogeneous sample of higher-quality spectra than provided by SDSS. Gemini/GMOS can efficiently supply these data, which we will publicly release in reduced form. They will also permit (i) an unparalleled survey for damped Lya and Lyman limit systems at z>4.5; (ii) constraints on the mean opacity of Lyman series transitions; and (iii) a survey for variable emission/absorption in quasar spectra.

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