A High Space Density of Luminous Ly α Emitters at $z\sim 6.5$

Citation data:

The Astrophysical Journal, ISSN: 1538-4357, Vol: 837, Issue: 1

Publication Year:
2017
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DOI:
10.3847/1538-4357/837/1/11
Author(s):
Micaela B. Bagley, Claudia Scarlata, Alaina Henry, Marc Rafelski, Matthew Malkan, Harry Teplitz, Y. Sophia Dai, Ivano Baronchelli, James Colbert, Michael Rutkowski, Vihang Mehta, Alan Dressler, Patrick McCarthy, Andrew Bunker, Hakim Atek, Thibault Garel, Crystal L. Martin, Nimish Hathi, Brian Siana Show More Hide
Publisher(s):
American Astronomical Society
Tags:
Physics and Astronomy, Earth and Planetary Sciences
article description
We present the results of a systematic search for Lyα emitters (LAEs) at 6 ≲ z ≲ 7.6 using the HST WFC3 Infrared Spectroscopic Parallel (WISP) Survey. Our total volume over this redshift range is ∼8 × 10Mpc, comparable to many of the narrowband surveys despite their larger area coverage. We find two LAEs at z = 6.38 and 6.44 with line luminosities of L∼ 4.7 × 10erg s, putting them among the brightest LAEs discovered at these redshifts. Taking advantage of the broad spectral coverage of WISP, we are able to rule out almost all lower-redshift contaminants. The WISP LAEs have a high number density of 7.7 × 10Mpc. We argue that the LAEs reside in megaparsec-scale ionized bubbles that allow the Lyα photons to redshift out of resonance before encountering the neutral intergalactic medium. We discuss possible ionizing sources and conclude that the observed LAEs alone are not sufficient to ionize the bubbles.

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