A High Space Density of Luminous Lyα Emitters at z ∼ 6.5
Document Type
Article
Publication Date
2-27-2017
Abstract
We present the results of a systematic search for Lyα emitters (LAEs) at using the HST WFC3 Infrared Spectroscopic Parallel (WISP) Survey. Our total volume over this redshift range is Mpc3, 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 erg s−1, 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 Mpc−3. 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.
Department
Physics and Astronomy
Print ISSN
0004-637X
Online ISSN
1538-4357
Publication Title
The Astrophysical Journal
Recommended Citation
Bagley, M., Scarlata, C., Henry, A., Rafelski, M., Malkan, M., Teplitz, H., Dai, Y. S., Baronchelli, I., Colbert, J., Rutkowski, M. J., Mehta, V., Dressler, A., McCarthy, P., Bunker, A., Atek, H., Garel, T., Martin C. L, Hathi, N,., & Siana, B. (2017). A high space density of luminous Lyα emitters at z ∼ 6.5. The Astrophysical Journal, 837(1), Article 11. https://doi.org/10.3847/1538-4357/837/1/11
DOI
10.3847/1538-4357/837/1/11
Link to Publisher Version (DOI)
Publisher's Copyright and Source
Copyright © 2017. The American Astronomical Society. All rights reserved.