The detection of photons sufficiently energetic to ionize neutral hydrogen, coming from a compact, star-forming galaxy, offers clues to how the first generation of galaxies may have reionized hydrogen gas in the early Universe. See Letter p.178
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References
Izotov, Y. I. et al. Nature 529, 178–180 (2016).
Planck Collaboration. Astron. Astrophys. 571, A16 (2014).
Fan, X., Carilli, C. L. & Keating, B. Annu. Rev. Astron. Astrophys. 44, 415–462 (2006).
Robertson, B. E. et al. Astrophys. J. 768, 71 (2013).
Steidel, C. S., Pettini, M. & Adelberger, K. L. Astrophys. J. 546, 665–671 (2001).
Vanzella, E. et al. Astrophys. J. 751, 70 (2012).
Bergvall, N. et al. Astron. Astrophys. 448, 513–524 (2006).
Leitet, E., Bergvall, N., Hayes, M., Linné, S. & Zackrisson, E. Astron. Astrophys. 553, A106 (2013).
Borthakur, S., Heckman, T. M., Leitherer, C. & Overzier, R. A. Science 346, 216–219 (2014).
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Erb, D. Photons from dwarf galaxy zap hydrogen. Nature 529, 159–160 (2016). https://doi.org/10.1038/529159a
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DOI: https://doi.org/10.1038/529159a