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Lyα EMISSION FROM A LUMINOUS z = 8.68 GALAXY: IMPLICATIONS FOR GALAXIES AS TRACERS OF COSMIC REIONIZATION

  • Authors: Adi Zitrin, Ivo Labbé, Sirio Belli, Rychard Bouwens, Richard S. Ellis, Guido Roberts-Borsani, Daniel P. Stark, Pascal A. Oesch, and Renske Smit

2015 The Astrophysical Journal Letters 810 L12.

  • Provider: AAS Journals

Caption: Figure 4.

Photometric SED fitting strongly supports a high-redshift solution for EGSY8p7: red points show magnitudes, where the horizontal error marks the filter width, and triangles denote 1σ upper-limits from non-detections. The blue SED shows the best-fit template at z = 8.57. The magenta SED shows the z = 8.48 solution adopting the strong emission line template used in RB15 (see their work for more details on the templates). The gray SED shows the best-fit low-redshift template, which cannot explain the absence of detection in the optical bands and which is ∼107 times less likely than the high-redshift solutions.

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