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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 2.

Confirmation of line detection in EGSY8p7 over two nights. Left: HST F160W image of the EGSY8p7 field with the slit orientations adopted in two successive nights. Right: extracted 1D signal-to-noise spectra across the J band for each night with a zoom of the 2D data around the line, marked with a vertical blue line. The 2D spectra are smoothed with a 3-pixel Gaussian for better illustration of the data. The 1D spectrum is smoothed with a Gaussian of σ = 5 Å, comparable to the measured line width. The Y axis is scaled so that the peak signal to noise matches the integrated value (e.g., F13). Horizontal dashed lines mark the ﹩\pm 3\sigma ﹩ region. On both nights, the signal to noise at the line location significantly exceeds that elsewhere.

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