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The Evolution of Lyα emitting Galaxies between z = 2 1 and z = 3 1

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Figure 2. Excess emission in the narrowband λ5010 filter over the continuum for objects in our survey field
Table 4 Photometric Uncertainties Log F 5010 σ Log F 5010 σ (mag) (mag) −15.50 0.012 −16.30 0.079 −15.60 0.016 −16.40 0.095 −15.70 0.022 −16.50 0.115 −15.80 0.029 −16.60 0.134 −15.90 0.036 −16.70 0.167 −16.00 0.044 −16.80 0.198 −16.10 0.052 −16.90 0.235 −1
Figure 5 displays the distribution of continuum-subtracted Lyα emission-line luminosities for our new sample of z = 3.1 LAEs
Figure 6. Left-hand panel displays the distribution of Lyα rest-frame equivalent widths as a function of (continuum-subtracted) Lyα emission-line luminosity, the middle panel shows these same equivalent widths as a function of continuum magnitude, and the
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