A lack of Lyman α emitters within 5 Mpc of a luminous quasar in an overdensity at z = 6.9: Potential evidence of negative quasar feedback at protocluster scales

Open Access

Fig. 3.

Predicted Z-NB964 color of a Ly-α emitter for redshifts ranging from 6.5 to 7 for varying equivalent widths. The dashed line indicates the Z-NB964 color selection criteria that we have adopted and the shaded region shows the NB964 filter profile.

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