Figure 2.
Optical spectrum of G1 obtained using MagE on the Magellan Clay Telescope. The data reveal numerous emission features (marked by long dashed lines) with a mean redshift at z = 0.4188 ± 0.0001. The corresponding 1σ error spectrum is shown in cyan at the bottom above the zero flux level (dash–dotted line). Contaminating sky residuals are dotted out for clarification.

Optical spectrum of G1 obtained using MagE on the Magellan Clay Telescope. The data reveal numerous emission features (marked by long dashed lines) with a mean redshift at z = 0.4188 ± 0.0001. The corresponding 1σ error spectrum is shown in cyan at the bottom above the zero flux level (dash–dotted line). Contaminating sky residuals are dotted out for clarification.

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