Fig. 13.
Spectrum of the candidate member for the cluster of 3C 187. Original data points are represented with gray background circles, while the blue line represents the best-fit smoothed model. Some spectral features, H, K, Ca I, Hb, and Na I, are potentially identified at redshift 0.466. The Hα⊙ was also detected as we observed the source during a bright night.
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