Image Details
Caption: Figure 3.
The rest-frame 1.4 GHz continuum luminosity (upper) of the background sources, the H I column density (middle), and the H I peak optical depth versus redshift (lower) for the 21 cm H I absorbers, including data points from K. Geréb et al. (2015), F. M. Maccagni et al. (2017), S. J. Curran & S. W. Duchesne (2018), and FASHI. In the upper panel, the different lines indicate different 1.4 GHz continuum-flux density.
© 2026. The Author(s). Published by the American Astronomical Society.