A deep MeerKAT view of associated H I absorption in radio AGNs at intermediate redshift: Role of absorber geometry and conditions of the gas

Open Access

Fig. 3.

Distribution of the peak optical depth taken from Maccagni et al. (2017, grey and empty bars) with overlaid the peak optical depth for the detected (dark red boxes) and limits thereof (light red) for the sources of the present sample. The distribution shows how the present observations reach very low optical depths.

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