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. 9.

UV luminosities for our sample (red points) together with some available in literature (black = Maccagni et al. (2017), green = Murthy et al. (2021), magenta = Murthy et al. (2022), and blue = Aditya (2019), adapted from Murthy et al. (2022). Square points are detections, crosses represent the limits. The dashed line represents the L_UV = 10²³ W Hz⁻¹ threshold proposed by Curran et al. (2008, see text for details).

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