Fig. 3.
![Gaussian FWHM of the [C ii] line as a function of the quasar absolute UV magnitude ($M_{\rm 1450}$). Compilations of $z \gt 5.7$ quasars from the literature (circle; Maiolino et al. 2005; Venemans et al. 2012, 2016, 2017c; Willott et al. 2013, 2015, 2017; Bañados et al. 2015; Mazzucchelli et al. 2017; Decarli et al. 2018) are plotted along with the HSC quasars (star) measured in Izumi et al. (2018b) and in this work. (Color online)](https://oup.silverchair-cdn.com/oup/backfile/Content_public/Journal/pasj/71/6/10.1093_pasj_psz096/2/pasj_71_6_111_f7.jpeg?Expires=1749862367&Signature=V5xMrBskTfJkEpD5t6NMTDI-Vd-i2Vu2PRwi6Qit~ahgjH3fIXw46FKG9Qu-YDxJRFzQT5N5BgtvrgNh5wA1XEpNbMBRWvlwy9GjQIjweYXmiCcAhAe3hH7hgUoJCVOzkay4guq~ARIgDLUCIAgJEWscUfwVcV8-rJHkgKPieMfZSN2zELjzyQSfQcGbMuxC4aL1J6visGPxmFwT1jvBsJLR-C-nLAUoJKNgyQ4c2OpACDlvDudpxBHhU1j~rjbQlwRmryvMsGFRtmrEzMoad8~fYyUPtDJu3pmZAlOHHs3mdnHKyodGPXC67USxIcEtYCmgQw~tHmnWefC1BQXCGA__&Key-Pair-Id=APKAIE5G5CRDK6RD3PGA)
Gaussian FWHM of the [C ii] line as a function of the quasar absolute UV magnitude (|$M_{\rm 1450}$|). Compilations of |$z \gt 5.7$| quasars from the literature (circle; Maiolino et al. 2005; Venemans et al. 2012, 2016, 2017c; Willott et al. 2013, 2015, 2017; Bañados et al. 2015; Mazzucchelli et al. 2017; Decarli et al. 2018) are plotted along with the HSC quasars (star) measured in Izumi et al. (2018b) and in this work. (Color online)
