Direct comparison between equivalent diameters obtained using the radiometric technique (x-axis) and those obtained from stellar occultations (y-axis). The references for the object diameters from occultation and radiometric data are: Eris (Sicardy et al. 2011; Santos-Sanz et al. 2012), Haumea (Ortiz et al. 2017; Fornasier et al. 2013), Makemake (Ortiz et al. 2012; Lim et al. 2010), Quaoar (Braga-Ribas et al. 2013; Fornasier et al. 2013), Varda (Souami et al. 2020; Vilenius et al. 2014), 2003 AZ₈₄ (Dias-Oliveira et al. 2017; Mommert et al. 2012), 2007 UK₁₂₆ (Benedetti-Rossi et al. 2016; Santos-Sanz et al. 2012), 2002 TC₃₀₂ (Ortiz et al. 2020b; Fornasier et al. 2013), 2003 VS₂ (Benedetti-Rossi et al. 2019; Mommert et al. 2012), 2002 TX₃₀₀ (Elliot et al. 2010; Vilenius et al. 2018), and Chariklo (Leiva et al. 2017; Lellouch et al. 2017).