Stellar parameters modeled with Hyperion SED fitting code (Robitaille 2017) compared to stellar parameters obtained by Venuti et al. (2014). (a) A_V, (b) distance from the Sun. The red point and error bars represent the mean and standard deviation of the distance of the cluster members studied in this work (d = 757 ± 80 pc), (c) stellar radii, (d) stellar temperatures. A_V and distances are input parameters of the code, while stellar radius and temperature are output parameters of the Hyperion SED Model. The distances were obtained from the Gaia parallax data (Luri et al. 2018). The solid line shows a slope equal to 1. Based on these plots, we conclude that our modeling is doing at least as well as the prior Venuti et al. (2014) modeling.