The Dark Energy Survey 5-year photometrically identified Type Ia Supernovae classification probabilities with SuperNNova

Classification probabilities obtained for the Dark Energy Survey 5-year photometrically identified SN Ia. Probabilities were obtained with SuperNNova (Möller et al. 2020) using multi-band light-curves and host galaxy redshifts. The classification models were trained to disentangle type Ia vs. non Ia supernovae.本数据集提供了暗能量巡天（Dark Energy Survey）5年期测光认证的Ia型超新星（SN Ia）的分类概率。该分类概率通过SuperNNova（Möller等人，2020）基于多波段光变曲线与宿主星系红移计算得到。本次训练的分类模型旨在区分Ia型超新星与非Ia型超新星。