Confusion matrices for theoretical young stellar object models

This is a data table supplementing the following publication: 

A framework for modeling the evolution of young stellar objects (Richardson et al., submitted).

It contains a set of confusion matrices comparing the evolutionary stages and classes of radiative transfer YSO models selected by proximity to protostellar evolutionary tracks. Models are included in a matrix based on their correspondence to particular modeled accretion histories, zero-age stellar masses, ages, mass accretion efficiencies, and levels of detectability (defined using flux in the ALMA Band 6 wavelength range). Details on the construction and use of the table are contained in the accompanying README file, and more information about the matrices is contained in Section 4.2 of the companion paper.

The YSO models populating these matrices are from Richardson et al. (2024); information on them is contained in the companion work and data release.

本数据表为以下学术成果的配套补充资料：《年轻恒星体（Young Stellar Objects, YSO）演化建模框架》（Richardson等人，已投稿）。
本数据表包含一组混淆矩阵（confusion matrices），用于对比基于与原恒星演化轨迹（protostellar evolutionary tracks）贴近度筛选出的辐射转移（radiative transfer）型YSO模型的演化阶段与分类。模型被纳入各矩阵的依据为其与特定模拟吸积历史、零年龄恒星质量、恒星年龄、质量吸积效率，以及以ALMA 6波段（ALMA Band 6）流量为定义依据的可探测性水平的匹配程度。
本数据表的构建与使用细节详见随附的README文件，关于该批混淆矩阵的更多信息可参阅配套论文的4.2节。
构成该批混淆矩阵的YSO模型源自Richardson等人（2024）的研究，相关模型信息详见该配套研究与数据集发布内容。