Bayesian analysis of resolved stellar spectra

We introduce a Bayesian method for fitting faint, resolved stellar spectra in order to obtain simultaneous estimates of redshift and stellar-atmospheric parameters. We apply the...本研究提出一种贝叶斯方法（Bayesian method），用于拟合暗弱且已分辨的恒星光谱，以同时获取红移与恒星大气参数的联合估算结果。我们将该方法应用于