A Bayesian Method for the Extinction
  We propose a Bayesian method to measure the total Galactic extinction parameters, $R_V$ and $A_V$. Validation tests based on the simulated data indicate that the method can achieve the accuracy of around 0.01\,mag. We apply this method to the SDSS BHB stars in the northern Galactic cap and find that the derived extinctions are highly consistent with those from \cite{SFD98}. It suggests that the Bayesian method is promising for the extinction estimation, even the reddening values are close to the observational errors. 
Hai-Jun Tian, Chao Liu, Jing-Yao Hu, Yang Xu, Xue-Lei Chen
astro-ph.IM astro-ph.GA