Bayesian inference of stellar parameters and interstellar extinction using parallaxes and multiband photometry
Abstract
Astrometric surveys provide the opportunity to measure the absolute magnitudes of large numbers of stars, but only if the individual lineofsight extinctions are known. Unfortunately, extinction is highly degenerate with stellar effective temperature when estimated from broadband optical/infrared photometry. To address this problem, I introduce a Bayesian method for estimating the intrinsic parameters of a star and its lineofsight extinction. It uses both photometry and parallaxes in a selfconsistent manner in order to provide a nonparametric posterior probability distribution over the parameters. The method makes explicit use of domain knowledge by employing the HertzsprungRussell Diagram (HRD) to constrain solutions and to ensure that they respect stellar physics. I first demonstrate this method by using it to estimate effective temperature and extinction from BVJHK data for a set of artificially reddened Hipparcos stars, for which accurate effective temperatures have been estimated from highresolution spectroscopy. Using just the four colours, we see the expected strong degeneracy (positive correlation) between the temperature and extinction. Introducing the parallax, apparent magnitude and the HRD reduces this degeneracy and improves both the precision (reduces the error bars) and the accuracy of the parameter estimates, the latter by about 35 per cent. The resulting accuracy is about 200 K in temperature and 0.2 mag in extinction. I then apply the method to estimate these parameters and absolute magnitudes for some 47 000 F, G, K Hipparcos stars which have been crossmatched with TwoMicron AllSky Survey (2MASS). The method can easily be extended to incorporate the estimation of other parameters, in particular metallicity and surface gravity, making it particularly suitable for the analysis of the 10^{9} stars from Gaia.
 Publication:

Monthly Notices of the Royal Astronomical Society
 Pub Date:
 February 2011
 DOI:
 10.1111/j.13652966.2010.17699.x
 arXiv:
 arXiv:1009.2766
 Bibcode:
 2011MNRAS.411..435B
 Keywords:

 methods: data analysis;
 methods: statistical;
 surveys;
 stars: fundamental parameters;
 HertzsprungRussell and colourmagnitude diagrams;
 dust;
 extinction;
 Astrophysics  Instrumentation and Methods for Astrophysics;
 Astrophysics  Astrophysics of Galaxies;
 Statistics  Applications
 EPrint:
 MNRAS, in press. The catalogue is available from http://tinyurl.com/qmethod. Minor changes/corrections to text made in v2