The Large-Scale Extinction Map of the Galactic Bulge from the MACHO Project Photometry

Abstract

We present a (V-R)-based reddening map of about 43 deg2 of the Galactic bulge/bar. The map is constructed using template image photometry from the MACHO microlensing survey, contains 9717 resolution elements, and is based on V-R color averages of the entire color-magnitude diagrams (CMDs) in 4' × 4' tiles. The conversion from the observed color to the reddening follows from an assumption that CMDs of all bulge fields would look similar in the absence of extinction. Consequently, the difference in observed color between various fields originates from varying contribution of the disk extinction summed along different lines of sight. We check that our V-R colors correlate very well with infrared and optical reddening maps. We show that a dusty disk obeying a csc |b| extinction law, E(V-R) = 0.0274 csc |b|, provides a good approximation to the extinction toward the MACHO bulge/bar fields.