The bulge luminosity functions in the MSX infrared bands
arXiv:astro-ph/0012039 · doi:10.1051/0004-6361:20000421
Abstract
We use an inversion technique to derive the luminosity functions of the Galactic bulge from point source counts extracted from the Midcourse Space Experiment's Point Source Catalog (version 1.2).
5 pages, 2 figures, to be published in A&A