Posted in astro-ph.CO · 2026-01-12 · M. Galloway, E. Gjerløw, M. San, R. M. Sullivan, D. J. Watts, R. Aurvik, A. Basyrov, L. A. Bianchi, A. Bonato, M. Brilenkov, H. K. Eriksen, U. Fuskeland, K. A. Glasscock, L. T. Hergt, D. Herman, J. G. S. Lunde, A. I. Silva Martins, D. Sponseller, N. -O. Stutzer, H. Thommesen, V. Vikenes, I. K. Wehus, L. Zapelli
We present a model of starlight emission in the Diffuse Infrared Background Explorer (DIRBE) data between 1.25 and 25$\,μ$m based on \textit{Gaia} and WISE measurements. We include two classes of compact objects, namely bright stars with individual spectral energy densities (SEDs) measured by \textit{Gaia}, and a combined diffuse...