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Modelling the Milky Way-I. Method and first results fitting the thick disc and halo with DES-Y3 data

A. Pieres*, L. Girardi, E. Balbinot, B. Santiago, L. N. da Costa, A. Carnero Rosell, A. B. Pace, K. Bechtol, M. A. T. Groenewegen, A. Drlica-Wagner, T. S. Li, M. A. G. Maia, R. L. C. Ogando, M. dal Ponte, H. T. Diehl, A. Amara, S. Avila, E. Bertin, D. Brooks, D. L. BurkeM. Carrasco Kind, J. Carretero, J. De Vicente, S. Desai, T. F. Eifler, B. Flaugher, P. Fosalba, J. Frieman, J. García-Bellido, E. Gaztanaga, D. W. Gerdes, D. Gruen, R. A. Gruendl, J. Gschwend, G. Gutierrez, D. L. Hollowood, K. Honscheid, D. J. James, K. Kuehn, N. Kuropatkin, J. L. Marshall, R. Miquel, A. A. Plazas, E. Sanchez, S. Serrano, I. Sevilla-Noarbe, E. Sheldon, M. Smith, M. Soares-Santos, F. Sobreira, E. Suchyta, M. E. C. Swanson, G. Tarle, D. Thomas, V. Vikram, A. R. Walker

*Corresponding author for this work

Research output: Contribution to journal › Article › peer-review

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