Orbital and spectral analysis of the benchmark brown dwarf HD 4747B

<p><strong>Context.</strong> The study of high-contrast imaged brown dwarfs and exoplanets depends strongly on evolutionary models. To estimate the mass of a directly imaged substellar object, its extracted photometry or spectrum is used and adjusted with model spectra together wit...

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Bibliographic Details
Main Authors:	Peretti, S, Ségransan, D, Lavie, B, Desidera, S, Maire, A, D'Orazi, V, Vigan, A, Baudino, J, Cheetham, A, Janson, M, Chauvin, G, Hagelberg, J, Menard, F, Heng, K, Udry, S, Boccaletti, A, Daemgen, S, Coroller, H, Mesa, D, Rouan, D, Samland, M, Schmidt, T, Zurlo, A, Bonnefoy, M, Feldt, M, Gratton, R, Lagrange, A, Langlois, M, Meyer, M, Carbillet, M, Carle, M, Caprio, V, Gluck, L, Hugot, E, Magnard, Y, Moulin, T, Pavlov, A, Pragt, J, Rabou, P, Ramos, J, Rousset, G, Sevin, A, Soenke, C, Stadler, E, Weber, L, Wildi, F
Format:	Journal article
Published:	EDP Sciences 2019

Orbital and spectral analysis of the benchmark brown dwarf HD 4747B

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