A remarkable ruby: absorption in dense gas, rather than evolved stars, drives the extreme Balmer break of a little red dot at z = 3.5

Author(s):: Graaff, A. de; Rix, H.-W.; Naidu, R.P.; Labbé, I.; Wang, B.; Leja, J.; Matthee, J.; Katz, H.; Greene, J.E.; Hviding, R.E.; Baggen, J.; Bezanson, R.; Boogaard, L.A. (0000-0002-3952-8588); Brammer, G.; Dayal, P.; Dokkum, P. van; Goulding, A.D.; Hirschmann, M.; Maseda, M.V.; McConachie, I.; Miller, T.B.; Nelson, E.; Oesch, P.A.; Setton, D.J.; Shivaei, I.; Weibel, A.; Whitaker, K.E.; Williams, C.C.

Published: 2025
Publication type: Article / Letter to editor

Date issued: 2025
Language: English
Is part of: Astronomy and Astrophysics (2025), A168
hdl: 1887/4288054
doi: 10.1051/0004-6361/202554681
URL: https://ui.adsabs.harvard.edu/abs/2025A&A...701A.168D