Gaussian fittings to the observed Brγ (H I 4–7, top panel) and Brα (H I 4–5, bottom panel) line profiles that disentangle emission and absorption components. The spectra shown here were taken on June 22 and June 28, 2015, respectively. The fittings combining all contributing Gaussian components (solid red line) are overlaid on the observations in black. The individual Gaussian components used to model the lines are shown with different colours and have been shifted down in the y direction for better visualisation.