Fig. 4.
Example of a simultaneous BEAGLE fit to HST photometry (top panel) and MUSE integrated fluxes (bottom panel) for the Mg II emitter ID17 at z = 0.84 (left panel) and Mg II absorbers ID14 at z = 0.77 (right panel). Top panel: HST (cyan diamonds) and predicted (black points and shaded red area) broad-band photometry. In black we show the full SED predicted from the BEAGLE fit. Bottom panel: integrated fluxes measured from MUSE spectra (red diamonds) and from the SED predicted by BEAGLE (gray diamonds). Error bars on the data points are contained within the markers.
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