Extended Data Fig. 4: Fit to the ultraviolet-to-mid-infrared spectral energy distribution.
From: A 100-kiloparsec wind feeding the circumgalactic medium of a massive compact galaxy
The best-fit model and 1σ error are shown with a black line and grey shading; observed fluxes with 1σ errors (usually smaller than the symbols) are yellow circles; and model fluxes are open cyan boxes. Flux is given in AB magnitudes and observed-frame wavelengths in micrometres. The posterior probability P(M) for stellar mass M is shown in the inset.
