Extended Data Fig. 5: Stellar population model fit.
From: A 100-kiloparsec wind feeding the circumgalactic medium of a massive compact galaxy
Spectral data from SDSS and the MMT and 1σ errors are shown as the black line and grey shading. SDSS ugriz photometry and 1σ errors are the cyan squares and grey vertical bars. The best-fit model is a magenta line; the stellar population components summed to produce this model are shown as coloured lines, with ages as shown. SSP, simple stellar population.
