Fig. 6.
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Examples of the spectral energy distribution of T CrB from quiescence (2008-2011) to SAP peak (2016), and for reference that of the M3III template HD 112300, plotted in black and scaled to the distance of T CrB. Quoted LUV and Lopt are the accretion luminosities (in L⊙) radiated over the 1700–3500 and 3500–8000 Å intervals, respectively. Note on the SED for 2008–2011 the effect of the red-leak affecting the Swift W2 filter.
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