SED for DF Tau A (blue) and B (red). Photometry that does not resolve A and B is shown in purple. The JWST-MIRI MRS spectrum is shown in black. A BT Settl model photosphere for an M2-type star is shown in gray, scaled to the J-band photometry, for reference (Allard et al. 2012). The SED has been de-reddened with an A_V=0.5 mag (Allen et al. 2017). Error bars are smaller than the markers in most cases. The photometric point at 1.3 mm from ALMA is the same for DF Tau A and B and the point for DF Tau A is shifted horizontally for clarity.