For each band, the plots (negative, linear scale) show: (left) SDO/AIA images rebinned to the EIS resolution; (middle) AIA images with the contribution from the “dominant” ion subtracted (with the exception of the 171 Å  see text); (right) radiances in a selection of Hinode EIS lines, with the log T[K] of peak formation temperature (in equilibrium) indicated. The vertical blank lines are due to missing data. The colorbars for the EIS radiances indicate the actual calibrated units (phot cm^-2 s^-1 arcsec^-2), those in the other images DN s^-1 EIS pixel^-1. The FOV of these images is 117.8 and 140.0 arcsec in the E-W and N-S direction. Their centers are 298.2, 344.3 arcsec from Sun center. The boxed areas indicate the FOV of Fig. 5, where strong cool emission is present.