Spatial distribution of classified spectra in Leo P. Left-hand panel: HST-ACS F475W image; right-hand panel: V-band image recovered from the MUSE cube. Objects are identified as follows: massive stars (filled cyan circles), candidate massive stars (open blue circles), carbon stars (filled red circles), additional candidate AGB stars from Lee (2016, open red circles), background galaxies (green circles), foreground stars (open green squares). The 100 pc scalebar assumes the distance of 1.62 Mpc from McQuinn et al. (2015).