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Fig. 1.

image

Three-color composite images of the two galaxies for which we present new Chandra and MUSE data in this paper. Left: SOAR Optical Imager (SOI) b-, ν-, and r-band composite of HE 0227-0913 (Markarian 1044). These bands have been assigned to the blue, green, and red channels, respectively. Right: composite made by collapsing three slices through the MUSE cube across wavelength ranges that roughly correspond to the g-, r-, and i-bands, again respectively assigned to the blue, red, and green channels. We have applied a logarithmic stretch to both panels to better show the low surface brightness galaxy outskirts alongside the bright type 1 nuclei. Both images have been rotated, with east left and north up.

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