Fig. 1.
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From top to bottom, rotated sky-subtracted images of the low-mass ultra-thin galaxy UGC 7321 in 3.6 μm, grz (stacked), NUV, and FUV. The red lines indicate the height at which SB equals 26 mag arcsec−2 in 3.6 μm, while the blue lines show the height (5′) above which 90% of the light comes from the thick disk. These values are averaged from the vertical luminosity cuts of Comerón et al. (2018).
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