Fig. 9

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CaMD of different stellar classes used to assign a variable signal to stellar contaminants. The respective class is written in the title header together with the number count of the class. The upper panels show the confinement of all stars that feature solar-like variability: (a) red giants, (b) solar-like dwarfs and subgiants, and (c) red dwarfs. The lower panels show the confinement of (d) binaries, (e) giants and compact objects (above the purple line and below the blue lines, respectively), and (f) all objects with an unknown spectral type. The black points are all stars in the LOPS2 (G ≲ 17), whereas the metallic contour defines stars within 1 kpc from the Sun.
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