Fig. 5.
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Top: Position in the E(B − V) vs Mstar plane of galaxy templates (points colour-coded according to the redshift) that provide an acceptable fit with probability P(z) > 0.5 to the F200W dropout candidates. The regions occupied by the 90% to 10%, at 10% steps, of the aforementioned templates are enclosed by dotted curves. The continuous curves enclose the regions occupied by the 90% to 10%, at 10% steps, of the objects in the same redshift range from the JADES-GS field. The black square and error-bars mark the positions of the confirmed interlopers. Bottom: Same as top panel for low-redshift solutions at 2 ≤ z ≤ 8 in the sSFR vs E(B − V) plane, colour-coded according to the stellar age.
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