Stars identified to match our solar-analogue criteria (see Sect. 5.8). The marker size indicates the visual magnitude (see legend), while the colour gives the [Fe/H]-value from Casagrande et al. (2011). Empty markers indicate known bright oscillators from ground-based surveys (and 16 Cyg B from Kepler) that match the solar-analogue criteria, but where no detection was obtained in this study. Markers with a thick black edge indicate the stars that are already known oscillators (see Table D.1). Left: identified (potential) solar analogues in terms of distance and ν_max (α Cen A at a distance of ~1.35 pc is moved to a higher distance for a better display of the sample). The horizontal dotted line gives the solar ν_max-value for reference. Right: identified (potential) solar analogues in terms of T_eff and luminosity, using magnitudes and distances from the TESS Input Catalog (TICv8.2; Paegert et al. 2021). The dotted lines provide the solar values for reference. For reference, we also show 1 M_⊙ MIST¹⁶ evolutionary tracks (Dotter 2016; Choi et al. 2016) with [Fe/H]-values of −0.3, 0, and +0.3 dex (increasing with tracks from left to right; also see color bar).