VPNEP: Detailed characterization of TESS targets around the Northern Ecliptic Pole - I. Survey design, pilot analysis, and initial data release

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Fig. 6

Comparison of the ParSES parameters for a mixed stellar subsample observed with STELLA+SES and VATT+PEPSI. Panel a: effective temperature in Kelvin. Panel b: logarithmic gravity in cm s⁻². Panel c: global metallicity relative to solar. Panel d: rotational line broadening υ sin i in km s⁻¹. Dashed line is just a 45-degree line to guide the eye.

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