Left panel: projected obliquities of warm Jupiter systems (10 d < P < 200 d and R_p > 6 R_⊕) as a function of orbital period. Warm Jupiters in single-star and multi-star systems are shown in cyan and magenta, respectively. The single-star TOI-4127 system is shown in gold. All other systems with measured obliquities are shown in black. Right panel: projected obliquities as a function of orbital eccentricity. System parameters were obtained from TEPCat (Southworth 2011).