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We report the detection of a hot Jupiter ($M_{p}=1.75_{-0.17}^{+0.14}\M_{J}$, $R_{p}=1.38\pm0.04\ R_{J}$) orbiting a middle-aged star ($\logg=4.152^{+0.030}_{-0.043}$) in the Transiting Exoplanet Survey Satellite (TESS)southern continuous viewing zone ($\beta=-79.59^{\circ}$). We confirm theplanetary nature of the candidate TOI-150.01 using radial velocity observationsfrom the APOGEE-2 South spectrograph and the Carnegie Planet FinderSpectrograph, ground-based photometric observations from the roboticThree-hundred MilliMeter Telescope at Las Campanas Observatory, and Gaiadistance estimates. Large-scale spectroscopic surveys, such as APOGEE/APOGEE-2,now have sufficient radial velocity precision to directly confirm the signatureof giant exoplanets, making such data sets valuable tools in the TESS era.Continual monitoring of TOI-150 by TESS can reveal additional planets andsubsequent observations can provide insights into planetary systemarchitectures involving a hot Jupiter around a star about halfway through itsmain-sequence life.

TOI-150: A transiting hot Jupiter in the TESS southern CVZ