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We present the discovery of TYC9191-519-1b (TOI-150b, TIC 271893367) andHD271181b (TOI-163b, TIC 179317684), two hot Jupiters initially detected using30-minute cadence Transiting Exoplanet Survey Satellite TESS photometry fromSector 1 and thoroughly characterized through follow-up photometry (CHAT,Hazelwood, LCO/CTIO, El Sauce, TRAPPIST-S), high-resolution spectroscopy(FEROS, CORALIE) and speckle imaging (Gemini/DSSI), confirming the planetarynature of the two signals. A simultaneous joint fit of photometry and radialvelocity using a new fitting package juliet reveals that TOI-150b is a$1.254\pm0.016\ R_J$, massive ($2.61^{+0.19}_{-0.12}\ M_J$) hot Jupiter in a$5.857$-day orbit, while TOI-163b is an inflated ($R_P$ =$1.478^{+0.022}_{-0.029} R_J$, $M_P$ = $1.219\pm0.11 M_J$) hot Jupiter on a $P$= $4.231$-day orbit; both planets orbit F-type stars. A particularlyinteresting result is that TOI-150b shows an eccentric orbit($e=0.262^{+0.045}_{-0.037}$), which is quite uncommon among hot Jupiters. Weestimate that this is consistent, however, with the circularization timescalewhich is slightly larger than the age of the system. These two hot Jupiters areboth prime candidates for further characterization --- in particular, both areexcellent candidates for determining spin-orbit alignments via theRossiter-McLaughlin (RM) effect and for characterizing atmospheric thermalstructures using secondary eclipse observations considering they are bothlocated closely to the James Webb Space Telescope (JWST) Continuous ViewingZone (CVZ).

TOI-150b and TOI-163b: two transiting hot Jupiters, one eccentric and one inflated, revealed by TESS near and at the edge of the JWST CVZ