Transiting Exoplanet Monitoring Project (TEMP). VI. The Homogeneous Refinement of System Parameters for 39 Transiting Hot Jupiters with 127 New Light Curves

We present 127 new transit light curves for 39 hot Jupiter systems, obtained over the span of five years by two ground-based telescopes. A homogeneous analysis these newly collected together with archived spectroscopic, photometric, and Doppler velocimetric data using EXOFASTv2 leads to a significant improvement in physical orbital parameters each system. All our stellar radii are constrained accuracies better than 3\%. The planetary 37 targets determined $5\%$. Compared results, literature eccentricities preferentially overestimated due Lucy-Sweeney bias. Our photometric observations therefore allow ephemerides correction future window amounts change exceeding $10\,{\rm min}$ ten at time JWST's launch, including $72\,{\rm WASP-56. measured mid-times both photometry show no deviations from updated linear ephemerides, ruling out system presence companion planets masses greater $0.39 - 5.0\, rm M_{\oplus}$, $1.23 14.36\, \rm $1.65 21.18\, $0.69 6.75\, M_{\oplus}$ near 1:2, 2:3, 3:2, 2:1 resonances Jupiters , respectively, confidence level $\pm 1\,\sigma$. absence resonant systems is inconsistent conventional expectation disk migration.