We have carried out a campaign to characterize the hot Jupiters WASP-5b, WASP-44b, and WASP-46b using multi-band photometry collected at the ObservatOrio do Pico Dos Dias in Brazil. We have determined the planetary physical properties and new transit ephemerides for these systems. The new orbital parameters and physical properties are consistent with previous estimates. We also studied the transit times including our new ephemerides. We did not find variations of a linear trend due to extra companions. Finally, we studied the fractional radius variation as a function of wavelength for these systems.