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We present results of a search for transiting exoplanets in 10-yr longphotometry with thousands of epochs taken in the direction of the Galacticbulge. This photometry was collected in the fourth phase of the OpticalGravitational Lensing Experiment (OGLE-IV). Our search covered approx. 222 000stars brighter than I = 15.5 mag. Selected transits were verified using aprobabilistic method. The search resulted in 99 high-probability candidates fortransiting exoplanets. The estimated distances to these targets are between 0.4kpc and 5.5 kpc, which is a significantly wider range than for previous transitsearches. The planets found are Jupiter-size, with the exception of one (namedOGLE-TR-1003b) located in the hot Neptune desert. If the candidate isconfirmed, it can be important for studies of highly irradiatedintermediate-size planets. The existing long-term, high-cadence photometry ofour candidates increases the chances of detecting transit timing variations atlong timescales. Selected candidates will be observed by the future NASAflagship mission, the Nancy Grace Roman Space Telescope, in its search forGalactic bulge microlensing events, which will further enhance the photometriccoverage of these stars.

Candidates for Transiting Planets in OGLE-IV Galactic Bulge Fields