MOA-2022-BLG-249Lb: Nearby microlensing super-Earth planet detected from high-cadence surveys

Aims. We investigate the data collected by the high-cadence microlensing surveys during the 2022 season in search of planetary signals appearing in the light curves of microlensing events. From this search, we find that the lensing event MOA-2022-BLG-249 exhibits a brief positive anomaly that lasted for about one day, with a maximum deviation of similar to 0.2 mag from a single-source, single-lens model. Methods. We analyzed the light curve under the two interpretations of the anomaly: one originated by a low-mass companion to the lens (planetary model) and the other originated by a faint companion to the source (binary-source model). Results. We find that the anomaly is better explained by the planetary model than the binary-source model. We identified two solutions rooted in the inner-outer degeneracy and for both of them, the estimated planet-to-host mass ratio, q similar to 8 x 10(-5), is very small. With the constraints provided by the microlens parallax and the lower limit on the Einstein radius, as well as the blend-flux constraint, we find that the lens is a planetary system, in which a super-Earth planet, with a mass of (4.83 +/- 1.44) M-circle dot, orbits a low-mass host star, with a mass of (0.18 +/- 0.05) M-circle dot, lying in the Galactic disk at a distance of (2.00 +/- 0.42) kpc. The planet detection demonstrates the elevated microlensing sensitivity of the current high-cadence lensing surveys to low-mass planets.

Automated summary

We analyze the data from high-cadence microlensing surveys in 2022 to search for planetary signals in the light curves of microlensing events. One lensing event, MOA-2022-BLG-249, exhibits a brief positive anomaly that can be better explained by a low-mass companion to the lens (planetary model) rather than a faint companion to the source (binary-source model). We find that the lens is a planetary system, with a super-Earth planet orbiting a low-mass host star in the Galactic disk.