Abstract
We report the discovery of WASP-13b, a low-mass transiting exoplanet with an orbital period of days. The transit has a depth of 9 mmag, and although our follow-up photometry does not allow us to constrain the impact parameter well (), with radius in the range the location of WASP-13b in the mass-radius plane is nevertheless consistent with H/He-dominated, irradiated, low core mass and core-free theoretical models. The G1V host star is similar to the Sun in mass (M) and metallicity ([M/H]=), but is possibly older ( Gyr).
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