We report the discovery of WASP-13b, a low-mass Mp=0.46−0.05+0.06MJ transiting exoplanet with an orbital period of 4.35298±0.00004 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 (0<b<0.46), with radius in the range Rp∼1.06−1.21RJ 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∗=1.03−0.09+0.11M⊙) and metallicity ([M/H]=0.0±0.2), but is possibly older (8.5−4.9+5.5 Gyr).
@article{arxiv.0905.3115,
title = {The 0.5M$_J$ transiting exoplanet WASP-13b},
author = {I. Skillen and D. Pollacco and A. Collier Cameron and L. Hebb and E. Simpson and F. Bouchy and D. J. Christian and N. P. Gibson and G. Hébrard and Y. C. Joshi and B. Loeillet and B. Smalley and H. C. Stempels and R. A. Street and S. Udry and R. G. West and D. R. Anderson and S. C. C. Barros and B. Enoch and C. A. Haswell and C. Hellier and K. Horne and J. Irwin and F. P. Keenan and T. A. Lister and P. Maxted and M. Mayor and C. Moutou and A. J. Norton and N. Parley and D. Queloz and R. Ryans and I. Todd and P. J. Wheatley and D. M. Wilson},
journal= {arXiv preprint arXiv:0905.3115},
year = {2015}
}
Comments
4 pages. Accepted for publication in Astronomy and Astrophysics