SIMBAD references

2015A&A...580A..63M - Astronomy and Astrophysics, volume 580A63-63 (2015/8-1)

HATS-13b and HATS-14b: two transiting hot Jupiters from the HATSouth survey.

MANCINI L., HARTMAN J.D., PENEV K., BAKOS G.A., BRAHM R., CICERI S., HENNING Th., CSUBRY Z., BAYLISS D., ZHOU G., RABUS M., DE VAL-BORRO M., ESPINOZA N., JORDAN A., SUC V., BHATTI W., SCHMIDT B., SATO B., TAN T.G., WRIGHT D.J., TINNEY C.G., ADDISON B.C., NOYES R.W., LAZAR J., PAPP I. and SARI P.

Abstract (from CDS):

We report the discovery of HATS-13b and HATS-14b, which are two hot-Jupiter transiting planets discovered by the HATSouth survey. The host stars are quite similar to each other (HATS-13: V=13.9 mag, M*=0.96M☉, R*=0.89R☉, Teff≃5500K, [Fe/H]=0.05; HATS-14: V=13.8 mag, M*=0.97M☉, R*=0.93R☉, Teff≃5350K, [Fe/H]=0.33) and both the planets orbit around them with a period of ∼3 days and a separation of ∼0.04 au. However, even though they are irradiated in a similar way, the physical characteristics of the two planets are very different. HATS-13b, with a mass of Mp=0.543±0.072MJ and a radius of Rp=1.212±0.035RJ, appears as an inflated planet, while HATS-14b, having a mass of Mp=1.071±0.070MJ and a radius of Rp=1.039±0.032RJ, is only slightly larger in radius than Jupiter.

Abstract Copyright: ∼

Journal keyword(s): planetary systems - stars: fundamental parameters - techniques: radial velocities - techniques: photometric - stars: individual: HATS-13 - stars: individual: HATS-14

VizieR on-line data: <Available at CDS (J/A+A/580/A63): h13hs.dat h13ctio.dat h13grg.dat h13gri.dat h13grr.dat h13grz.dat h13p1.dat h13p2.dat h13rv.dat h14hs.dat h14p.dat h14grg.dat h14gri.dat h14grr.dat h14grz.dat h14rv.dat>

Simbad objects: 7

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