SIMBAD references

2007AJ....134.1707W - Astron. J., 134, 1707-1712 (2007/October-0)

The transit light curve project. VII. The not-so-bloated exoplanet HAT-P-1b.

WINN J.N., HOLMAN M.J., BAKOS G.A., PAL A., JOHNSON J.A., WILLIAMS P.K.G., SHPORER A., MAZEH T., FERNANDEZ J., LATHAM D.W. and GILLON M.

Abstract (from CDS):

We present photometry of the G0 star HAT-P-1 during six transits of its close-in giant planet, and we refine the estimates of the system parameters. Relative to Jupiter's properties, HAT-P-1b is 1.20±0.05 times larger, and its surface gravity is 2.7±0.2 times weaker. Although it remains the case that HAT-P-1b is among the least dense of the known sample of transiting exoplanets, its properties are in accord with previously published models of strongly irradiated, coreless, solar-composition giant planets. The times of the transits have a typical accuracy of 1 minute and do not depart significantly from a constant period.

Abstract Copyright: ∼

Journal keyword(s): Stars: Planetary Systems - stars: individual (HAT-P-1) - stars: individual (ADS 16402B)

VizieR on-line data: <Available at CDS (J/AJ/134/1707): table1.dat>

Errata: erratum vol. 136, p. 1735 (2008)

Simbad objects: 4

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