We report on observations of 11 transit events of the transiting extrasolar planet XO-1b by the SuperWASP North observatory. From our data, obtained during 2004 May-September, we find that the XO-1b orbital period is 3.941634 +/- 0.000137 days, the planetary radius is 1.34R(J) +/- 0.12R(J), and the inclination is 88.degrees 92 +/- 1.degrees 04, in good agreement with previously published values. We tabulate the transit timings from 2004 SuperWASP and XO data, which are the earliest obtained for XO-1b and which will therefore be useful for future investigations of timing variations caused by additional perturbing planets. We also present an ephemeris for the transits
Artículo de publicación ISIWe report five new transit epochs of the extrasolar planet OGLE-TR-111b, ...
Extrasolar planet transit photometry is a relatively new astronomical technique developed over the p...
Wide-field photometric surveys in search of transiting extrasolar planets are now numerous and have ...
We report on observations of 11 transit events of the transiting extrasolar planet XO-1b by the Supe...
We report on observations of 11 transit events of the transiting extrasolar planet XO-1b by the Supe...
We report on observations of 11 transit events of the transiting extrasolar planet XO-1b by the Supe...
We report on observations of transit events of the transiting planets XO-1b, TrES-1 and TrES-2 with ...
We report on observations of transit events of the transiting planets XO-1b and TrES-1 with the AIU ...
Abstract. We report on observations of transit events of the transiting planets XO-1b, TrES-1 and Tr...
The Wide Angle Search for Planets (WASP) survey currently operates two installations, designated Sup...
The Wide Angle Search for Planets (WASP) survey currently operates two installations, designated Sup...
We present RIz photometry of four consecutive transits of the newly discovered exoplanet XO-1b. We i...
A planet transits an 11th magnitude, G1V star in the constellation Corona Borealis. We designate the...
We present RIz photometry of four consecutive transits of the newly discovered exoplanet XO-1b. We i...
We present RIz photometry of four consecutive transits of the newly discovered exoplanet XO-1b. We i...
Artículo de publicación ISIWe report five new transit epochs of the extrasolar planet OGLE-TR-111b, ...
Extrasolar planet transit photometry is a relatively new astronomical technique developed over the p...
Wide-field photometric surveys in search of transiting extrasolar planets are now numerous and have ...
We report on observations of 11 transit events of the transiting extrasolar planet XO-1b by the Supe...
We report on observations of 11 transit events of the transiting extrasolar planet XO-1b by the Supe...
We report on observations of 11 transit events of the transiting extrasolar planet XO-1b by the Supe...
We report on observations of transit events of the transiting planets XO-1b, TrES-1 and TrES-2 with ...
We report on observations of transit events of the transiting planets XO-1b and TrES-1 with the AIU ...
Abstract. We report on observations of transit events of the transiting planets XO-1b, TrES-1 and Tr...
The Wide Angle Search for Planets (WASP) survey currently operates two installations, designated Sup...
The Wide Angle Search for Planets (WASP) survey currently operates two installations, designated Sup...
We present RIz photometry of four consecutive transits of the newly discovered exoplanet XO-1b. We i...
A planet transits an 11th magnitude, G1V star in the constellation Corona Borealis. We designate the...
We present RIz photometry of four consecutive transits of the newly discovered exoplanet XO-1b. We i...
We present RIz photometry of four consecutive transits of the newly discovered exoplanet XO-1b. We i...
Artículo de publicación ISIWe report five new transit epochs of the extrasolar planet OGLE-TR-111b, ...
Extrasolar planet transit photometry is a relatively new astronomical technique developed over the p...
Wide-field photometric surveys in search of transiting extrasolar planets are now numerous and have ...