Add to ORKGAbstract The transiting exoplanet system HAT-P-24 was observed by using CCD cameras at Yunnan Observatory and Hokoon Astronomical Centre, China in 2010 and 2012. In order to enhance the signal to noise ratio of transit events, the observed data are corrected for systematic errors according to Collier Cameron et al.’s coarse de-correlation and Tamuz et al.’s SYSREM algorithms. Three new complete transit light curves are analyzed by means of the Markov chain Monte Carlo technique, and the new physical parameters of the system are derived. They are consistent with the old ones from the discovered paper except for a new larger radiusRp = 1.364RJ of HAT-P-24b, which confirms its inflated nature. By combining the five available epochs of mid-tran...
Context. By now, more than 300 planets transiting their host star have been found, and much effort i...
We present four new light curves of the transiting exoplanets WASP-1b and HAT-P-20b, observed within...
Upon its discovery, the low-density transiting Neptune HAT-P-26b showed a 2.1σ detection drift in it...
Three transit events of HAT-P-8 are observed by using the 1 m telescope of Yunnan Observatory and 2....
Abstract We report new photometric observations of the transiting exoplanetary sys-tem WASP-32 made ...
This work was supported by the National Natural Science Foundation of China (No. 10873031), Chinese ...
Thesis: S.B., Massachusetts Institute of Technology, Department of Earth, Atmospheric, and Planetary...
As part of our ongoing effort to investigate transit timing variations (TTVs) of known exoplanets, w...
We present seven light curves of the exoplanet system HAT-P-3, taken as part of a transit timing pro...
We present photometry of the G0 star HAT-P-1 during six transits of its close-in giant planet, and w...
Context. By now, more than 300 planets transiting their host star have been found, and much effort i...
Context. Accurate and repeated photometric follow-up observations of planetary transit events are im...
As part of our ongoing effort to investigate transit timing variations (TTVs) of known exoplanets, w...
We report the photometry of six transits of the hot Jupiter HAT-P-29b obtained from 2013 October to ...
Context. By now, more than 300 planets transiting their host star have been found, and much effort i...
We present four new light curves of the transiting exoplanets WASP-1b and HAT-P-20b, observed within...
Upon its discovery, the low-density transiting Neptune HAT-P-26b showed a 2.1σ detection drift in it...
Three transit events of HAT-P-8 are observed by using the 1 m telescope of Yunnan Observatory and 2....
Abstract We report new photometric observations of the transiting exoplanetary sys-tem WASP-32 made ...
This work was supported by the National Natural Science Foundation of China (No. 10873031), Chinese ...
Thesis: S.B., Massachusetts Institute of Technology, Department of Earth, Atmospheric, and Planetary...
As part of our ongoing effort to investigate transit timing variations (TTVs) of known exoplanets, w...
We present seven light curves of the exoplanet system HAT-P-3, taken as part of a transit timing pro...
We present photometry of the G0 star HAT-P-1 during six transits of its close-in giant planet, and w...
Context. By now, more than 300 planets transiting their host star have been found, and much effort i...
Context. Accurate and repeated photometric follow-up observations of planetary transit events are im...
As part of our ongoing effort to investigate transit timing variations (TTVs) of known exoplanets, w...
We report the photometry of six transits of the hot Jupiter HAT-P-29b obtained from 2013 October to ...
Context. By now, more than 300 planets transiting their host star have been found, and much effort i...
We present four new light curves of the transiting exoplanets WASP-1b and HAT-P-20b, observed within...
Upon its discovery, the low-density transiting Neptune HAT-P-26b showed a 2.1σ detection drift in it...