Light curves of HAT-P-3b and HAT-P-14b (Nascimbeni+, 2011)

Details Light curves of HAT-P-3b and HAT-P-14b (Nascimbeni+, 2011) Light curves of HAT-P-3b and HAT-P-14b (Nascimbeni+, 2011)

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..35279085n&link_type=abstract

VizieR On-line Data Catalog: J/A+A/527/A85. Originally published in: 2011A&A...527A..85N

Computer Science

Stars: Double And Multiple, Planets, Photometry

Scientific paper

A promising method for detecting earth-sized exoplanets is the timing analysis of a known transit. The technique allows a search for variations in either the transit duration or the center induced by the perturbation of a third body, e.g. a second planet or an exomoon. By applying this method, the TASTE (The Asiago Search for Transit Timing variations of Exoplanets) project will collect high- precision, short-cadence light curves for a selected sample of transits by using imaging differential photometry at the Asiago 1.82m telescope. The first light curves show that our project can achieve a competitive timing accuracy, as well as a significant improvement of the orbital parameters. We derived refined ephemerides for HAT-P-3b and HAT-P-14b with a timing accuracy of 11 and 25s, respectively.
(2 data files).

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