Add to ORKGTransiting planet discoveries have largely been restricted to the short-period or low-periastron distance regimes due to the bias inherent in the geometric transit probability. Through the refinement of planetary orbital parameters, and hence reducing the size of transit windows, long-period planets become feasible targets for photometric follow-up. Here we describe the TERMS project that is monitoring these host stars at predicted transit times
A transiting exoplanet is a planet that passes in front of its host star and blocks a fraction of th...
Transit events of extrasolar planets offer a wealth of information for planetary characterization. H...
In 2015, K2 observations of the bright (V = 8.9, K = 7.7) star HIP 41378 revealed a rich system of a...
Transiting planet discoveries have yielded a plethora of information towards understanding the struc...
Transiting planet discoveries have largely been restricted to the short-period or low-periastron dis...
The orbital parameters of extrasolar planets have a significant impact on the probability that the p...
11 pages, 5 figures, to be published in PASP, comments welcomeHere, we introduce an online tool for ...
The Transit Ephemeris Refinement and Monitoring Survey conducts radial velocity and photometric moni...
Transiting exoplanets provide access to data to study the mass-radius relation and internal structur...
The Transit Ephemeris Refinement and Monitoring Survey conducts radial velocity and photometric moni...
Kepler will monitor a sufficient number of stars that it is likely to detect single transits of plan...
The search for planets outside our solar system is vital for models of planetary formation. However,...
The inventory of known extrasolar planets (planets orbiting stars other than our Sun) has grown expl...
The exoplanet yield of the TESS mission is expected to surpass that of Kepler, and the relatively br...
The timing and duration of exoplanet transits has a dependency on observer position due to parallax....
A transiting exoplanet is a planet that passes in front of its host star and blocks a fraction of th...
Transit events of extrasolar planets offer a wealth of information for planetary characterization. H...
In 2015, K2 observations of the bright (V = 8.9, K = 7.7) star HIP 41378 revealed a rich system of a...
Transiting planet discoveries have yielded a plethora of information towards understanding the struc...
Transiting planet discoveries have largely been restricted to the short-period or low-periastron dis...
The orbital parameters of extrasolar planets have a significant impact on the probability that the p...
11 pages, 5 figures, to be published in PASP, comments welcomeHere, we introduce an online tool for ...
The Transit Ephemeris Refinement and Monitoring Survey conducts radial velocity and photometric moni...
Transiting exoplanets provide access to data to study the mass-radius relation and internal structur...
The Transit Ephemeris Refinement and Monitoring Survey conducts radial velocity and photometric moni...
Kepler will monitor a sufficient number of stars that it is likely to detect single transits of plan...
The search for planets outside our solar system is vital for models of planetary formation. However,...
The inventory of known extrasolar planets (planets orbiting stars other than our Sun) has grown expl...
The exoplanet yield of the TESS mission is expected to surpass that of Kepler, and the relatively br...
The timing and duration of exoplanet transits has a dependency on observer position due to parallax....
A transiting exoplanet is a planet that passes in front of its host star and blocks a fraction of th...
Transit events of extrasolar planets offer a wealth of information for planetary characterization. H...
In 2015, K2 observations of the bright (V = 8.9, K = 7.7) star HIP 41378 revealed a rich system of a...