Add to ORKGTransiting planet discoveries have yielded a plethora of information towards understanding the structure and atmospheres of extra-solar planets. These discoveries have 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 parmaters, and hence reducing the size of transit windows, long-period planets become feasible targets for photometric follow-up. Here we describe the TERMS project which is monitoring these host stars at predicted transit times
Context. Transiting planetary systems allow us to extract geometrical information, e.g., the angle ϵ...
The transit signature of exoplanets provides an avenue through which characterization of exoplanetar...
The Kepler mission has been the catalyst for discovery of nearly 5,000 confirmed and candidate exopl...
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...
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...
The Transit Ephemeris Refinement and Monitoring Survey conducts radial velocity and photometric moni...
The inventory of known extrasolar planets (planets orbiting stars other than our Sun) has grown expl...
We report follow-up observations of transiting exoplanets that have either large uncertainties (>...
Transiting exoplanets provide access to data to study the mass-radius relation a...
Kepler will monitor a sufficient number of stars that it is likely to detect single transits of plan...
11 pages, 5 figures, to be published in PASP, comments welcomeHere, we introduce an online tool for ...
In 2015, K2 observations of the bright (V = 8.9, K = 7.7) star HIP 41378 revealed a rich system of a...
Context. Transiting planetary systems allow us to extract geometrical information, e.g., the angle ϵ...
The transit signature of exoplanets provides an avenue through which characterization of exoplanetar...
The Kepler mission has been the catalyst for discovery of nearly 5,000 confirmed and candidate exopl...
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...
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...
The Transit Ephemeris Refinement and Monitoring Survey conducts radial velocity and photometric moni...
The inventory of known extrasolar planets (planets orbiting stars other than our Sun) has grown expl...
We report follow-up observations of transiting exoplanets that have either large uncertainties (>...
Transiting exoplanets provide access to data to study the mass-radius relation a...
Kepler will monitor a sufficient number of stars that it is likely to detect single transits of plan...
11 pages, 5 figures, to be published in PASP, comments welcomeHere, we introduce an online tool for ...
In 2015, K2 observations of the bright (V = 8.9, K = 7.7) star HIP 41378 revealed a rich system of a...
Context. Transiting planetary systems allow us to extract geometrical information, e.g., the angle ϵ...
The transit signature of exoplanets provides an avenue through which characterization of exoplanetar...
The Kepler mission has been the catalyst for discovery of nearly 5,000 confirmed and candidate exopl...