Loading...
Please wait, while we are loading the content...
BENEFITS OF GROUND-BASED PHOTOMETRIC FOLLOW-UP FOR TRANSITING EXTRASOLAR PLANETS DISCOVERED WITHKEPLERANDCoRoT
| Content Provider | Scilit |
|---|---|
| Author | Colón, Knicole D. Ford, Eric B. |
| Copyright Year | 2009 |
| Description | Journal: The Astrophysical Journal Currently, over forty transiting planets have been discovered by ground-based photometric surveys, and space-based missions like Kepler and CoRoT are expected to detect hundreds more. Follow-up photometric observations from the ground will play an important role in constraining both orbital and physical parameters for newly discovered planets, especially those with small radii (R_p less than approximately 4 Earth radii) and/or intermediate to long orbital periods (P greater than approximately 30 days). Here, we simulate transit light curves from Kepler-like photometry and ground-based observations in the near-infrared (NIR) to determine how jointly modeling space-based and ground-based light curves can improve measurements of the transit duration and planet-star radius ratio. We find that adding observations of at least one ground-based transit to space-based observations can significantly improve the accuracy for measuring the transit duration and planet-star radius ratio of small planets (R_p less than approximately 4 Earth radii) in long-period (~1 year) orbits, largely thanks to the reduced effect of limb darkening in the NIR. We also demonstrate that multiple ground-based observations are needed to gain a substantial improvement in the measurement accuracy for small planets with short orbital periods (~3 days). Finally, we consider the role that higher ground-based precisions will play in constraining parameter measurements for typical Kepler targets. Our results can help inform the priorities of transit follow-up programs (including both primary and secondary transit of planets discovered with Kepler and CoRoT), leading to improved constraints for transit durations, planet sizes, and orbital eccentricities. |
| Related Links | http://iopscience.iop.org/article/10.1088/0004-637X/703/1/1086/pdf |
| Ending Page | 1095 |
| Page Count | 10 |
| Starting Page | 1086 |
| ISSN | 0004637X |
| DOI | 10.1088/0004-637x/703/1/1086 |
| Journal | The Astrophysical Journal |
| Issue Number | 1 |
| Volume Number | 703 |
| Language | English |
| Publisher | IOP Publishing |
| Publisher Date | 2009-09-04 |
| Access Restriction | Open |
| Subject Keyword | Journal: The Astrophysical Journal Astronomy and Astrophysics Extrasolar Planet Planetary Systems Near Infrared |
| Content Type | Text |
| Resource Type | Article |
| Subject | Astronomy and Astrophysics Space and Planetary Science |