Analytic approximations for transit light curve observables, uncertainties, and covariances
The light curve of an exoplanetary transit can be used to estimate the planetary radius and other parameters of interest. Because accurate parameter estimation is a non-analytic and computationally intensive problem, it is often useful to have analytic approximations for the parameters as well as th...
| Main Authors: | , , , , |
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| Other Authors: | |
| Format: | Article |
| Language: | en_US |
| Published: |
Cambridge University Press
2010
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| Online Access: | http://hdl.handle.net/1721.1/51811 https://orcid.org/0000-0002-4265-047X |