Extrasolar Planet Transit Light Curves and a Method to Select the Best Planet Candidates for Mass Follow-up

S. Seager; G. Mallen-Ornelas

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arXiv · astro-ph/0210076

Extrasolar Planet Transit Light Curves and a Method to Select the Best Planet Candidates for Mass Follow-up

S. Seager·G. Mallen-Ornelas

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Abstract

A unique analytical solution of planet and star parameters can be derived from an extrasolar planet transit light curve under a number of assumptions. This analytical solution can be used to choose the best planet transit candidates for radial velocity follow-up measurements, with or without a known spectral type. In practice, high photometric precision (< 0.005 mag) and high time sampling (< 5 minutes) are needed for this method. See Seager & Mallen-Ornelas (2002) for full details.

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S. Seager, G. Mallen-Ornelas. 2002-10-02. Extrasolar Planet Transit Light Curves and a Method to Select the Best Planet Candidates for Mass Follow-up. https://arxiv.org/abs/astro-ph/0210076

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