THE TRANSIT LIGHT CURVE PROJECT. XIV. CONFIRMATION OF ANOMALOUS RADII FOR THE EXOPLANETS TRES-4b, HAT-P-3b, AND WASP-12b
We present transit photometry of three exoplanets, TrES-4b, HAT-P-3b, and WASP-12b, allowing for refined estimates of the systems' parameters. TrES-4b and WASP-12b were confirmed to be "bloated" planets, with radii of 1.706 [plus-minus] 0.056R [subscript Jup] and 1.736 [plus-minus] 0....
Main Authors: | , , , , , , |
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Other Authors: | |
Format: | Article |
Language: | en_US |
Published: |
Institute of Physics Publishing
2012
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Online Access: | http://hdl.handle.net/1721.1/72421 https://orcid.org/0000-0002-4265-047X |