Improved precision on the radius of the nearby super-Earth 55 Cnc e

We report on new transit photometry for the super-Earth 55 Cnc e obtained with Warm Spitzer/IRAC at 4.5 μm. An individual analysis of these new data leads to a planet radius of [superscript 2.21]+0.15 [over] -0.16 R[subscript ⊕], which agrees well with the values previously derived from the MOST and...

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Bibliographic Details
Main Authors: Gillon, M. (Author), Demory, Brice-Olivier (Contributor), Benneke, Bjoern (Contributor), Valencia, Diana (Contributor), Deming, Drake (Author), Seager, Sara (Contributor), Lovis, Christophe (Author), Mayor, Michel (Author), Pepe, F. (Author), Queloz, D. (Author), Ségransan, D. (Author), Udry, S. (Author)
Other Authors: Massachusetts Institute of Technology. Department of Aeronautics and Astronautics (Contributor), Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences (Contributor)
Format: Article
Language:English
Published: EDP Sciences, 2012-12-10T13:59:39Z.
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