Detection of a transit of the super-Earth 55 Cancri e with warm Spitzer

We report on the detection of a transit of the super-Earth 55 Cnc e with warm Spitzer in IRAC’s 4.5 μm band. Our MCMC analysis includes an extensive modeling of the systematic effects affecting warm Spitzer photometry, and yields a transit depth of 410 ± 63 ppm, which translates to a planetary radiu...

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Váldodahkkit: Gillon, M., Deming, Drake, Lovis, Christophe, Cubillos, P., Stevenson, K. B., Mayor, Michel, Pepe, F., Queloz, D., Segransan, D., Udry, S., Demory, Brice-Olivier, Valencia, Diana, Seager, Sara, Benneke, Bjoern, Harrington, Joseph, III
Eará dahkkit: Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
Materiálatiipa: Artihkal
Giella:en_US
Almmustuhtton: EDP Sciences 2014
Liŋkkat:http://hdl.handle.net/1721.1/86109
https://orcid.org/0000-0002-6892-6948

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