A New 24 μm Phase Curve for υ Andromedae b

A New 24 μm Phase Curve for υ Andromedae b

We report the detection of 24 μm variations from the planet-hosting υ Andromedae system consistent with the orbital periodicity of the system's innermost planet, υ And b. We find a peak-to-valley phase curve amplitude of 0.00130 times the mean system flux. Using a simple model with two hemisphe...

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Bibliographic Details
Main Authors: Crossfield, Ian J., Hansen, Brad M. S., Cho, James Y. -K., Deming, Drake, Menou, Kristen, Seager, Sara, Harrington, Joseph, III
Other Authors: Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
Format: Article
Language:en_US
Published: IOP Publishing 2012
Online Access:http://hdl.handle.net/1721.1/74153
https://orcid.org/0000-0002-6892-6948

Internet

http://hdl.handle.net/1721.1/74153
https://orcid.org/0000-0002-6892-6948

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