Hot Jupiter secondary eclipses measured by Kepler
Hot-Jupiters are known to be dark in visible bandpasses, mainly because of the alkali metal absorption features. The outstanding quality of the Kepler mission photometry allows a detection (or non-detection upper limits on) giant planet secondary eclipses at visible wavelengths. We present such meas...
| Main Authors: | , |
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| Format: | Article |
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EDP Sciences
2018
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| Online Access: | http://hdl.handle.net/1721.1/118346 https://orcid.org/0000-0002-6892-6948 |