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: | , |
---|---|
Other Authors: | |
Format: | Article |
Language: | English |
Published: |
EDP Sciences,
2018-10-04T13:36:29Z.
|
Subjects: | |
Online Access: | Get fulltext |