Modelling secondary eclipses of Kepler exoplanets
We have selected several Kepler objects with potentially the deepest secondary eclipses. By combination of many single phased light-curves (LCs) we have produced a smooth LC with a larger SNR and made the secondary eclipses more distinct. This allowed us to measure the depth of primary and secondary...
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| Format: | Article |
| Language: | English |
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EDP Sciences
2015-01-01
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| Series: | EPJ Web of Conferences |
| Online Access: | http://dx.doi.org/10.1051/epjconf/201510106031 |