- Abstract:
-
With more than 80 transits observed in the CoRoT lightcurve with a cadence of 32 s, CoRoT-Exo-2b provides an excellent case to search for the secondary eclipse of the planet, with an expected signal of less than 10-4 in relative flux. The activity of the star causes a modulation on the flux that makes the detection of this signal challenging. We describe the technique used to seek for the secondary eclipse, that leads to a tentative 2.5σ detection of a 5.5×10-5 eclipse. If the effect of the s...
Expand abstract - Publication status:
- Published
- Publisher copy:
- 10.1017/S1743921308026276
-
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- Volume:
- 4
- Issue:
- 253
- Pages:
- 91-96
- Publication date:
- 2009
- DOI:
- EISSN:
-
1743-9221
- ISSN:
-
1743-9213
- URN:
-
uuid:866c8462-bd52-4446-8319-9600eb68aa70
- Source identifiers:
-
158513
- Local pid:
- pubs:158513
- ISBN:
- 978-0-521-88984-1
- Copyright date:
- 2009
Conference
Searching for the secondary eclipse of CoRoT-Exo-2b and its transit timing variations
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