WASP-21 b
AIMS
WASP-21b was found by Bouchy et al. (2010). Its host star is a G3 main sequence star. Planetary parameters of a radius of 1.07 jupiter radii and a mass of 0.3 jupiter masses were derived. Though the eccentricity was derived to be very small and therefore fixed to zero in the models, the radial velocity analysis shows some interesting deviations from the fit.
Figure caption: The original phase folded radial velocity data of WASP-21 published by Bouchy et al. (2010) (their fig. 3).
RESULTS
No updates available yet
STATUS
The campaign started in 2011 and is continuing in 2012. If you can contribute a light curve, please let me know.
LIGHT CURVES
(update: 2013-03-18)
Reliable
| No. | Date | Epoch | Sight | Comment |
| 1 | 2011 Aug 24 | 244 | Swarthmore 0.6m | |
| 2 | 2012 Aug 16 | 327 | Trebur 1.4m |
Other
| No. | Date | Sight | Comment |
| 1 | 2011 Aug 24 | Gettysburg 0.4m | only first half of transit usable |
| 2 | 2012 Mar 07 | Stara Lesna 0.5m | |
| 3 | 2012 May 28 | Cerro Armazones 0.15m | wrong pointing |
| 4 | 2012 Oct 20 | Tubitak 1.0m |
CONTACT
PI: Martin Seeliger martin.seeliger@uni-jena.de
