WASP-38 b
AIMS
WASP-38b is a recently by Barros et al. (2010) discovered planet around a F8 main sequence star showing a nonzero eccentricity. Radial velocity follow-up observations show that there are some points that cannot be explained by a strictly Keplerian orbit, making WASP-38 an interesting case to look for variations.
Figure caption: The original radial velocity data published by Barros et al. (2010). Upper panel: Phase folded radial velocities of WASP-38. Lower panel: The residuals from the orbital fit against time showing some deiviations (their fig. 2).
RESULTS
No updates available yet
STATUS
The campaign is starting in January 2011. If you can contribute a light curve, please let me know.
LIGHT CURVES
Reliable
| No. | Date | Epoch | Instrument | Comment |
other
| No. | Date | Instrument | Comment |
| 1 | 2011 April 24 | OSN 1.5m | only second half of transit due to weather |
CONTACT
PI: Martin Seeliger martin.seeliger@uni-jena.de
