Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Both sides previous revision Previous revision
Next revision
Previous revision
wasp38 [2011/02/18 14:00]
Martin Seeliger
wasp38 [2017/02/21 10:23] (current)
Line 1: Line 1:
 +===== WASP-38 b =====
 +
 +=== AIMS ===
 +
 +WASP-38b is a recently by [[http://​adsabs.harvard.edu/​abs/​2011A%26A...525A..54B|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. \\
 +
 +{{ :​wasp-38_rv.gif |}} \\
 +
 +**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>​
 +
 +
  
 
Recent changes RSS feed Donate Powered by PHP Valid XHTML 1.0 Valid CSS Driven by DokuWiki