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Fig. 4.— Radial velocity measurements from Pont et al. (2004) together with the best fit (solid line), and the corresponding ±1σ curves (dotted lines). Also shown is the fit for e = 0 (dashed line).
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Journal Article
•
DOI
•
Detection of period variations in extrasolar transiting planet OGLE-TR-111b
[...]
Rodrigo F. Díaz
1
,
Patricio Rojo
2
,
Mario Daniel Melita
1
,
Sergio Hoyer
2
,
Dante Minniti
3
,
Pablo J. D. Mauas
1
,
Maria Teresa Ruiz
2
- Show less
+3 more
•
Institutions (3)
University of Buenos Aires
1
,
University of Chile
2
,
Pontifical Catholic University of Chile
3
06 Jun 2008
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arXiv: Astrophysics