38 citations
- Institute of Astrophysics and Space SciencesPT4 papers
- Universidade do PortoPT4 papers
- University of GöttingenDE3 papers
- Instituto de Astrofísica de CanariasES2 papers
- Centre National de la Recherche ScientifiqueFR1 paper
- European Southern ObservatoryCL1 paper
- Institut de Mécanique Céleste et de Calcul des ÉphéméridesFR1 paper
- Institut de Planétologie et d'Astrophysique de GrenobleFR1 paper
- Keele UniversityGB1 paper
- Max Planck Institute for Solar System ResearchDE1 paper
- Sorbonne UniversitéFR1 paper
- Université Grenoble AlpesFR1 paper
4 papers
Constraining the oblateness of transiting planets with photometry and spectroscopy
B. Akinsanmi, S. C. C. Barros, N. C. Santos +2
Rapid planetary rotation can cause the equilibrium shape of a planet to be oblate. While planetary oblateness has mostly been probed by examining the subtle ingress and egress feat…
The correlation between photometric variability and radial velocity jitter, based on TESS and HARPS observations
S. Hojjatpanah, M. Oshagh, P. Figueira +9
The current and upcoming high precision photometric surveys such as TESS, CHEOPS, and PLATO will provide the community with thousands of new exoplanet candidates. As a consequence,…
Detectability of shape deformation in short-period exoplanets
B. Akinsanmi, S. C. C. Barros, N. C. Santos +4
Short-period planets suffer from extreme tidal forces from their parent stars causing them to deform and attain non-spherical shapes. The planet shapes, modeled here as triaxial el…
Detecting transit signatures of exoplanetary rings using SOAP3.0
B. Akinsanmi, M. Oshagh, N. C. Santos +1
CONTEXT. It is theoretically possible for rings to have formed around extrasolar planets in a similar way to that in which they formed around the giant planets in our solar system.…