output
20172024
most citedQuality at a Glance: An Audit of Web-Crawled Multilingual Datasets

177 citations

Showing astro-ph.EPShow all

5 papers · 1 filter

astro-ph.EP2020★ 10 cited

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…

astro-ph.EP2020★ 38 cited

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,…

astro-ph.EP2020★ 45 cited

Can planetary rings explain the extremely low density of HIP 41378f?

B. Akinsanmi, N. C. Santos, J. P. Faria +4

The presence of rings around a transiting planet can cause its radius to be overestimated and lead to an underestimation of its density if the mass is known. We employ a Bayesian f…

astro-ph.EP2018★ 34 cited

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…

astro-ph.EP2017★ 29 cited

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.…