activity
20092019
most citedDetection of titanium oxide in the atmosphere of a hot Jupiter

194 citations · 437 across the 9 of their papers we have counts for

collaborators

8 papers

astro-ph.EP201917 cited

The CARMENES search for exoplanets around M dwarfs Detection of a mini-Neptune around LSPM J2116+0234 and refinement of orbital parameters of a super-Earth around GJ 686 (BD+18 3421)

S. Lalitha, D. Baroch, J. C. Morales +34

Although M dwarfs are known for high levels of stellar activity, they are ideal targets for the search of low-mass exoplanets with the radial velocity (RV) method. We report the di…

astro-ph.EP20177 cited

Noise Sources in Photometry and Radial Velocities

M. Oshagh

The quest for Earth-like, extrasolar planets (exoplanets), especially those located inside the habitable zone of their host stars, requires techniques sensitive enough to detect th…

astro-ph.EP2017194 cited

Detection of titanium oxide in the atmosphere of a hot Jupiter

Elyar Sedaghati, Henri M. J. Boffin, Ryan J. MacDonald +6

As an exoplanet transits its host star, some of the light from the star is absorbed by the atoms and molecules in the planet's atmosphere, causing the planet to seem bigger; plotti…

astro-ph.EP201729 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.…

astro-ph.EP201737 cited

Understanding stellar activity-induced radial velocity jitter using simultaneous K2 photometry and HARPS RV measurements

M. Oshagh, N. C. Santos, P. Figueira +15

One of the best ways to improve our understanding of the stellar activity-induced signal in radial velocity (RV) measurements is through simultaneous high-precision photometric and…

astro-ph.EP201798 cited

Observational evidence for two distinct giant planet populations

N. C. Santos, V. Adibekyan, P. Figueira +9

Analysis of the statistical properties of exoplanets, together with those of their host stars, are providing a unique view into the process of planet formation and evolution. In th…