activity
19992021
most citedAtomic iron and titanium in the atmosphere of the exoplanet KELT-9b

252 citations · 1.3k across the 26 of their papers we have counts for

collaborators

26 papers

astro-ph.EP2021★ 22 cited

The GAPS Programme with HARPS-N at TNG. XXXI. The WASP-33 system revisited with HARPS-N

F. Borsa, A. F. Lanza, I. Raspantini +33

[abridged] We analyse four transits of WASP-33b observed with the optical high-resolution HARPS-N spectrograph to confirm its nodal precession, study its atmosphere and investigate…

astro-ph.EP2021★ 1 cited

TOI-1634 b: an Ultra-Short Period Keystone Planet Sitting Inside the M Dwarf Radius Valley

R. Cloutier, D. Charbonneau, K. G. Stassun +63

Studies of close-in planets orbiting M dwarfs have suggested that the M dwarf radius valley may be well-explained by distinct formation timescales between enveloped terrestrials, a…

astro-ph.EP2020★ 136 cited

Neutral Iron Emission Lines From The Day-side Of KELT-9b -- The GAPS Programme With HARPS-N At TNG XX

L. Pino, J. M. Désert, M. Brogi +47

We present the first detection of atomic emission lines from the atmosphere of an exoplanet. We detect neutral iron lines from the day-side of KELT-9b (Teq 4, 000 K). We com…

astro-ph.EP2020★ 97 cited

A pair of TESS planets spanning the radius valley around the nearby mid-M dwarf LTT 3780

Ryan Cloutier, Jason D. Eastman, Joseph E. Rodriguez +84

We present the confirmation of two new planets transiting the nearby mid-M dwarf LTT 3780 (TIC 36724087, TOI-732, , , =0.374 R, =0.401 M$_{\…

astro-ph.EP2019★ 47 cited

Pluto's lower atmosphere and pressure evolution from ground-based stellar occultations, 1988-2016

E. Meza, B. Sicardy, M. Assafin +167

Context. Pluto's tenuous nitrogen (N2) atmosphere undergoes strong seasonal effects due to high obliquity and orbital eccentricity, and has been recently (July 2015) observed by th…

astro-ph.EP2018★ 252 cited

Atomic iron and titanium in the atmosphere of the exoplanet KELT-9b

H. Jens Hoeijmakers, David Ehrenreich, Kevin Heng +10

The chemical composition of an exoplanet is a key ingredient in constraining its formation history. Iron is the most abundant transition metal, but has never been directly detected…