activity
20172025
most citedDetection of Fe I in the atmosphere of the ultra-hot Jupiter WASP-121b, and a new likelihood-based approach for Doppler-resolved spectroscopy

210 citations · 471 across the 12 of their papers we have counts for

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Showing 2020Show all

4 papers · 1 filter

astro-ph.EP2020★ 35 cited

Is TiO emission present in the ultra-hot Jupiter WASP-33b? A reassessment using the improved ExoMol Toto line list

Dilovan B. Serindag, Stevanus K. Nugroho, Paul Mollière +3

[abridged] Efficient absorption of stellar UV and visible radiation by TiO and VO is predicted to drive temperature inversions in the upper atmospheres of hot Jupiters. However, fe…

astro-ph.EP2020★ 44 cited

Arid or Cloudy: Characterizing the Atmosphere of the super-Earth 55 Cancri e using High-Resolution Spectroscopy

Abhinav Jindal, Ernst J. W. de Mooij, Ray Jayawardhana +6

The nearby super-Earth 55 Cnc e orbits a bright (V = 5.95 mag) star with a period of ~ 18 hours and a mass of ~ 8 Earth masses. Its atmosphere may be water-rich and have a large sc…

astro-ph.EP2020★ 33 cited

Search for TiO and Optical Night-side Emission from the Exoplanet WASP-33b

Miranda K. Herman, Ernst J. W. de Mooij, Ray Jayawardhana +1

With a temperature akin to an M-dwarf, WASP-33b is among the hottest Jupiters known, making it an ideal target for high-resolution optical spectroscopy. By analyzing both transmiss…

astro-ph.EP2020★ 210 cited

Detection of Fe I in the atmosphere of the ultra-hot Jupiter WASP-121b, and a new likelihood-based approach for Doppler-resolved spectroscopy

Neale P. Gibson, Stephanie Merritt, Stevanus K. Nugroho +10

High-resolution Doppler-resolved spectroscopy has opened up a new window into the atmospheres of both transiting and non-transiting exoplanets. Here, we present VLT/UVES observatio…