activity
20142023
most citedGlobal Climate and Atmospheric Composition of the Ultra-Hot Jupiter WASP-103b from HST and Spitzer Phase Curve Observations

221 citations · 2.6k across the 44 of their papers we have counts for

collaborators

44 papers

astro-ph.EP2023★ 9 cited

LRG-BEASTS: Evidence for clouds in the transmission spectrum of HATS-46 b

E. Ahrer, P. J. Wheatley, S. Gandhi +4

We have performed low-resolution ground-based spectroscopy of HATS-46 b in transmission, using the EFOSC2 instrument on the ESO New Technology Telescope (NTT). HATS-46 b is a highl…

astro-ph.EP2022★ 69 cited

K2 and Spitzer phase curves of the rocky ultra-short-period planet K2-141 b hint at a tenuous rock vapor atmosphere

S. Zieba, M. Zilinskas, L. Kreidberg +11

K2-141 b is a transiting, small (1.5 Re) ultra-short-period (USP) planet discovered by Kepler orbiting a K-dwarf host star every 6.7 hours. The planet's high surface temperature ma…

astro-ph.EP2022★ 31 cited

LRG-BEASTS: sodium absorption and Rayleigh scattering in the atmosphere of WASP-94A b using NTT/EFOSC2

E. Ahrer, P. J. Wheatley, J. Kirk +3

We present an optical transmission spectrum for WASP-94A b, the first atmospheric characterisation of this highly-inflated hot Jupiter. The planet has a reported radius of $1.72^{+…

astro-ph.EP2021★ 4 cited

The near-UV transit of HD 189733b with the XMM-Newton Optical Monitor

George W. King, Lía Corrales, Peter J. Wheatley +6

We present analysis of XMM-Newton Optical Monitor observations in the near-ultraviolet of HD 189733, covering twenty primary transits of its hot Jupiter planet. The transit is clea…

astro-ph.EP2021★ 74 cited

ACCESS & LRG-BEASTS: a precise new optical transmission spectrum of the ultrahot Jupiter WASP-103b

James Kirk, Ben Rackham, Ryan MacDonald +17

We present a new ground-based optical transmission spectrum of the ultrahot Jupiter WASP-103b (K). Our transmission spectrum is the result of combining five new tran…

astro-ph.EP2020★ 85 cited

An Ultra-Hot Neptune in the Neptune desert

James S. Jenkins, Matías R. Díaz, Nicolás T. Kurtovic +81

About one out of 200 Sun-like stars has a planet with an orbital period shorter than one day: an ultra-short-period planet (Sanchis-ojeda et al. 2014; Winn et al. 2018). All of the…