activity
20172026
most citedA Sub-Neptune Exoplanet with a Low-Metallicity Methane-Depleted Atmosphere and Mie-Scattering Clouds

238 citations · 1.7k across the 68 of their papers we have counts for

collaborators
Showing 2022Show all

8 papers · 1 filter

astro-ph.EP202259 cited

Water and an escaping helium tail detected in the hazy and methane-depleted atmosphere of HAT-P-18b from JWST NIRISS/SOSS

Guangwei Fu, Néstor Espinoza, David K. Sing +11

JWST is here. The early release observation program (ERO) provides us with the first look at the scientific data and the spectral capabilities. One of the targets from ERO is HAT-P…

astro-ph.SR20223 cited

Near-infrared spectra of the inflated post-common envelope brown dwarf NLTT 5306B

Cam Buzard, Sarah Casewell, Joshua Lothringer +1

NLTT 5306 is a post-common envelope binary made up of a white dwarf host and brown dwarf companion that has shown evidence of inflation and active mass donation despite not filling…

astro-ph.EP20222 cited

UV Absorption by Silicate Cloud Precursors in Ultra-hot Jupiter WASP-178b

Joshua D. Lothringer, David K. Sing, Zafar Rustamkulov +6

Aerosols have been found to be nearly ubiquitous in substellar atmospheres. The precise temperature at which these aerosols begin to form in exoplanets has yet to be observationall…

astro-ph.SR20222 cited

Sunbathing under white light -- 3D modelling of brown dwarf - white dwarf atmospheres with strong UV irradiation

Elspeth K. H. Lee, Joshua D. Lothringer, Sarah L. Casewell +3

The atmospheres of brown dwarfs orbiting in close proximity to their parent white dwarf represent some of the most extreme irradiated environments known. Understanding their comple…

astro-ph.EP20225 cited

The Hubble PanCET program: Emission spectrum of hot Jupiter HAT-P-41b

Guangwei Fu, David K. Sing, Drake Deming +6

We present the most complete emission spectrum for inflated hot Jupiter HAT-P-41b combining new HST WFC/G141 spectrum from the Hubble Panchromatic Comparative Exoplanet Treasury (P…

astro-ph.EP202244 cited

Evidence that the Hot Jupiter WASP-77 A b Formed Beyond Its Parent Protoplanetary Disk's H2O Ice Line

Henrique Reggiani, Kevin C. Schlaufman, Brian F. Healy +2

Idealized protoplanetary disk and giant planet formation models have been interpreted to suggest that a giant planet's atmospheric abundances can be used to infer its formation loc…