activity
20142026
most citedNo Thermal Inversion and a Solar Water Abundance for the Hot Jupiter HD209458b from HST WFC3 Emission Spectroscopy

174 citations · 920 across the 28 of their papers we have counts for

collaborators
Showing 2025Show all

6 papers · 1 filter

astro-ph.EP2025

JWST TRAPPIST-1 e/b Program: Motivation and first observations

Natalie H. Allen, Néstor Espinoza, V. A. Boehm +24

One of the forefront goals in the field of exoplanets is the detection of an atmosphere on a temperate terrestrial exoplanet, and among the best suited systems to do so is TRAPPIST…

astro-ph.EP2025★ 2 cited

Hot Rocks Survey IV: Emission from LTT 3780 b is consistent with a bare rock

Natalie H. Allen, Néstor Espinoza, Hannah Diamond-Lowe +19

It is an open question whether small planets around M dwarfs are able to maintain atmospheres. The Hot Rocks Survey aims to address this question by observing 9 rocky exoplanets or…

astro-ph.EP2025

Do Rocky Planets around M Stars Have Atmospheres? A Statistical Approach to the Cosmic Shoreline

Jegug Ih, Eliza M. -R. Kempton, Hannah Diamond-Lowe +6

Answering the question "do rocky exoplanets around M stars have atmospheres?" is a key science goal of the JWST mission, with 500 hours of Director's Discretionary Time (DDT) award…

astro-ph.EP2025★ 20 cited

Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels

Mark Fortune, Neale P. Gibson, Hannah Diamond-Lowe +14

Time-series photometry at mid-infrared wavelengths is becoming a common technique to search for atmospheres around rocky exoplanets. This method constrains the brightness temperatu…

astro-ph.EP2025★ 23 cited

Hot Rocks Survey II: The thermal emission of TOI-1468 b reveals a hot bare rock

E. A. Meier Valdés, B. -O. Demory, H. Diamond-Lowe +17

Terrestrial exoplanets orbiting nearby small, cool stars known as M dwarfs are well suited for atmospheric characterisation. Given the strong XUV irradiation from M dwarf host star…

astro-ph.EP2025

Limits on the atmospheric metallicity and aerosols of the sub-Neptune GJ 3090 b from high-resolution CRIRES+ spectroscopy

Luke T. Parker, João M. Mendonça, Hannah Diamond-Lowe +9

The sub-Neptune planets have no solar system analogues, and their low bulk densities suggest thick atmospheres containing degenerate quantities of volatiles and H/He, surrounding c…