activity
20182025
most citedEarly Release Science of the exoplanet WASP-39b with JWST NIRSpec PRISM

327 citations · 1k across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.SR2025★ 2 cited

Tracing Planetary Accretion in a 3 Gyr-old Hydrogen-Rich White Dwarf: The Extremely Polluted Atmosphere of LSPM J0207+3331

Érika Le Bourdais, Patrick Dufour, Carl Melis +7

We report the detection of 13 heavy elements (Na, Mg, Al, Si, Ca, Ti, Cr, Mn, Fe, Co, Ni, Cu, and Sr) in the photosphere of LSPM J0207+3331, a ~3 Gyr old hydrogen-rich white dwarf…

astro-ph.EP2025

Activity in White Dwarf Debris Disks I: Spitzer Legacy Reveals Variability Incompatible with the Canonical Model

Hiba Tu Noor, Jay Farihi, Scott J. Kenyon +11

This study presents all available, multi-epoch 3.6 and 4.5 m photometry from Spitzer Space Telescope observations of white dwarf debris disks, including weekly cadence observati…

astro-ph.EP2024

Seven white dwarfs with circumstellar gas discs II: Tracing the composition of exoplanetary building blocks

L. K. Rogers, A. Bonsor, S. Xu +8

This second paper presents an in-depth analysis of the composition of the planetary material that has been accreted onto seven white dwarfs with circumstellar dust and gas emission…

astro-ph.EP2024★ 1 cited

The chemistry of extra-solar materials from white dwarf planetary systems

Siyi Xu, Laura K. Rogers, Simon Blouin

White dwarf planetary systems provide a unique way to measure the bulk composition of exoplanetary material. Extrasolar asteroids/comets/moons which have survived the evolution of…

astro-ph.EP2024

Modeling Circumstellar Gas Emission around a White Dwarf Using Cloudy

Siyi Xu, Sherry Yeh, Laura. K. Rogers +9

The chemical composition of an extrasolar planet is fundamental to its formation, evolution and habitability. In this study, we explore a new way to measure the chemical compositio…

astro-ph.EP2023

Seven white dwarfs with circumstellar gas discs I: white dwarf parameters and accreted planetary abundances

L. K. Rogers, A. Bonsor, S. Xu +9

Observations of planetary material polluting the atmospheres of white dwarfs are an important probe of the bulk composition of exoplanetary material. Medium- and high-resolution op…

astro-ph.EP2023

WD0141-675: A case study on how to follow-up astrometric planet candidates around white dwarfs

Laura K. Rogers, John Debes, Richard J. Anslow +22

This work combines spectroscopic and photometric data of the polluted white dwarf WD0141-675 which has a now retracted astrometric super-Jupiter candidate and investigates the most…

astro-ph.EP2022★ 232 cited

Early Release Science of the exoplanet WASP-39b with JWST NIRISS

Adina D. Feinstein, Michael Radica, Luis Welbanks +86

Transmission spectroscopy provides insight into the atmospheric properties and consequently the formation history, physics, and chemistry of transiting exoplanets. However, obtaini…

astro-ph.EP2022★ 327 cited

Early Release Science of the exoplanet WASP-39b with JWST NIRSpec PRISM

Z. Rustamkulov, D. K. Sing, S. Mukherjee +91

Transmission spectroscopy of exoplanets has revealed signatures of water vapor, aerosols, and alkali metals in a few dozen exoplanet atmospheres. However, these previous inferences…

astro-ph.EP2022★ 18 cited

Asynchronous accretion can mimic diverse white dwarf pollutants II: water content

Marc G. Brouwers, Andrew M. Buchan, Amy Bonsor +3

Volatiles, notably water, are key to the habitability of rocky planets. The presence of water in planetary material can be inferred from the atmospheric oxygen abundances of pollut…

astro-ph.EP2022★ 193 cited

Identification of carbon dioxide in an exoplanet atmosphere

The JWST Transiting Exoplanet Community Early Release Science Team, Eva-Maria Ahrer, Lili Alderson +129

Carbon dioxide (CO2) is a key chemical species that is found in a wide range of planetary atmospheres. In the context of exoplanets, CO2 is an indicator of the metal enrichment (i.…

astro-ph.SR2021★ 35 cited

Infrared Excesses around Bright White Dwarfs from Gaia and unWISE. II

Samuel Lai, Erik Dennihy, Siyi Xu +7

Infrared excesses around white dwarf stars indicate the presence of various astrophysical objects of interest, including companions and debris disks. In this second paper of a seri…

astro-ph.EP2021★ 35 cited

Host-star and exoplanet compositions: a pilot study usinga wide binary with a polluted white dwarf

Amy Bonsor, Paula Jofre, Oliver Shorttle +3

Planets and stars ultimately form out of the collapse of the same cloud of gas. Whilst planets, and planetary bodies, readily loose volatiles, a common hypothesis is that they reta…

astro-ph.SR2020★ 6 cited

Serendipitous discovery of a dusty disc around WDJ181417.84-735459.83

E. González Egea, R. Raddi, D. Koester +8

Spectroscopic observations of white dwarfs reveal that many of them are polluted by exoplanetary material, whose bulk composition can be uniquely probed this way. We present a spec…

astro-ph.EP2020★ 40 cited

Exocomets from a Solar System Perspective

Paul A. Strøm, Dennis Bodewits, Matthew M. Knight +24

Exocomets are small bodies releasing gas and dust which orbit stars other than the Sun. Their existence was first inferred from the detection of variable absorption features in ste…

astro-ph.EP2020★ 20 cited

Near-infrared variability in dusty white dwarfs: tracing the accretion of planetary material

Laura K. Rogers, Siyi Xu, Amy Bonsor +4

The inwards scattering of planetesimals towards white dwarfs is expected to be a stochastic process with variability on human time-scales. The planetesimals tidally disrupt at the…

astro-ph.EP2018★ 48 cited

Dust Production and Depletion in Evolved Planetary Systems

J. Farihi, R. van Lieshout, P. W. Cauley +15

The infrared dust emission from the white dwarf GD 56 is found to rise and fall by 20% peak-to-peak over 11.2 yr, and is consistent with ongoing dust production and depletion. It i…

astro-ph.EP2018★ 43 cited

Infrared Variability of Two Dusty White Dwarfs

Siyi Xu, Kate Y. L. Su, Laura Rogers +11

The most heavily polluted white dwarfs often show excess infrared radiation from circumstellar dust disks, which are modeled as a result of tidal disruption of extrasolar minor pla…