activity
20122026
most citedGaseous Material Orbiting the Polluted, Dusty White Dwarf HE1349-2305

75 citations · 120 across the 17 of their papers we have counts for

collaborators

21 papers

astro-ph.IM2026

Early Exploration of the Scientific Discovery Space for the Habitable Worlds Observatory

Courtney D. Dressing, Danica Adams, Evelyne Alecian +324

The Habitable Worlds Observatory (HWO) is a future NASA flagship mission concept identified by the Astro2020 Decadal Survey as the highest priority for large space missions. HWO sh…

astro-ph.EP2026

Tracing outer planetary systems through white dwarf pollution in wide binaries

Carolina Lizana-Vidal, Claudia Aguilera-Gómez, Laura K. Rogers +5

White dwarf (WD) atmospheric metal pollution provides strong evidence for the presence of remnant planetary material and it can be used as an indirect tracer of outer planetary sys…

astro-ph.SR2026

Spectroscopic Monitoring of Metal Lines in Polluted White Dwarfs

Laura K. Rogers, Michael M. Shara, Amy Bonsor +12

The disruption and accretion of planetary material onto white dwarfs is expected to be inherently dynamic and stochastic, potentially driving variability in the accretion rate and…

astro-ph.IM2026

From Hubble to HWO: Bridging the Frontier of White Dwarf Exoplanet Science

Laura K. Rogers, Siyi Xu, Martin Barstow +20

White dwarf stars, the endpoint of stellar evolution for 97% of stars in our Milky Way, offer a unique and powerful window into the bulk elemental composition of rocky exoplanetary…

astro-ph.SR2026

High Velocity Circumstellar Gas Orbiting a White Dwarf Star

B. Zuckerman, Érika Le Bourdais, Beth L. Klein +6

Numerous white dwarf stars are known to be orbited by disks of gas and dust. To date, broad, about 300 km s-1 wide, gaseous circumstellar absorption features have only been reporte…

astro-ph.SR2026

The MIRI Excess around Degenerates (MEAD) Survey II: A Probable Planet detected via IR Excess around WD 0644+025

Sabrina Poulsen, John Debes, Ashley Messier +14

The MIRI Excess Around Degenerates (MEAD) Survey is a cycle 2 JWST program designed to image nearby white dwarfs with MIRI at 10 and 15 microns. This survey targeted 56 white dwarf…

astro-ph.SR2025

The MIRI Excesses around Degenerates (MEAD) Survey I: A candidate cold brown dwarf in orbit around the nearby white dwarf 2MASS J09424023-4637176

Loïc Albert, Sabrina R. Poulsen, Érika Le Bourdais +17

The MIRI Excesses Around Degenerates Survey is a Cycle 2 James Webb Space Telescope (JWST) Survey program designed to image nearby white dwarfs in the mid-IR with the MIRI imaging…

astro-ph.EP2025★ 2 cited

Do White Dwarfs Sample Water-Rich Planetary Material?

Isabella L. Trierweiler, Carl Melis, Érika Le Bourdais +9

Polluted white dwarfs offer a unique way to directly probe the compositions of exoplanetary bodies. We examine the water content of accreted material using the oxygen abundances of…

astro-ph.SR2025

An All-sky Survey of White Dwarf Merger Remnants: Far-UV is the Key

Mukremin Kilic, Pierre Bergeron, Warren R. Brown +5

The majority of merging white dwarfs leave behind a white dwarf remnant. Hot/warm DQ white dwarfs with carbon-rich atmospheres have high masses and unusual kinematics. All evidence…

astro-ph.IM2025

White dwarfs as probes of extrasolar planet compositions and fundamental astrophysics

Siyi Xu, Martin Barstow, Andy Buchan +2

White dwarfs represent the most common end stage of stellar evolution and are important for a range of astrophysical questions. The high-resolution ultraviolet spectroscopic capabi…

astro-ph.EP2025★ 1 cited

Metal Polluted White Dwarfs with 21 μm IR excesses from JWST/MIRI: Planets or Dust?

John H. Debes, Sabrina Poulsen, Ashley Messier +13

White dwarfs with metal pollution are caused by the accretion of rocky dust from tidally disrupted minor bodies and are signposts for planetary systems. These minor bodies are pert…

astro-ph.EP2025

A Machine-Learning Compositional Study of Exoplanetary Material Accreted Onto Five Helium-Atmosphere White Dwarfs with

Mariona Badenas-Agusti, Siyi Xu, Andrew Vanderburg +8

We present the first application of the Machine Learning (ML) pipeline to determine the physical parameters and photospheric composition of five metal-polluted H…

astro-ph.EP2024

The Origins of Lithium Enhancement in Polluted White Dwarfs

Benjamin C. Kaiser, J. Christopher Clemens, Simon Blouin +4

The bulk abundances of exoplanetesimals can be measured when they are accreted by white dwarfs. Recently, lithium from the accretion of exoplanetesimals was detected in relatively…

astro-ph.SR2024★ 1 cited

JWST Resolves CIA Features in White Dwarfs

Simon Blouin, Mukremin Kilic, Loic Albert +2

Infrared-faint white dwarfs are cool white dwarfs exhibiting significant infrared flux deficits, most often attributed to collision-induced absorption (CIA) from H-He in mixed…

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.SR2024★ 2 cited

PHL 5038AB: Is the brown dwarf causing pollution of its white dwarf host star?

S. L. Casewell, J. Debes, T. J. Dupuy +9

We present new results on PHL 5038AB, a widely separated binary system composed of a white dwarf and a brown dwarf, refining the white and brown dwarf parameters and determining th…

astro-ph.IM2024

cecilia: A Machine Learning-Based Pipeline for Measuring Metal Abundances of Helium-rich Polluted White Dwarfs

M. Badenas-Agusti, J. Viaña, A. Vanderburg +4

Over the past several decades, conventional spectral analysis techniques of polluted white dwarfs have become powerful tools to learn about the geology and chemistry of extrasolar…

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.SR2023

Detection and Preliminary Characterisation of Polluted White Dwarfs from Gaia EDR3 and LAMOST

Mariona Badenas-Agusti, Andrew Vanderburg, Simon Blouin +4

We present a catalogue of 62 polluted white dwarfs observed by the 9th Low-Resolution Data Release of the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST LRS DR9v…

astro-ph.EP2020★ 39 cited

Lithium pollution of a white dwarf records the accretion of an extrasolar planetesimal

Benjamin C. Kaiser, J. Christopher Clemens, Simon Blouin +4

Tidal disruption and subsequent accretion of planetesimals by white dwarfs can reveal the elemental abundances of rocky bodies in exoplanetary systems. Those abundances provide inf…

astro-ph.SR2012★ 75 cited

Gaseous Material Orbiting the Polluted, Dusty White Dwarf HE1349-2305

Carl Melis, P. Dufour, J. Farihi +6

We present new spectroscopic observations of the polluted, dusty, helium-dominated atmosphere white dwarf star HE1349-2305. Optical spectroscopy reveals weak CaII infrared triplet…