activity
20162026
most citedA Giant Planet Candidate Transiting a White Dwarf

183 citations · 2k across the 70 of their papers we have counts for

collaborators

70 papers

astro-ph.SR2026

Searching for Massive Remnant Planetary System Hosts with White Dwarf Gaia XP Spectra

Lou Baya Ould Rouis, J. J. Hermes, Pierre Bergeron +5

Remnant planetary systems around massive white dwarfs () are intrinsically rare and remain poorly characterized. As the evolutionary endpoints of i…

astro-ph.EP2026★ 3 cited

Aerosols and hydrocarbons in the atmosphere of a white dwarf planet

Ryan J. MacDonald, Christopher E. O'Connor, Victoria A. Boehm +15

Most stars, including our Sun, will one day evolve into red giants and, subsequently, white dwarfs. Several planet candidates have recently been identified orbiting white dwarfs, d…

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.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.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.EP2025

Thermal Emission and Confirmation of the Frigid White Dwarf Exoplanet WD 1856+534b

Mary Anne Limbach, Andrew Vanderburg, Ryan J. MacDonald +12

We report the detection of thermal emission from and confirm the planetary nature of WD 1856+534b, the first transiting planet known to orbit a white dwarf star. Observations with…

astro-ph.SR2024

The 100 pc White Dwarf Sample in the SDSS Footprint II. A New Look at the Spectral Evolution of White Dwarfs

Mukremin Kilic, Pierre Bergeron, Simon Blouin +5

We increase the spectroscopic completeness of the 100 pc white dwarf sample in the SDSS footprint with 840 additional spectra. Our spectroscopy is 86% complete for white dwarfs hot…

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

Serendipitous observation of a white dwarf companion to a JWST/MIRI coronagraphic calibrator

Alexander Venner, Mary Anne Limbach, Mathilde Mâlin +3

We present the unplanned detection of a white dwarf companion to the star HD 218261 in mid-infrared (10-16 m) observations with JWST/MIRI. This star was observed as a calibrator…

astro-ph.SR2024★ 5 cited

Host-star and exoplanet composition: Polluted white dwarf reveals depletion of moderately refractory elements in planetary material

Claudia Aguilera-Gómez, Laura K. Rogers, Amy Bonsor +6

Planets form from the same cloud of molecular gas and dust as their host stars. Confirming if planetary bodies acquire the same refractory element composition as their natal disc d…

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.SR2024★ 43 cited

Buoyant crystals halt the cooling of white dwarf stars

Antoine Bédard, Simon Blouin, Sihao Cheng

White dwarfs are stellar remnants devoid of a nuclear energy source, gradually cooling over billions of years and eventually freezing into a solid state from the inside out. Recent…

astro-ph.EP2024★ 1 cited

The MIRI Exoplanets Orbiting White Dwarfs (MEOW) Survey: Mid-Infrared Excess Reveals a Giant Planet Candidate around a Nearby White Dwarf

Mary Anne Limbach, Andrew Vanderburg, Alexander Venner +17

The MIRI Exoplanets Orbiting White dwarfs (MEOW) Survey is a cycle 2 JWST program to search for exoplanets around dozens of nearby white dwarfs via infrared excess and direct imagi…

astro-ph.SR2024

Massive White Dwarfs in the 100 pc Sample: Magnetism, Rotation, Pulsations, and the Merger Fraction

Gracyn Jewett, Mukremin Kilic, Pierre Bergeron +6

We present a detailed model atmosphere analysis of massive white dwarfs with and K in the Montreal White Dwarf Database 100 pc sample and…

astro-ph.SR2024★ 6 cited

Fundamental Tests of White Dwarf Cooling Physics with Wide Binaries

Manuel Barrientos, Mukremin Kilic, Pierre Bergeron +3

We present follow-up spectroscopy and a detailed model atmosphere analysis of 29 wide double white dwarfs, including eight systems with a crystallized C/O core member. We use state…

astro-ph.EP2024

Absence of a Correlation between White Dwarf Planetary Accretion and Primordial Stellar Metallicity

Sydney Jenkins, Andrew Vanderburg, Allyson Bieryla +8

Over a quarter of white dwarfs have photospheric metal pollution, which is evidence for recent accretion of exoplanetary material. While a wide range of mechanisms have been propos…

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.IM2024★ 6 cited

FORECASTOR -- I. Finding Optics Requirements and Exposure times for the Cosmological Advanced Survey Telescope for Optical and UV Research mission

Isaac Cheng, Tyrone E. Woods, Patrick Côté +21

The Cosmological Advanced Survey Telescope for Optical and ultraviolet Research (CASTOR) is a proposed Canadian-led 1m-class space telescope that will carry out ultraviolet and blu…

astro-ph.SR2024★ 2 cited

White Dwarf Merger Remnants: The DAQ Subclass

Mukremin Kilic, Pierre Bergeron, Simon Blouin +3

Four years after the discovery of a unique DAQ white dwarf with a hydrogen-dominated and carbon-rich atmosphere, we report the discovery of four new DAQ white dwarfs, including two…

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.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.SR2023★ 1 cited

The Q Branch Cooling Anomaly Can Be Explained by Mergers of White Dwarfs and Subgiant Stars

Ken J. Shen, Simon Blouin, Katelyn Breivik

Gaia's exquisite parallax measurements allowed for the discovery and characterization of the Q branch in the Hertzsprung-Russell diagram, where massive C/O white dwarfs (WDs) pause…

astro-ph.SR2023

3D hydrodynamics simulations of a 3 core-helium burning star

Simon Blouin, Falk Herwig, Huaqing Mao +2

The inner structure of core-helium burning (CHeB) stars remains uncertain due to the yet unknown nature of mixing at the boundary of their cores. Large convective cores beyond a ba…

astro-ph.SR2023★ 14 cited

The ubiquity of carbon dredge-up in hydrogen-deficient white dwarfs as revealed by GALEX

Simon Blouin, Mukremin Kilic, Antoine Bédard +1

The convective dredge-up of carbon from the interiors of hydrogen-deficient white dwarfs has long been invoked to explain the presence of carbon absorption features in the spectra…