activity
20242026
most citedAerosols and hydrocarbons in the atmosphere of a white dwarf planet

3 citations · 3 across the 2 of their papers we have counts for

collaborators

11 papers

astro-ph.EP20263 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…