collaborators

6 papers

astro-ph.SR2026

A Detailed Model Atmosphere Analysis of Cool White Dwarfs in DESI DR1

Mukremin Kilic, Pierre Bergeron, Simon Blouin +9

We present a detailed model atmosphere analysis of cool white dwarfs in the Dark Energy Spectroscopic Instrument Data Release 1 (DESI DR1). Our sample includes 25,642 unique target…

astro-ph.SR2026

Dormant black hole candidates from Gaia DR3 summary diagnostics

Johanna Müller-Horn, Hans-Walter Rix, Kareem El-Badry +4

We present a rigorous identification of candidates for dormant black holes (BHs) and neutron stars (NSs) in binaries using summary statistics from Gaia DR3, rather than full orbita…

astro-ph.SR2026

Long-term eclipse time variations in white dwarf binaries

Amalie Yates, S. G. Parsons, A. J. Brown +15

The overwhelming majority of eclipsing white dwarf (WD) binary systems show quasi-periodic variations in eclipse timings on many year timescales. Currently, the mechanism behind th…

astro-ph.SR2026

A Detailed Model Atmosphere Analysis of Hot White Dwarfs in DESI DR1

Mukremin Kilic, Pierre Bergeron, Adam Moss +6

We present a detailed model atmosphere analysis of hot white dwarfs in the Dark Energy Spectroscopic Instrument (DESI) Data Release 1. Our sample includes 19,321 unique targets wit…

astro-ph.SR2025

The ZZ Ceti Instability Strip for The Most Massive White Dwarf Pulsators

Gracyn Jewett, Mukremin Kilic, Adam Moss +10

We present time-series photometry of 31 massive DA white dwarfs with within the ZZ Ceti instability strip from the Montreal White Dwarf Database 100 pc sampl…

astro-ph.SR2025

The Fraction of Distilled White Dwarfs with Long-Lived Habitable Zones

Manuel Barrientos, Mukremin Kilic, Simon Blouin +3

After carbon and oxygen, Ne is the most abundant element in white dwarf interiors. As C/O white dwarfs (WDs) crystallize, they are predicted to go through a distillation pro…