collaborators

10 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

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.SR2026

White Dwarf Merger Remnants with Cooling Delays on the Q Branch Lack Strong Magnetism

Lou Baya Ould Rouis, J. J. Hermes, Joseph A. Guidry +8

A population of anomalous ultra-massive white dwarfs discovered with Gaia, often referred to as the Q branch, show high (multi-Gyr) cooling delays produced by exotic physical mecha…

astro-ph.SR2025

Multiperiodic pulsations of the unique DAQ white dwarf J0551+4135: insights into a merger remnant

Murat Uzundag, Mukremin Kilic, Francisco C. De Gerónimo +7

2MASS J05513444+4135297 (herafter J0551+4135) is the only pulsating DAQ white dwarf known with a carbon and hydrogen atmosphere. Its unusual atmospheric composition and kinematics…

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

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…