activity
20162026
most citedThe 40 pc sample of white dwarfs from Gaia

88 citations · 152 across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.IM2026

White dwarf planetary systems in the ultraviolet

Jamie Williams, Amy Bonsor, Boris Gänsicke +9

Almost every known planet host will evolve into a white dwarf, and the surviving planetary material will continue to orbit this stellar remnant. Asteroids perturbed onto star-grazi…

astro-ph.SR2026

Detection of a weak magnetic field in the Balmer emission line white dwarf WDJ1653-1001

Abbigail Elms, Stefano Bagnulo, Pier-Emmanuel Tremblay +8

The small DAHe and DAe spectral classes comprise isolated, hydrogen-dominated atmosphere white dwarfs that exhibit variable photometric flux and Balmer line emission. These mysteri…

astro-ph.SR2026

Classifying white dwarfs from multi-object spectroscopy surveys with machine learning

James Munday, Pier-Emmanuel Tremblay, Ingrid Pelisoli +5

With tens to hundreds of spectra of white dwarfs being taken each night from multi-object spectroscopic surveys, automated spectral classification is essential as part of efficient…

astro-ph.IM2025

The Galactic White Dwarf Population

Santiago Torres, Roberto Raddi, Alberto Rebassa-Mansergas +15

The ESA Gaia mission has revolutionized our understanding of the white dwarf population, delivering an unprecedented census of these nearby remnants and revealing previously unseen…

astro-ph.SR2025

The DBL Survey II: towards a mass-period distribution of double white dwarf binaries

James Munday, Ingrid Pelisoli, Pier-Emmanuel Tremblay +14

Double white dwarf binaries are an important remnant of binary evolution as they are possible type Ia supernova progenitors and strong sources of gravitational waves in the low-fre…

astro-ph.SR2025★ 8 cited

A super-Chandrasekhar mass type Ia supernova progenitor at 49 pc set to detonate in 23 Gyr

James Munday, Ruediger Pakmor, Ingrid Pelisoli +9

Double white dwarf binaries are a leading explanation to the origin of type Ia supernovae, but no system exceeding the Chandrasekhar mass limit (1.4 M) has been found that…

astro-ph.SR2025

Comparison of methods used to derive the Galactic star formation history from white dwarf samples

Emily K. Roberts, Pier-Emmanuel Tremblay, Mairi W. O'Brien +4

We compare three methods of deriving the local Galactic star formation history, using as a benchmark the Gaia-defined 40 pc white dwarf sample, currently the largest volume complet…

astro-ph.SR2024★ 5 cited

A network of cooler white dwarfs as infrared standards for flux calibration

Abbigail K. Elms, Nicola Pietro Gentile Fusillo, Pier-Emmanuel Tremblay +6

The accurate flux calibration of observational data is vital for astrophysics and cosmology because absolute flux uncertainties of stellar standards propagate into scientific resul…

astro-ph.SR2024

Constraints on Remnant Planetary Systems as a Function of Main-Sequence Mass with HST/COS

Lou Baya Ould Rouis, J. J. Hermes, Boris T. Gänsicke +8

As the descendants of stars with masses less than 8 M on the main sequence, white dwarfs provide a unique way to constrain planetary occurrence around intermediate-mass s…

astro-ph.SR2024★ 1 cited

The Gaia Ultracool Dwarf Sample -- IV. GTC/OSIRIS optical spectra of Gaia late-M and L dwarfs

W. J. Cooper, H. R. A. Jones, R. L. Smart +20

As part of our comprehensive, ongoing characterisation of the low-mass end of the main sequence in the Solar neighbourhood, we used the OSIRIS instrument at the 10.4 m Gran Telesco…

astro-ph.SR2024

The DBL Survey I: discovery of 34 double-lined double white dwarf binaries

James Munday, Ingrid Pelisoli, P. E. Tremblay +8

We present the first discoveries of the double-lined double white dwarf (DBL) survey that targets over-luminous sources with respect to the canonical white dwarf cooling sequence a…

astro-ph.SR2024

A Test of Spectroscopic Age Estimates of White Dwarfs using Wide WD+WD Binaries

Tyler M. Heintz, J. J. Hermes, P. -E. Tremblay +4

White dwarf stars have been used for decades as precise and accurate age indicators. This work presents a test of the reliability of white dwarf total ages when spectroscopic obser…

astro-ph.SR2024

The Gaia white dwarf revolution

Pier-Emmanuel Tremblay, Antoine Bédard, Mairi W. O'Brien +4

This review highlights the role of the Gaia space mission in transforming white dwarf research. These stellar remnants constitute 5-7% of the local stellar population in volume, ye…

astro-ph.SR2024★ 88 cited

The 40 pc sample of white dwarfs from Gaia

Mairi W. O'Brien, P. -E. Tremblay, B. L. Klein +14

We present a comprehensive overview of a volume-complete sample of white dwarfs located within 40 pc of the Sun, a significant proportion of which were detected in Gaia Data Releas…

astro-ph.SR2023

Main sequence companions to white dwarfs II: the age-activity-rotation relation from a sample of Gaia common proper motion pairs

A. Rebassa-Mansergas, J. Maldonado, R. Raddi +8

Magnetic activity and rotation are related to the age of low-mass main sequence stars. To further constrain these relations, we study a sample of 574 main sequence stars members of…

astro-ph.SR2018★ 22 cited

Discovery of the first resolved triple white dwarf

M. Perpinyà-Vallès, A. Rebassa-Mansergas, B. T. Gänsicke +4

We report the discovery of J1953-1019, the first resolved triple white dwarf system. The triplet consists of an inner white dwarf binary and a wider companion. Using Gaia DR2 photo…

astro-ph.SR2016★ 28 cited

Outbursts in two new cool pulsating DA white dwarfs

Keaton J. Bell, J. J. Hermes, M. H. Montgomery +9

The unprecedented extent of coverage provided by Kepler observations recently revealed outbursts in two hydrogen-atmosphere pulsating white dwarfs (DAVs) that cause hours-long incr…