activity
20112026
most citedThe Gaia DR1 Mass-Radius Relation for White Dwarfs

66 citations · 134 across the 16 of their papers we have counts for

collaborators

17 papers

astro-ph.SR2026

The white dwarf binary pathways survey - XI. The Gaia-GALEX UV Excess Sample for systems within 350 pc

James A. Garbutt, S. G. Parsons, N. Gentile Fusillo +9

White dwarfs (WDs) with F, G or K type binary companions are the last common ancestor to a zoo of exotic phenomena. Finding a clean sample of such systems is difficult, as WDs in s…

astro-ph.IM2025

White Dwarf Binaries: Probes of Future Astrophysics

Anna F. Pala, Roberto Raddi, Alberto Rebassa-Mansergas +25

White dwarf binaries are fundamental astrophysical probes. They represent ideal laboratories to test the models of binary evolution, which also apply to the sources of gravitationa…

astro-ph.IM2025

White Dwarfs in Wide Binary Systems as Reliable Age Calibrators

Alberto Rebassa-Mansergas, Roberto Raddi, Anna F. Pala +13

Deriving precise stellar ages is a challenging task. Consequently, age-dependent relations - such as the age-metallicity and age-velocity dispersion relations of the Milky Way, or…

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.IM2025

ESO Expanding Horizons White Paper: Electromagnetic characterisation of millihertz gravitational-wave sources in the Milky Way

James Munday, Valeriya Korol, Camilla Danielski +8

The millihertz band is densely populated by continuous gravitational-wave signals from Galactic compact binaries, dominated by double white dwarfs (DWDs; binaries of two white dwar…

astro-ph.SR2025

Constraints on an optical counterpart for the long-period radio transient GPM J1839-10

Ingrid Pelisoli, A. J. Brown, N. Castro Segura +14

Long period radio transients (LPTs) are periodic radio sources showing pulsed emission on timescales from minutes to hours. The underlying sources behind this emission are currentl…

astro-ph.SR2025★ 1 cited

A Sibling of AR Scorpii: SDSS J230641.47244055.8 and the Observational Blueprint of White Dwarf Pulsars

N. Castro Segura, I. Pelisoli, B. T. Gänsicke +21

Radio pulsating white dwarf (WD) systems, known as WD pulsars, are non-accreting binary systems where the rapidly spinning WD interacts with a low-mass companion producing pulsed n…

astro-ph.SR2025

Asteroseismology of WD J004917.14-252556.81, the Most Massive Pulsating White Dwarf

O. Caliskan, M. Uzundag, M. Kilic +10

We present extensive follow-up time-series photometry of WD J00492525, the most massive pulsating white dwarf currently known with and $\log{\i…

astro-ph.SR2025★ 6 cited

A magnitude-limited catalogue of unresolved white dwarf-main sequence binaries from Gaia DR3

Alberto Rebassa-Mansergas, Enrique Solano, Alex J. Brown +6

Binary stars containing a white dwarf and a main-sequence star, WDMS binaries, can be used to study a wide range of aspects of stellar astrophysics. We build a magnitude-limited sa…

astro-ph.SR2025

A targeted search for binary white dwarf pulsars using Gaia and WISE

Ingrid Pelisoli, T. R. Marsh, G. Tovmassian +24

After its discovery in 2016, the white dwarf binary AR Scorpii (AR Sco) remained for several years the only white dwarf system to show pulsed radio emission associated with a fast-…

astro-ph.SR2025★ 7 cited

Reconstructing post-common envelope white dwarf+main sequence binary histories through inverse population synthesis techniques

Santiago Torres, Marta Gili, Alberto Rebassa-Mansergas +3

The evolution of binary stellar systems involves a wide range of physical processes, many of which are not yet well understood. We aim to build a general-purpose algorithm based on…

astro-ph.SR2024

A gravitational wave detectable candidate Type Ia supernova progenitor

Emma T. Chickles, Kevin B. Burdge, Joheen Chakraborty +37

Type Ia supernovae, critical for studying cosmic expansion, arise from thermonuclear explosions of white dwarfs, but their precise progenitor pathways remain unclear. Growing evide…

astro-ph.SR2024★ 2 cited

The white dwarf binary pathways survey -- X. Gaia orbits for known UV excess binaries

J. A. Garbutt, S. G. Parsons, O. Toloza +9

White dwarfs with a F, G or K type companion represent the last common ancestor for a plethora of exotic systems throughout the galaxy, though to this point very few of them have b…

astro-ph.SR2024★ 1 cited

A Survey for Radio Emission from White Dwarfs in the VLA Sky Survey

Ingrid Pelisoli, Laura Chomiuk, Jay Strader +22

Radio emission has been detected from tens of white dwarfs, in particular in accreting systems. Additionally, radio emission has been predicted as a possible outcome of a planetary…

astro-ph.EP2024

TOI-2266 b: a keystone super-Earth at the edge of the M dwarf radius valley

Hannu Parviainen, Felipe Murgas, Emma Esparza-Borges +59

We validate the Transiting Exoplanet Survey Satellite (TESS) object of interest TOI-2266.01 (TIC 348911) as a small transiting planet (most likely a super-Earth) orbiting a faint M…

astro-ph.SR2016★ 66 cited

The Gaia DR1 Mass-Radius Relation for White Dwarfs

P. -E. Tremblay, N. Gentile-Fusillo, R. Raddi +8

The Gaia Data Release 1 (DR1) sample of white dwarf parallaxes is presented, including 6 directly observed degenerates and 46 white dwarfs in wide binaries. This data set is combin…

astro-ph.SR2011★ 51 cited

The shortest period detached white dwarf + main-sequence binary

S. G. Parsons, T. R. Marsh, B. T. Gänsicke +8

We present high-speed ULTRACAM and SOFI photometry and X-shooter spectroscopy of the recently discovered 94 minute orbital period eclipsing white dwarf / main-sequence binary SDSS…