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20132026
most citedA Data Release 2 catalogue of white dwarfs and a comparison with SDSS

424 citations · 3.5k across the 82 of their papers we have counts for

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astro-ph.SR2026

Plato benchmark stars I. The initial benchmark sample

T. Merle, P. F. L. Maxted, O. L. Creevey +22

The ESA PLATO mission aims to detect and characterise Earth-size exoplanets orbiting bright, late-type stars using high-precision photometry and asteroseismology. Precise stellar p…

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.SR2026

WEAVE imaging spectroscopy of NGC 6720: an iron bar in the Ring

R. Wesson, J. E. Drew, M. J. Barlow +23

We present spatially resolved spectroscopic observations of the planetary nebula NGC 6720, the Ring Nebula, taken during the science verification phase of WEAVE, a new instrument m…

astro-ph.SR2025

Spectroscopic and kinematic analyses of a warm survivor of a D6 supernova

Mark A. Hollands, Ken. J. Shen, Roberto Raddi +3

SDSSJ163712.21+363155.9 is a candidate hyper-runaway star, first identified from its unusual spectrum in the Sloan Digital Sky Survey, which exhibits oxygen, magnesium, and silicon…

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★ 1 cited

Benchmark brown dwarfs -- I. A blue M2 + T5 wide binary and a probable young [M4 + M4] + [T7 + T8] hierarchical quadruple

Z. H. Zhang, F. Navarete, M. C. Galvez-Ortiz +13

Benchmark brown dwarfs in wide binary systems are crucial for characterizing substellar objects and calibrating atmospheric and evolutionary models. However, brown dwarf benchmarks…

astro-ph.SR2025★ 7 cited

Testing the mass-radius relation of white dwarfs in common proper motion pairs I.Hydrogen-dominated atmospheres

Roberto Raddi, Alberto Rebassa-Mansergas, Santiago Torres +6

The main goal of this work was to measure the masses and radii of white dwarfs that belong to widely separated, common proper motion binaries with non-degenerate companions. These…

astro-ph.SR2024★ 18 cited

Main sequence dynamo magnetic fields emerging in the white dwarf phase

Maria Camisassa, J. R. Fuentes, Matthias R. Schreiber +4

Recent observations of volume-limited samples of magnetic white dwarfs (WD) have revealed a higher incidence of magnetism in older WDs. Specifically, these studies indicate that ma…

astro-ph.SR2024★ 7 cited

Primeval very low-mass stars and brown dwarfs -- VIII. The first age benchmark L subdwarf, a wide companion to a halo white dwarf

Z. H. Zhang, R. Raddi, A. J. Burgasser +12

We report the discovery of five white dwarf + ultracool dwarf systems identified as common proper motion wide binaries in the Gaia Catalogue of Nearby Stars. The discoveries includ…

astro-ph.SR2024★ 11 cited

A spectroscopic and kinematic survey of fast hot subdwarfs

S. Geier, U. Heber, A. Irrgang +19

Hot subdwarfs (sdO/B) are the stripped helium cores of red giants formed by binary interactions. Close hot subdwarf binaries with massive white dwarf companions have been proposed…

astro-ph.SR2024★ 4 cited

Kinematic origin of white dwarfs in the solar neighborhood

Ainhoa Zubiaur, Roberto Raddi, Santiago Torres

Thanks to the recent space-borne mission Gaia, there is a nearly complete sample of white dwarfs up to about 100 parsecs from the Sun, which may have very diverse origins. We aim t…

astro-ph.SR2024

A 500 pc volume-limited sample of hot subluminous stars I. Space density, scale height, and population properties

H. Dawson, S. Geier, U. Heber +25

We present the first volume-limited sample of spectroscopically confirmed hot subluminous stars out to 500 pc, defined using the accurate parallax measurements from the {\em Gaia}…

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★ 5 cited

J0526+5934: a peculiar ultra-short period double white dwarf

Alberto Rebassa-Mansergas, Mark Hollands, Steven G. Parsons +6

Ultra-short period compact binaries are important sources of gravitational waves, which include e.g. the progenitors of type Ia supernovae or the progenitors of merger episodes tha…

astro-ph.SR2023★ 2 cited

The Initial Mass Function Based on the Full-sky 20-pc Census of 3,600 Stars and Brown Dwarfs

J. Davy Kirkpatrick, Federico Marocco, Christopher R. Gelino +85

A complete accounting of nearby objects -- from the highest-mass white dwarf progenitors down to low-mass brown dwarfs -- is now possible, thanks to an almost complete set of trigo…

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.SR2023★ 9 cited

The unusual planetary nebula nucleus in the Galactic open cluster M37 and six further hot white dwarf candidates

Klaus Werner, Nicole Reindl, Roberto Raddi +6

Planetary nebulae in Galactic open star clusters are rare objects; only three are known to date. They are of particular interest because their distance can be determined with high…

astro-ph.SR2023★ 24 cited

White dwarf spectral type-temperature distribution from Gaia-DR3 and the Virtual Observatory

S. Torres, P. Cruz, R. Murillo-Ojeda +6

The characterization of white dwarf atmospheres is crucial for accurately deriving stellar parameters such as effective temperature, mass, and age. We aim to classify the populatio…

astro-ph.SR2023★ 16 cited

Carbon-oxygen ultra-massive white dwarfs in general relativity

Leandro G. Althaus, Alejandro H. Córsico, María E. Camisassa +4

We employ the La Plata stellar evolution code, LPCODE, to compute the first set of constant rest-mass carbon-oxygen ultra-massive white dwarf evolutionary sequences for masses high…

astro-ph.SR2023★ 26 cited

A hidden population of white dwarfs with atmospheric carbon traces in the Gaia bifurcation

Maria Camisassa, Santiago Torres, Mark Hollands +4

The ESA Gaia space mission has revealed a bifurcation of the white dwarf (WD) sequence on the color magnitude diagram in two branches: A and B. While the A branch consists mostly o…

astro-ph.SR2022★ 20 cited

The White Dwarf Binary Pathways Survey -- IX. Three long period white dwarf plus subgiant binaries

S. G. Parsons, M. S. Hernandez, O. Toloza +8

Virtually all binaries consisting of a white dwarf with a non-degenerate companion can be classified as either close post-interaction systems (with orbital periods of a few days or…

astro-ph.SR2022★ 54 cited

white dwarfs within 40 pc III: spectroscopic observations of new candidates in the southern hemisphere

Mairi W. O'Brien, P. -E. Tremblay, N. P. Gentile Fusillo +31

We present a spectroscopic survey of 248 white dwarf candidates within 40 pc of the Sun; of these 244 are in the southern hemisphere. Observations were performed mostly with the Ve…

astro-ph.SR2022★ 32 cited

The White Dwarf Binary Pathways Survey -- VIII: a post common envelope binary with a massive white dwarf and an active G-type secondary star

M. S. Hernandez, M. R. Schreiber, S. G. Parsons +6

The white dwarf binary pathways survey is dedicated to studying the origin and evolution of binaries containing a white dwarf and an intermediate-mass secondary star of the spectra…

astro-ph.SR2022★ 8 cited

Perfecting our set of spectrophotometric standard DA white dwarfs

A. Calamida, T. Matheson, E. W. Olszewski +17

We verified for photometric stability a set of DA white dwarfs with Hubble Space Telescope magnitudes from the near-ultraviolet to the near-infrared and ground-based spectroscopy b…