activity
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

collaborators

82 papers

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.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.GA2025

Uniformly-calibrated VPHAS+ photometry in the third quadrant of the Galactic plane

J. E. Drew, R. Greimel, J. Eislöffel +2

The southern Galactic plane has been mapped at optical wavelengths and at under one-arcsecond angular resolution by the VST Photometric Ha Survey of the Galactic plane and bulge (V…

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.IM2024★ 12 cited

The Wide-field Spectroscopic Telescope (WST) Science White Paper

Vincenzo Mainieri, Richard I. Anderson, Jarle Brinchmann +214

The Wide-field Spectroscopic Telescope (WST) is proposed as a new facility dedicated to the efficient delivery of spectroscopic surveys. This white paper summarises the initial con…

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…