We present a catalogue of white dwarf candidates selected from Gaia Early Data Release 3
(EDR3). We applied several selection criteria in absolute magnitude, colour, and Gaia …

We present a catalogue of white dwarf candidates selected from the second data release of
Gaia (DR2). We used a sample of spectroscopically confirmed white dwarfs from the Sloan …

Introduction Neutron stars with masses above 1.8 solar masses (M☉), possess extreme
gravitational fields, which may give rise to phenomena outside general relativity. These …

During the last decade white dwarfs have become important as tools in many areas beyond
traditional stellar physics: from the age determination of the stars in the solar neighborhood …

White dwarfs are the final remnants of low-and intermediate-mass stars. Their evolution is
essentially a cooling process that lasts for∼ 10 Gyr. Their observed properties provide …

A large number of extremely low-mass helium white dwarfs (ELM WDs) have been
discovered in recent years. The majority of them are found in close binary systems …

We present a catalogue of 73 221 white dwarf candidates extracted from the astrometric and
photometric data of the recently published Gaia-DR2 catalogue. White dwarfs were selected …

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 …

We present the full spectroscopic white dwarf and hot subdwarf sample from the Sloan
Digital Sky Survey (SDSS) first data release, DR1. We find 2551 white dwarf stars of various …

PSR J1738+ 0333 is one of the four millisecond pulsars known to be orbited by a white
dwarf companion bright enough for optical spectroscopy. Of these, it has the shortest orbital …