activity
20152026
most citedA million binaries from Gaia eDR3: sample selection and validation of Gaia parallax uncertainties

454 citations · 7.2k across the 161 of their papers we have counts for

collaborators
Showing 2025Show all

18 papers · 1 filter

astro-ph.SR2025

The physical properties of post-mass-transfer binaries

Rhys Seeburger, Hans-Walter Rix, Kareem El-Badry +4

Aims. We present and analyse the detailed physical properties of six binary stellar systems, originally proposed as possible star-black hole binaries on the basis of radial velocit…

astro-ph.SR2025★ 7 cited

Dormant black hole candidates from Gaia DR3 summary diagnostics

Johanna Müller-Horn, Hans-Walter Rix, Kareem El-Badry +4

We present a rigorous identification of candidates for dormant black holes (BHs) and neutron stars (NSs) in binaries using summary statistics from Gaia DR3, rather than full orbita…

astro-ph.GA2025

Active galactic nuclei do not exhibit strictly sinusoidal brightness variations

Kareem El-Badry, David W. Hogg, Hans-Walter Rix

Periodic variability in active galactic nuclei (AGN) light curves has been proposed as a signature of close supermassive black hole (SMBH) binaries. Recently, 181 candidate SMBH bi…

astro-ph.SR2025★ 4 cited

Complex spectral variability and hints of a luminous companion in the Be star + black hole binary candidate ALS 8814

Kareem El-Badry, Matthias Fabry, Hugues Sana +2

The emission-line binary ALS 8814 was recently proposed as a Be star + black hole (BH) binary based on large-amplitude radial velocity (RV) variations of a Be star and non-detectio…

astro-ph.SR2025★ 1 cited

A Spectroscopic Search for Dormant Black Holes in Low-Metallicity Binaries

Pranav Nagarajan, Kareem El-Badry, Henrique Reggiani +9

The discovery of the massive black hole (BH) system Gaia BH3 in pre-release Gaia DR4 data suggests that wide BH binaries with luminous companions may be significantly overrepresent…

astro-ph.SR2025

Double White Dwarf Binaries in SDSS-V DR19 : The discovery of a rare DA+DQ white dwarf binary with 31 hour orbital period

Gautham Adamane Pallathadka, Vedant Chandra, Boris T. Gansicke +13

Binaries of two white dwarfs (WDs) are an important class of astrophysical objects that are theorized to lead to Type Ia supernovae and are also used to gain insight into complex p…

astro-ph.SR2025★ 3 cited

Millions of Main-Sequence Binary Stars from Gaia BP/RP Spectra

Jiadong Li, Hans-Walter Rix, Yuan-Sen Ting +6

We present the main-sequence binary (MSMS) Catalog derived from Gaia Data Release 3 BP/RP (XP) spectra. Leveraging the vast sample of low-resolution Gaia XP spectra, we develop a f…

astro-ph.GA2025★ 8 cited

The Nineteenth Data Release of the Sloan Digital Sky Survey

SDSS Collaboration, Gautham Adamane Pallathadka, Mojgan Aghakhanloo +210

Mapping the local and distant Universe is key to our understanding of it. For decades, the Sloan Digital Sky Survey (SDSS) has made a concerted effort to map millions of celestial…

astro-ph.SR2025★ 12 cited

How to use Gaia parallaxes for stars with poor astrometric fits

Kareem El-Badry

Gaia parallax measurements for stars with poor astrometric fits -- as evidenced by high renormalized unit weight error (RUWE) -- are often assumed to be unreliable, but the extent…

astro-ph.SR2025★ 11 cited

Population demographics of white dwarf binaries with intermediate separations: Gaia constraints on post-AGB mass transfer

Natsuko Yamaguchi, Kareem El-Badry, Sahar Shahaf

Astrometry from the Gaia mission has revealed a large population of white dwarf (WD) + main sequence (MS) binaries with periods of d. These systems have separations i…

astro-ph.SR2025★ 6 cited

HIP 15429: A newborn Be star on an eccentric binary orbit

Johanna Müller-Horn, Kareem El-Badry, Hans-Walter Rix +9

We identified a new post-interaction binary, HIP 15429, consisting of a stripped star and a recently formed, rapidly rotating Be star companion ( km/s) sharin…

astro-ph.GA2025

Realistic predictions for Gaia black hole discoveries: comparison of isolated binary and dynamical formation models

Pranav Nagarajan, Kareem El-Badry, Chirag Chawla +6

Astrometry from Gaia has enabled discovery of three dormant black holes (BHs) in au-scale binaries. Numerous models have been proposed to explain their formation, including several…

astro-ph.SR2025★ 5 cited

Resolution of a paradox: SDSS J1257+5428 can be explained as a descendant of a cataclysmic variable with an evolved donor

Diogo Belloni, Matthias R. Schreiber, Kareem El-Badry

The existence of the binary system SDSS J1257+5428 has been described as paradoxical. Here we investigate under which conditions SDSS J1257+5428 could be understood as a descendant…

astro-ph.SR2025

Discovery of two new polars evolved past the period bounce

Tim Cunningham, Ilaria Caiazzo, Gracjan Sienkiewicz +13

We report the discovery of two new magnetic cataclysmic variables with brown dwarf companions and long orbital periods ( and min). This discovery incr…

astro-ph.SR2025★ 3 cited

Unevolved Li-rich stars at low metallicity: a possible formation pathway through novae

Tadafumi Matsuno, Alex Kemp, Ataru Tanikawa +7

A small fraction of low-mass stars have been found to have anomalously high Li abundances. Although it has been suggested that mixing during the red giant branch phase can lead to…

astro-ph.SR2025

Variability of Central Stars of Planetary Nebulae with the Zwicky Transient Facility. II. Long-Timescale Variables including Wide Binary and Late Thermal Pulse Candidates

Soumyadeep Bhattacharjee, Nicole Reindl, Howard E. Bond +14

In this second paper on our variability survey of central stars of planetary nebulae (CSPNe) using ZTF, we report 11 long-timescale variables with variability timescales ranging fr…

astro-ph.SR2025★ 5 cited

A ZTF Search for Circumstellar Debris Transits in White Dwarfs: Six New Candidates, one with Gas Disk Emission, identified in a Novel Metric Space

Soumyadeep Bhattacharjee, Zachary P. Vanderbosch, Mark A. Hollands +13

White dwarfs (WDs) showing transits from orbiting planetary debris provide significant insights into the structure and dynamics of debris disks. This is a rare class of objects wit…

astro-ph.SR2025

A Link Between White Dwarf Pulsars and Polars: Multiwavelength Observations of the 9.36-Minute Period Variable Gaia22ayj

Antonio C. Rodriguez, Kareem El-Badry, Pasi Hakala +30

White dwarfs (WDs) are the most abundant compact objects, and recent surveys have suggested that over a third of WDs in accreting binaries host a strong (B 1 MG) magnetic…