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20242026
most citedOverview of the JWST Advanced Deep Extragalactic Survey (JADES)

106 citations · 137 across the 18 of their papers we have counts for

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21 papers · 1 filter

astro-ph.SR2026

Spectroscopic follow-up of compact object binary candidates from Gaia DR3: White dwarfs, neutron stars, black holes, and the parallax zeropoint

Kareem El-Badry, David W. Latham, Hans-Walter Rix +12

Astrometry and radial velocities (RVs) from Gaia DR3 yielded orbits for hundreds of thousands of binary systems, including several samples proposed to contain black holes (BHs), ne…

astro-ph.SR2026

A Galactic intermediate-mass stripped star with a Wolf-Rayet-like wind

Johanna Müller-Horn, Kareem El-Badry, Andreas A. C. Sander +17

Binary interaction in massive stars is expected to produce a large population of intermediate-mass (- M) envelope-stripped stars, yet such objects have remained elusi…

astro-ph.SR20266 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.SR20261 cited

IK Pegasi and the Double-merger Path to Type Ia Supernovae

Na'ama Hallakoun, Sahar Shahaf, Sagi Ben-Ami +3

Recent Gaia astrometry has revealed thousands of main-sequence + white-dwarf binaries (MS+WD) at separations of ~0.1-10 au, including a subset hosting unusually massive (>~0.8 Msun…

astro-ph.SR2026

Evaluating Classifications of Extremely Metal-poor Candidates Selected from Gaia XP Spectra

Riley Thai, Andrew R. Casey, Alexander Ji +2

Extremely metal-poor stars are intrinsically rare, but emerging methods exist to accurately classify them from all-sky Gaia XP low-resolution spectra. To assess their overall accur…

astro-ph.SR20265 cited

Gaia Barium Dwarfs and Their Ostensibly Ordinary Counterparts

Param Rekhi, Sahar Shahaf, Sagi Ben-Ami +4

The recently identified Gaia population of main-sequence--white dwarf (MS+WD) binaries at separations of , often with moderate eccentricities, is not readily re…