Identifies 596 WD-MS binary candidates within 100 pc (497 new) by detecting NUV excess in Gaia sources and fitting SEDs to estimate WD temperatures and masses.
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4 Pith papers cite this work. Polarity classification is still indexing.
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VLBA observations of Orion young stellar binaries yield Keplerian orbits and dynamical masses for four systems, with two showing agreement to SED-based estimates and one confirming an intermediate-mass star with nonthermal emission.
The paper presents quantitative metrics and thresholds for selecting the Prime Sample of 15,000 stars in the PLATO LOPS2 field to enable ground-based follow-up of exoplanet candidates.
New optical identifications and precise astrometry are reported for four quiescent black hole X-ray transients, with 3-sigma magnitude limits for five additional candidates.
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A search for optical counterparts in quiescent black hole X-ray transients
New optical identifications and precise astrometry are reported for four quiescent black hole X-ray transients, with 3-sigma magnitude limits for five additional candidates.