The authors deliver a combined SBCR for stars below ~16 solar masses spanning V-Ks from -0.9 to 2.1 mag with 0.025 mag scatter, plus a separate O-star relation, and verify it on an M33 eclipsing binary.
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5 Pith papers cite this work, alongside 270 external citations. Polarity classification is still indexing.
5
Pith papers citing it
270
external citations · OpenAlex
years
2026 5verdicts
UNVERDICTED 5representative citing papers
Asteroseismic modeling of RY Leporis gives a mass of ~2 solar masses and age of ~730 Myr, locating it in the post-main-sequence hydrogen shell-burning stage with consistent metallicity.
Three anomalous microlensing events are re-modeled as binary-lens binary-source (2L2S) systems that resolve prior residuals, with source stars identified as G8V/M3V, G8V/K2V, and G6V/G8V pairs and lenses inferred as low-mass binaries via Bayesian methods.
A new HST wide-field survey of the Galactic Bulge supplies high-angular-resolution data to enhance Roman exoplanet detections and serve as a community legacy dataset for stellar populations and dynamics.
Analyses of ten microlensing events identify candidate brown dwarf companions in binary systems, with two events suggesting brown dwarf binaries.
citing papers explorer
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Toward Early-type Eclipsing Binaries as Extragalactic Milestones: First Calibration of the SBCR from O- and B-type Stars in Detached Eclipsing Binaries
The authors deliver a combined SBCR for stars below ~16 solar masses spanning V-Ks from -0.9 to 2.1 mag with 0.025 mag scatter, plus a separate O-star relation, and verify it on an M33 eclipsing binary.
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Asteroseismic analysis of RY Leporis: the post-main sequence HADS in a binary system
Asteroseismic modeling of RY Leporis gives a mass of ~2 solar masses and age of ~730 Myr, locating it in the post-main-sequence hydrogen shell-burning stage with consistent metallicity.
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Four-Body Gravitational Microlensing Events Involving Both a Binary Lens and a Binary Source
Three anomalous microlensing events are re-modeled as binary-lens binary-source (2L2S) systems that resolve prior residuals, with source stars identified as G8V/M3V, G8V/K2V, and G6V/G8V pairs and lenses inferred as low-mass binaries via Bayesian methods.
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An HST Wide Field Survey of the Galactic Bulge: Overview, Strategy, and First Results
A new HST wide-field survey of the Galactic Bulge supplies high-angular-resolution data to enhance Roman exoplanet detections and serve as a community legacy dataset for stellar populations and dynamics.
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Candidate Microlensing Brown Dwarfs in Binary Lens Systems from the 2023--2025 Observing Seasons
Analyses of ten microlensing events identify candidate brown dwarf companions in binary systems, with two events suggesting brown dwarf binaries.