activity
20192026
most citedOGLE-2018-BLG-0022: A Nearby M-dwarf Binary

11 citations · 11 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.CO2026

AMPM II. A Lunar-Mass Primordial Black Hole Microlensing Candidate in the Milky Way Halo

Renee Key, Edward N. Taylor, Ken C. Freeman +5

Primordial Black Holes (PBH) are hypothesised to form during inflation and have long been considered a candidate for compact dark matter. Gravitational microlensing is known as a p…

astro-ph.GA2026

AMPM I. A Targeted Search for Asteroid Mass Primordial Black Hole Microlenses

Renee Key, Edward N. Taylor, Ken C. Freeman +5

Gravitational microlensing is a powerful technique for constraining the abundance of dark matter in asteroid mass to supermassive primordial black holes at masses of $-11 \lesssim…

astro-ph.IM2026

Attaining Spectral Energy Distributions With Sub-Percent Uncertainties: All-Sky DA White Dwarf Spectrophotometric Standard Stars For Large Telescopes And Surveys

Abhijit Saha, Edward W. Olszewski, Benjamin M. Boyd +14

We present a synopsis of the project to establish thirty-two new faint () DA white dwarfs as spectrophotometric standards distributed over the whole sky. O…

astro-ph.GA2024

ROME/REA: Three-year, Tri-color Timeseries Photometry of the Galactic Bulge

R. A. Street, E. Bachelet, Y. Tsapras +11

The ROME/REA (Robotic Observations of Microlensing Events/Reactive Event Assessment) Survey was a Key Project at Las Cumbres Observatory (hereafter LCO) which continuously monitore…

astro-ph.EP2019★ 11 cited

OGLE-2018-BLG-0022: A Nearby M-dwarf Binary

R. A. Street, E. Bachelet, Y. Tsapras +28

We report observations of the binary microlensing event OGLE-2018-BLG-0022, provided by the ROME/REA Survey, which indicate that the lens is a low-mass binary star consisting of M3…