activity
20092024
most citedMass Measurements of Isolated Objects from Space-based Microlensing

54 citations · 126 across the 6 of their papers we have counts for

collaborators

8 papers

nucl-ex2024

Enhanced -factor for the NO reaction and its impact on the solar composition problem

X. Chen, J. Su, Y. P. Shen +44

The solar composition problem has puzzled astrophysicists for more than 20 years. Recent measurements of carbon-nitrogen-oxygen (CNO) neutrinos by the Borexino experiment show a $\…

astro-ph.SR2015★ 23 cited

Spitzer Microlensing Program as a Probe for Globular Cluster Planets. Analysis of OGLE-2015-BLG-0448

Radosław Poleski, Wei Zhu, Grant W. Christie +83

The microlensing event OGLE-2015-BLG-0448 was observed by Spitzer and lay within the tidal radius of the globular cluster NGC 6558. The event had moderate magnification and was int…

astro-ph.SR2015★ 54 cited

Mass Measurements of Isolated Objects from Space-based Microlensing

Wei Zhu, S. Calchi Novati, A. Gould +78

We report on the mass and distance measurements of two single-lens events from the 2015 \emph{Spitzer} microlensing campaign. With both finite-source effect and microlens parallax…

nucl-ex2014★ 11 cited

Proton widths of the low-lying 16F states from the 15N(7Li, 6Li)16N reaction

Z. D. Wu, B. Guo, Z. H. Li +24

All the 16F levels are unbound by proton emission. To date the four low-lying 16F levels below 1 MeV have been experimentally identified with well established spin-parity values an…

nucl-ex2013★ 22 cited

Spectroscopic factors for low-lying 16N levels and the astrophysical 15N(n,gamma)16N reaction rate

B. Guo, Z. H. Li, Y. J. Li +23

Fluorine is a key element for nucleosynthetic studies since it is extremely sensitive to the physical conditions within stars. The astrophysical site to produce fluorine is suggest…

astro-ph.SR2013★ 16 cited

Constraining nova observables: direct measurements of resonance strengths in 33S(p,γ)34Cl

J. Fallis, A. Parikh, P. F. Bertone +32

The 33S(p,γ)34Cl reaction is important for constraining predictions of certain isotopic abundances in oxygen-neon novae. Models currently predict as much as 150 times the solar abu…