Area of research
Astronomy and Astrophysics · Oceanography
Research interest
Research interests include Physics, Astrophysics, Neutron star, Kilonova, Gravitational wave, and Ejecta.
Heavy-element production in a compact object merger observed by JWST
The First JWST Spectrum of a GRB Afterglow: No Bright Supernova in Observations of the Brightest GRB of all Time, GRB 221009A
JWST detection of heavy neutron capture elements in a compact object merger
The Challenges Ahead for Multimessenger Analyses of Gravitational Waves and Kilonova: A Case Study on GW190425
GROWTH on S190814bv: Deep Synoptic Limits on the Optical/Near-infrared Counterpart to a Neutron Star–Black Hole Merger
The Panchromatic Afterglow of GW170817: The full uniform dataset, modeling, comparison with previous results and implications
Distinguishing the nature of comparable-mass neutron star binary systems with multimessenger observations: GW170817 case study
Superluminal motion of a relativistic jet in the neutron-star merger GW170817
A cocoon shock breakout as the origin of the γ-ray emission in GW170817
A radio counterpart to a neutron star merger
A mildly relativistic wide-angle outflow in the neutron-star merger event GW170817
Analytic heating rate of neutron star merger ejecta derived from Fermi's theory of beta decay
Effects of Neutron-Star Dynamic Tides on Gravitational Waveforms within the Effective-One-Body Approach
The Macronova in GRB 050709 and the GRB-macronova connection
Measurability of the tidal deformability by gravitational waves from coalescing binary neutron stars
Radioactive decay products in neutron star merger ejecta: heating efficiency and γ-ray emission
NATAL KICKS AND TIME DELAYS IN MERGING NEUTRON STAR BINARIES: IMPLICATIONS FOR r-PROCESS NUCLEOSYNTHESIS IN ULTRA-FAINT DWARFS AND IN THE MILKY WAY
r-PROCESS PRODUCTION SITES AS INFERRED FROM Eu ABUNDANCES IN DWARF GALAXIES
ARE ULTRA-LONG GAMMA-RAY BURSTS CAUSED BY BLUE SUPERGIANT COLLAPSARS, NEWBORN MAGNETARS, OR WHITE DWARF TIDAL DISRUPTION EVENTS?
Institutional Repositories DataBase (IRDB) 2016cited by 30position: middle
A possible macronova in the late afterglow of the long–short burst GRB 060614
Mass ejection from neutron star mergers: different components and expected radio signals
Short-lived 244Pu points to compact binary mergers as sites for heavy r-process nucleosynthesis
Exploring tidal effects of coalescing binary neutron stars in numerical relativity. II. Long-term simulations