Area of research
Nuclear and High Energy Physics · Astronomy and Astrophysics
Research interest
Research interests include Astrophysics and Cosmic Phenomena, Dark Matter and Cosmic Phenomena, Gamma-ray bursts and supernovae, and Particle Detector Development and Performance.
Isovalent metal doping tuning electronic structure to boost molecular oxygen adsorption and lattice oxygen activation for efficient o-xylene oxidation
Galactic Gamma-Ray Diffuse Emission at TeV Energies with HAWC Data
Discovery of Gamma Rays from the Quiescent Sun with HAWC
HAWC Detection of a TeV Halo Candidate Surrounding a Radio-quiet Pulsar
An optimized search for dark matter in the galactic halo with HAWC
Cosmic ray spectrum of protons plus helium nuclei between 6 and 158 TeV from HAWC data
Long-term Spectra of the Blazars Mrk 421 and Mrk 501 at TeV Energies Seen by HAWC
Gamma/hadron separation with the HAWC observatory
Evidence of 200 TeV Photons from HAWC J1825-134
Spectrum and Morphology of the Very-high-energy Source HAWC J2019+368
HAWC Study of the Ultra-High-Energy Spectrum of MGRO J1908+06
Multimessenger Gamma-Ray and Neutrino Coincidence Alerts Using HAWC and IceCube Subthreshold Data
Constraints on Lorentz Invariance Violation from HAWC Observations of Gamma Rays above 100 TeV
HAWC J2227+610 and its association with G106.3+2.7, a new potential Galactic PeVatron
MPG.PuRe (Max Planck Society) 2020cited by 64position: middle
Constraining the local burst rate density of primordial black holes with HAWC
Search for gamma-ray spectral lines from dark matter annihilation in dwarf galaxies with the High-Altitude Water Cherenkov observatory
Dark Matter Limits from Dwarf Spheroidal Galaxies with the HAWC Gamma-Ray Observatory
All-Sky Measurement of the Anisotropy of Cosmic Rays at 10 TeV and Mapping of the Local Interstellar Magnetic Field
Constraints on spin-dependent dark matter scattering with long-lived mediators from TeV observations of the Sun with HAWC
First HAWC observations of the Sun constrain steady TeV gamma-ray emission
All-particle cosmic ray energy spectrum measured by the HAWC experiment from 10 to 500 TeV
SEARCH FOR TeV GAMMA-RAY EMISSION FROM POINT-LIKE SOURCES IN THE INNER GALACTIC PLANE WITH A PARTIAL CONFIGURATION OF THE HAWC OBSERVATORY