Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Physics, Astrophysics, Galaxy, Astronomy, Star formation, and Globular cluster.
<i>Euclid</i> : Early Release Observations – Interplay between dwarf galaxies and their globular clusters in the Perseus galaxy cluster
<i>Euclid</i> preparation
<i>Euclid</i> preparation
<i>Euclid</i>: Early Release Observations – Globular clusters in the Fornax galaxy cluster, from dwarf galaxies to the intracluster field
<i>Euclid</i> preparation
<i>Euclid</i>preparation – XXIII. Derivation of galaxy physical properties with deep machine learning using mock fluxes and<i>H</i>-band images
Excitation of Polycyclic Aromatic Hydrocarbon Emission: Dependence on Size Distribution, Ionization, and Starlight Spectrum and Intensity
Compact binary mergers: R-process kilonovae and ultra-relativistic jets
UWA Profiles and Research Repository (University of Western Australia) 2020cited by 0position: middle
Identification of strontium in the merger of two neutron stars
Comprehensive comparison of models for spectral energy distributions from 0.1<i>μ</i>m to 1 mm of nearby star-forming galaxies
Spectroscopic identification of r-process nucleosynthesis in a double neutron-star merger
The Radio Spectral Energy Distribution and Star-formation Rate Calibration in Galaxies
Updated 34-band Photometry for the SINGS/KINGFISH Samples of Nearby Galaxies
THE SPATIALLY RESOLVED COOLING LINE DEFICIT IN GALAXIES
Massive stars formed in atomic hydrogen reservoirs: H I observations of gamma-ray burst host galaxies
Molecular line emission in NGC 1068 imaged with ALMA
Cool dust heating and temperature mixing in nearby star-forming galaxies
Dissecting the origin of the submillimetre emission in nearby galaxies with Herschel and LABOCA
A quiescent galaxy at the position of the long GRB 050219A
A FAR-IR VIEW OF THE STARBURST-DRIVEN SUPERWIND IN NGC 2146
THE CO-TO-H<sub>2</sub>CONVERSION FACTOR AND DUST-TO-GAS RATIO ON KILOPARSEC SCALES IN NEARBY GALAXIES
Calibration of the total infrared luminosity of nearby galaxies from Spitzer and Herschel bands
TOWARD A REMOVAL OF TEMPERATURE DEPENDENCIES FROM ABUNDANCE DETERMINATIONS: NGC 628
<i>HERSCHEL</i>FAR-INFRARED AND SUBMILLIMETER PHOTOMETRY FOR THE KINGFISH SAMPLE OF NEARBY GALAXIES