Area of research
Instrumentation · Astronomy and Astrophysics
Research interest
Research interests include Physics, Astrophysics, Galaxy, Redshift, Astronomy, and Star formation.
UVCANDELS: The Role of Dust on the Stellar Mass–Size Relation of Disk Galaxies at 0.5 ≤ z ≤ 3.0
CEERS Key Paper. III. The Diversity of Galaxy Structure and Morphology at z = 3–9 with JWST
A Census of the Bright z = 8.5–11 Universe with the Hubble and Spitzer Space Telescopes in the CANDELS Fields
Morphological signatures of mergers in the TNG50 simulation and the Kilo-Degree Survey: the merger fraction from dwarfs to Milky Way-like galaxies
DeepAdversaries: examining the robustness of deep learning models for galaxy morphology classification
3D-DASH: The Widest Near-infrared Hubble Space Telescope Survey
DeepMerge – II. Building robust deep learning algorithms for merging galaxy identification across domains
DeepMerge: Classifying high-redshift merging galaxies with deep neural networks
Stellar masses of giant clumps in CANDELS and simulated galaxies using machine learning
The nature of giant clumps in high- <i>z</i> discs: a deep-learning comparison of simulations and observations
Automated distant galaxy merger classifications from Space Telescope images using the Illustris simulation
The optical morphologies of galaxies in the IllustrisTNG simulation: a comparison to Pan-STARRS observations
The role of mergers and halo spin in shaping galaxy morphology
z ∼ 2: An Epoch of Disk Assembly
Massive close pairs measure rapid galaxy assembly in mergers at high redshift
STAR FORMATION AND AGN ACTIVITY IN GALAXY CLUSTERS FROM z = 1–2: A MULTI-WAVELENGTH ANALYSIS FEATURING HERSCHEL/PACS
The Illustris simulation: the evolving population of black holes across cosmic time
The illustris simulation: Public data release
The formation of massive, compact galaxies at z = 2 in the Illustris simulation
Galaxy morphology and star formation in the Illustris Simulation at<i>z</i> = 0
Synthetic galaxy images and spectra from the Illustris simulation
Recoiling black holes: prospects for detection and implications of spin alignment
Diverse structural evolution at<i>z</i> > 1 in cosmologically simulated galaxies
Properties of galaxies reproduced by a hydrodynamic simulation
THE ERA OF STAR FORMATION IN GALAXY CLUSTERS
The evolution of dust-obscured star formation activity in galaxy clusters relative to the field over the last 9 billion years★
IDCS J1426.5+3508: SUNYAEV-ZEL’DOVICH MEASUREMENT OF A MASSIVE INFRARED-SELECTED CLUSTER AT<i>z</i>= 1.75