Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Physics, Astrophysics, Galaxy, Redshift, Stellar mass, and Star formation.
<i>Euclid</i> preparation
A Census of Star Formation Histories of Massive Galaxies at 0.6 < z < 1 from Spectrophotometric Modeling Using Bagpipes and Prospector
JWST MIRI and NIRCam observations of NGC 891 and its circumgalactic medium
Bulge+disc decomposition of HFF and CANDELS galaxies: UVJ diagrams and stellar mass–size relations of galaxy components at 0.2 ≤ <i>z</i> ≤ 1.5
The Gas and Stellar Content of a Metal-poor Galaxy at <i>z</i> = 8.496 as Revealed by JWST and ALMA
Stellar Half-mass Radii of 0.5 z < 2.3 Galaxies: Comparison with JWST/NIRCam Half-light Radii
PHANGS–JWST First Results: Interstellar Medium Structure on the Turbulent Jeans Scale in Four Disk Galaxies Observed by JWST and the Atacama Large Millimeter/submillimeter Array
Galaxy And Mass Assembly (GAMA): Data Release 4 and the <i>z</i> &lt; 0.1 total and <i>z</i> &lt; 0.08 morphological galaxy stellar mass functions
The Mass Scale of High-redshift Galaxies: Virial Mass Estimates Calibrated with Stellar Dynamical Models from LEGA-C
Diagnosing DASH: A Catalog of Structural Properties for the COSMOS-DASH Survey
The LEGA-C of Nature and Nurture in Stellar Populations at z ∼ 0.6–1.0: D<sub> n </sub>4000 and Hδ Reveal Different Assembly Histories for Quiescent Galaxies in Different Environments
The Velocity Dispersion Function for Massive Quiescent and Star-forming Galaxies at 0.6 < z ≤ 1.0
3D-DASH: The Widest Near-infrared Hubble Space Telescope Survey
Resolved stellar mass maps of galaxies in the Hubble Frontier Fields : evidence for mass dependency in environmental quenching
LEGA-C: Analysis of Dynamical Masses from Ionized Gas and Stellar Kinematics at z ∼ 0.8
The LEGA-C and SAMI galaxy surveys: quiescent stellar populations and the mass–size plane across 6 Gyr
Resolved Stellar Mass Maps of Galaxies in the Hubble Frontier Fields: Evidence for Mass Dependency in Environmental Quenching
The Large Early Galaxy Astrophysics Census (LEGA-C) Data Release 3: 3000 High-quality Spectra of K <sub> s </sub>-selected Galaxies at z > 0.6
Extending the evolution of the stellar mass–size relation at <i>z</i> ≤ 2 to low stellar mass galaxies from HFF and CANDELS
The Fundamental Plane in the LEGA-C Survey: Unraveling the M/L Ratio Variations of Massive Star-forming and Quiescent Galaxies at z ∼ 0.8
The LEGA-C and SAMI Galaxy Surveys: Quiescent Stellar Populations and the Mass-Size Plane across 6 Gyr
HST/WFC3 Grism Observations of z ∼ 1 Clusters: Evidence for Rapid Outside-in Environmental Quenching from Spatially Resolved Hα Maps
Stellar Dynamical Models for 797 z ∼ 0.8 Galaxies from LEGA-C
Ubiquitous [O ii] Emission in Quiescent Galaxies at z ≈ 0.85 from the LEGA-C Survey*
Toward Precise Galaxy Evolution: A Comparison between Spectral Indices of z ∼1 Galaxies in the IllustrisTNG Simulation and the LEGA-C Survey
The LEGA-C Survey Completed: Stellar Populations and Stellar Kinematics of Galaxies 7 Gyr Ago
Quenching as a Contest between Galaxy Halos and Their Central Black Holes
Inverse stellar population age gradients of post-starburst galaxies at z = 0.8 with LEGA-C
Tightly Coupled Morpho-kinematic Evolution for Massive Star-forming and Quiescent Galaxies across 7 Gyr of Cosmic Time
Dust Attenuation Curves at z ~ 0.8 from LEGA-C : Precise Constraints on the Slope and 2175Å Bump Strength
Lancaster EPrints (Lancaster University) 2020cited by 9position: middle