Area of research
Instrumentation · Astronomy and Astrophysics
Research interest
Research interests include Physics, Astrophysics, Galaxy, Redshift, Astronomy, and Weak gravitational lensing.
Bound star clusters observed in a lensed galaxy 460 Myr after the Big Bang
Strong gravitational lensing’s ‘external shear’ is not shear
SPT clusters with DES and HST weak lensing. I. Cluster lensing and Bayesian population modeling of multiwavelength cluster datasets
SPT-SZ MCMF: an extension of the SPT-SZ catalogue over the DES region
TEMPLATES: Direct Abundance Constraints for Two Lensed Lyman-break Galaxies
The Extended [C ii] under Construction? Observation of the Brightest High-z Lensed Star-forming Galaxy at z = 6.2
COSMOS-Web: An Overview of the JWST Cosmic Origins Survey
JWST/NIRCam Probes Young Star Clusters in the Reionization EraSunrise Arc
Star formation at the smallest scales: a JWST study of the clump populations in SMACS0723
High-redshift Galaxy Candidates at z = 9–10 as Revealed by JWST Observations of WHL0137-08
Two Lensed Star Candidates at z ≃ 4.8 behind the Galaxy Cluster MACS J0647.7+7015
JWST Reveals a Possible z ∼ 11 GalaxyMerger in Triply Lensed MACS0647–JD
Precision Modeling of JWST's First Cluster Lens SMACS J0723.3–7327*
Discovering gravitationally lensed gravitational waves: predicted rates, candidate selection, and localization with the Vera Rubin Observatory
Small Region, Big Impact: Highly Anisotropic Lyman-continuum Escape from a Compact Starburst Region with Extreme Physical Properties
Exploring the correlation between dark matter, intracluster light, and globular cluster distribution in SMACS0723
JWST's TEMPLATES for Star Formation: The First Resolved Gas-phase Metallicity Maps of Dust-obscured Star-forming Galaxies at z ∼ 4
REQUIEM-2D: A Diversity of Formation Pathways in a Sample of Spatially Resolved Massive Quiescent Galaxies at z ∼ 2
The impact of human expert visual inspection on the discovery of strong gravitational lenses
A new step forward in realistic cluster lens mass modelling: analysis of Hubble Frontier Field Cluster Abell S1063 from joint lensing, X-ray, and galaxy kinematics data
Hubble Constant Measurement from Three Large-separation Quasars Strongly Lensed by Galaxy Clusters
COOL–LAMPS. III. Discovery of a 25.″9 Separation Quasar Lensed by a Merging Galaxy Cluster*
COOL-LAMPS. Discovery of COOL J0335−1927, a Gravitationally Lensed Quasar at z = 3.27 with an Image Separation of 23.″3
Revealing galaxy candidates out to <i>z</i> ∼ 16 with JWST observations of the lensing cluster SMACS0723
A highly magnified star at redshift 6.2
JWST Imaging of Earendel, the Extremely Magnified Star at Redshift z = 6.2
The Cosmic Telescope That Lenses the Sunburst Arc, PSZ1 G311.65–18.48: Strong Gravitational Lensing Model and Source Plane Analysis*
Pilot-WINGS: An extended MUSE view of the structure of Abell 370
Recovery and analysis of rest-frame UV emission lines in 2052 galaxies observed with MUSE at 1.5 <<i>z</i>< 6.4
Recent Star Formation in a Massive Slowly Quenched Lensed Quiescent Galaxy at z = 1.88