Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Physics, Astrophysics, Galaxy, Redshift, Astronomy, and Dark matter.
<i>Euclid</i> : Early Release Observations – Weak gravitational lensing analysis of Abell 2390
<i>Euclid</i>: Early Release Observations – Programme overview and pipeline for compact- and diffuse-emission photometry
COSMOS2025: The COSMOS-Web galaxy catalog of photometry, morphology, redshifts, and physical parameters from JWST, HST, and ground-based imaging
Euclid preparation. LXXIV. Euclidised observations of Hubble Frontier Fields and CLASH galaxy clusters
Bright extragalactic ALMA redshift survey (BEARS) III: detailed study of emission lines from 71<i>Herschel</i>targets
<i>z</i>-GAL: A NOEMA spectroscopic redshift survey of bright<i>Herschel</i>galaxies
Strong lensing selection effects
<i>z</i>-GAL: A NOEMA spectroscopic redshift survey of bright <i>Herschel</i> galaxies
Euclid Preparation TBD. Characterization of convolutional neural networks for the identification of galaxy-galaxy strong lensing events
The bright extragalactic ALMA redshift survey (BEARS) I: redshifts of bright gravitationally lensed galaxies from the <i>Herschel</i> ATLAS
The bright extragalactic ALMA redshift survey (BEARS) – II. Millimetre photometry of gravitational lens candidates
<i>Euclid</i> preparation
The Cluster HEritage project with<i>XMM-Newton</i>: Mass Assembly and Thermodynamics at the Endpoint of structure formation
The strong gravitational lens finding challenge
Total density profile of massive early-type galaxies in H <scp>orizon</scp>-AGN simulation: impact of AGN feedback and comparison with observations
Density profile of dark matter haloes and galaxies in the horizon–agn simulation: the impact of AGN feedback
<i>Planck</i>’s dusty GEMS
THE STORY OF SUPERNOVA “REFSDAL” TOLD BY MUSE*
THE GRISM LENS-AMPLIFIED SURVEY FROM SPACE (GLASS). I. SURVEY OVERVIEW AND FIRST DATA RELEASE
GREAT3 results – I. Systematic errors in shear estimation and the impact of real galaxy morphology
HerMES: ALMA IMAGING OF<i>HERSCHEL</i>-SELECTED DUSTY STAR-FORMING GALAXIES
THE SLOAN LENS ACS SURVEY. XII. EXTENDING STRONG LENSING TO LOWER MASSES
Highly ionized region surrounding SN Refsdal revealed by MUSE
Dancing in the dark: galactic properties trace spin swings along the cosmic web
A dust-obscured massive maximum-starburst galaxy at a redshift of 6.34
CFHTLenS: the Canada–France–Hawaii Telescope Lensing Survey – imaging data and catalogue products
AGN-driven quenching of star formation: morphological and dynamical implications for early-type galaxies
GRAVITATIONAL LENS MODELS BASED ON SUBMILLIMETER ARRAY IMAGING OF<i>HERSCHEL</i>-SELECTED STRONGLY LENSED SUB-MILLIMETER GALAXIES AT<i>z</i>> 1.5
HerMES: CANDIDATE GRAVITATIONALLY LENSED GALAXIES AND LENSING STATISTICS AT SUBMILLIMETER WAVELENGTHS
Lancaster EPrints (Lancaster University) 2013cited by 114position: middle
H<sub>2</sub>O emission in high-<i>z</i>ultra-luminous infrared galaxies