Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Galaxies: Formation, Evolution, Phenomena, Astronomy and Astrophysical Research, Cosmology and Gravitation Theories, and Stellar, planetary, and galactic studies.
Dark Energy Survey Year 3 results: Simulation-based cosmological inference with wavelet harmonics, scattering transforms, and moments of weak lensing mass maps. Validation on simulations
Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and weak lensing
Dark Energy Survey Year 3 results: A 2.7% measurement of baryon acoustic oscillation distance scale at redshift 0.835
Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and galaxy-galaxy lensing using the MagLim lens sample
Dark energy survey year 3 results: Cosmology with peaks using an emulator approach
Dark Energy Survey Year 3 Results: Measuring the Survey Transfer Function with Balrog
Dark Energy Survey Year 3 results: Cosmology with moments of weak lensing mass maps
Dark Energy Survey Year 3 results: Exploiting small-scale information with lensing shear ratios
Dark Energy Survey Year 3 results: Cosmology from combined galaxy clustering and lensing validation on cosmological simulations
Dark Energy Survey Year 3 results: Galaxy-halo connection from galaxy-galaxy lensing
Cross-correlation of Dark Energy Survey Year 3 lensing data with ACT and <i>Planck</i> thermal Sunyaev-Zel’dovich effect observations. I. Measurements, systematics tests, and feedback model constraints
The Observed Evolution of the Stellar Mass–Halo Mass Relation for Brightest Central Galaxies
Superclustering with the Atacama Cosmology Telescope and Dark Energy Survey. I. Evidence for Thermal Energy Anisotropy Using Oriented Stacking
Velocity dispersions of clusters in the Dark Energy Survey Y3 redMaPPer catalogue
Constraints on Dark Matter Properties from Observations of Milky Way Satellite Galaxies
Dark Energy Survey Year 3 Results: Photometric Data Set for Cosmology
Dark Energy Survey Year 3 results: redshift calibration of the weak lensing source galaxies
Dark Energy Survey Year 1 Results: Cosmological Constraints from Cluster Abundances, Weak Lensing, and Galaxy Correlations
Dark Energy Survey year 3 results: covariance modelling and its impact on parameter estimation and quality of fit
Assessing tension metrics with dark energy survey and Planck data
Galaxy morphological classification catalogue of the Dark Energy Survey Year 3 data with convolutional neural networks
Baryonic imprints on DM haloes: population statistics from dwarf galaxies to galaxy clusters
Probing Galaxy Evolution in Massive Clusters Using ACT and DES: Splashback as a Cosmic Clock
A machine learning approach to galaxy properties: joint redshift–stellar mass probability distributions with Random Forest
DES Y1 results: Splitting growth and geometry to test <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi mathvariant="normal">Λ</mml:mi><mml:mi>CDM</mml:mi></mml:math>
The WaZP galaxy cluster sample of the dark energy survey year 1
Dark Energy Survey Year 3 results: galaxy sample for BAO measurement
Dark Energy Survey Year 3 Results: Galaxy mock catalogs for BAO analysis
Dark Energy Survey Year 1 Results: Cosmological constraints from cluster abundances and weak lensing
STRIDES: a 3.9 per cent measurement of the Hubble constant from the strong lens system DES J0408−5354