Area of research
Astronomy and Astrophysics · Condensed Matter Physics
Research interest
Research interests include Physics, Dark energy, Astrophysics, Weak gravitational lensing, Cosmology, and Redshift.
Dark Energy Survey Year 3 results: Simulation-based cosmological inference with wavelet harmonics, scattering transforms, and moments of weak lensing mass maps. II. cosmological results
The Atacama Cosmology Telescope: DR6 Gravitational Lensing Map and Cosmological Parameters
The Atacama Cosmology Telescope: A Measurement of the DR6 CMB Lensing Power Spectrum and Its Implications for Structure Growth
SPT clusters with DES and HST weak lensing. II. Cosmological constraints from the abundance of massive halos
Weak lensing combined with the kinetic Sunyaev–Zel’dovich effect: a study of baryonic feedback
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
SPT clusters with DES and HST weak lensing. I. Cluster lensing and Bayesian population modeling of multiwavelength cluster datasets
Cosmological constraints from the tomography of DES-Y3 galaxies with CMB lensing from ACT DR4
Cosmology from cross-correlation of ACT-DR4 CMB lensing and DES-Y3 cosmic shear
The Simons Observatory: impact of bandpass, polarization angle and calibration uncertainties on small-scale power spectrum analysis
Enhancing weak lensing redshift distribution characterization by optimizing the Dark Energy Survey Self-Organizing Map Photo-z method
DES Y3 + KiDS-1000: Consistent cosmology combining cosmic shear surveys
Dark Energy Survey Year 3 results: Constraints on extensions to <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> with weak lensing and galaxy clustering
Joint analysis of Dark Energy Survey Year 3 data and CMB lensing from SPT and <i>Planck</i>. III. Combined cosmological constraints
Detection of the significant impact of source clustering on higher order statistics with DES Year 3 weak gravitational lensing data
Cosmological shocks around galaxy clusters: a coherent investigation with DES, SPT, and ACT
Dark Energy Survey Year 3 results: redshift calibration of the <scp>MagLim</scp> lens sample from the combination of SOMPZ and clustering and its impact on cosmology
Cosmology intertwined: A review of the particle physics, astrophysics, and cosmology associated with the cosmological tensions and anomalies
Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and weak lensing
Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to data calibration
Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to modeling uncertainty
Dark Energy Survey year 3 results: Constraints on cosmological parameters and galaxy-bias models from galaxy clustering and galaxy-galaxy lensing using the redMaGiC sample
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: cosmological constraints from the analysis of cosmic shear in harmonic space
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: High-precision measurement and modeling of galaxy-galaxy lensing
Dark Energy Survey Year 3 results: Exploiting small-scale information with lensing shear ratios
Constraining the baryonic feedback with cosmic shear using the DES Year-3 small-scale measurements