Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Galaxies: Formation, Evolution, Phenomena, Astronomy and Astrophysical Research, Gamma-ray bursts and supernovae, and Stellar, planetary, and galactic studies.
DESI 2024 VI: cosmological constraints from the measurements of baryon acoustic oscillations
DESI 2024 VII: cosmological constraints from the full-shape modeling of clustering measurements
DESI 2024 II: sample definitions, characteristics, and two-point clustering statistics
Comparing the DES-SN5YR and Pantheon+ SN cosmology analyses: investigation based on ‘evolving dark energy or supernovae systematics’?
The hierarchical growth of bright central galaxies and intracluster light as traced by the magnitude gap
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
Dark energy survey year 3 results: Cosmological constraints from cluster abundances, weak lensing, and galaxy clustering
Kilonova Constraints for the LIGO/Virgo/KAGRA Neutron Star Merger Candidate S250206dm: GW-MMADS Observations
Dark Energy Survey Year 6 Results: Synthetic-source Injection Across the Full Survey Using Balrog
The SRG/eROSITA all-sky survey
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: likelihood-free, simulation-based <i>w</i>CDM inference with neural compression of weak-lensing map statistics
The dark energy survey supernova program: investigating beyond-ΛCDM
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
A Search for Faint Resolved Galaxies Beyond the Milky Way in DES Year 6: A New Faint, Diffuse Dwarf Satellite of NGC 55
Cosmological constraints from the tomography of DES-Y3 galaxies with CMB lensing from ACT DR4
Dark energy survey year 3 results: cosmology from galaxy clustering and galaxy–galaxy lensing in harmonic space
Examining the self-interaction of dark matter through central cluster galaxy offsets
SPT-SZ MCMF: an extension of the SPT-SZ catalogue over the DES region
Cosmology from cross-correlation of ACT-DR4 CMB lensing and DES-Y3 cosmic shear
DESI complete calibration of the colour–redshift relation (DC3R2): results from early DESI data
The dark energy survey: detection of weak lensing magnification of supernovae and constraints on dark matter haloes
Dark Energy Survey Year 3 results: likelihood-free, simulation-based $w$CDM inference with neural compression of weak-lensing map statistics
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
Dark Energy Survey Year 3 results: magnification modelling and impact on cosmological constraints from galaxy clustering and galaxy–galaxy lensing
Joint analysis of Dark Energy Survey Year 3 data and CMB lensing from SPT and<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>P</mml:mi><mml:mi>l</mml:mi><mml:mi>a</mml:mi><mml:mi>n</mml:mi><mml:mi>c</mml:mi><mml:mi>k</mml:mi></mml:mrow></mml:math>. II. Cross-correlation measurements and cosmological constraints