Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Gamma-ray bursts and supernovae, Astronomy and Astrophysical Research, Galaxies: Formation, Evolution, Phenomena, and Stellar, planetary, and galactic studies.
Dark Energy Survey: Implications for cosmological expansion models from the final DES baryon acoustic oscillation and supernova data
Union through UNITY: Cosmology with 2000 SNe Using a Unified Bayesian Framework
Comparing the DES-SN5YR and Pantheon+ SN cosmology analyses: investigation based on ‘evolving dark energy or supernovae systematics’?
The Dark Energy Survey Supernova Program: an updated measurement of the Hubble constant using the inverse distance ladder
The Dark Energy Survey Supernova Program: Light Curves and 5 Yr Data Release
Dark Energy Survey: A 2.1% measurement of the angular baryonic acoustic oscillation scale at redshift <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msub><mml:mrow><mml:mi>z</mml:mi></mml:mrow><mml:mrow><mml:mi>eff</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mn>0.85</mml:mn></mml:mrow></mml:math> from the final dataset
The dark energy survey supernova program: investigating beyond-ΛCDM
Dark energy survey year 3 results: cosmology from galaxy clustering and galaxy–galaxy lensing in harmonic space
The Dark Energy Survey 5-yr photometrically classified type Ia supernovae without host-galaxy redshifts
Optical Spectroscopy of Type Ia Supernovae by the Carnegie Supernova Projects I and II
The dark energy survey: detection of weak lensing magnification of supernovae and constraints on dark matter haloes
The Mass Density of Mg ii Absorbers from the Australian Dark Energy Survey
High-quality Extragalactic Legacy-field Monitoring (HELM) with DECam
OzDES Reverberation Mapping Program: Hβ lags from the 6-yr survey
Measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic Sunyaev-Zel’dovich effect with SPT-3G and DES
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
Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and weak lensing
The Pantheon+ Analysis: SuperCal-fragilistic Cross Calibration, Retrained SALT2 Light-curve Model, and Calibration Systematic Uncertainty
Dark Energy Survey Year 3 results: A 2.7% measurement of baryon acoustic oscillation distance scale at redshift 0.835
The DECam Local Volume Exploration Survey Data Release 2
Dark energy survey year 3 results: Cosmology with peaks using an emulator approach
Dark Energy Survey Year 3 results: Cosmology with moments of weak lensing mass maps
Concerning colour: The effect of environment on type Ia supernova colour in the dark energy survey
A galaxy-driven model of type Ia supernova luminosity variations
The dark energy survey 5-yr photometrically identified type Ia supernovae
Dwarf AGNs from Optical Variability for the Origins of Seeds (DAVOS): insights from the dark energy survey deep fields
Measuring Cosmological Parameters with Type Ia Supernovae in redMaGiC Galaxies
MIGHTEE-Hi: Evolution of Hi Scaling Relations of Star-forming Galaxies at z < 0.5*
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 Dark Energy Survey supernova program: cosmological biases from supernova photometric classification