Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Galaxies: Formation, Evolution, Phenomena, Astronomy and Astrophysical Research, Stellar, planetary, and galactic studies, and Cosmology and Gravitation Theories.
DESI 2024: Constraints on physics-focused aspects of dark energy using DESI DR1 BAO data
Extended dark energy analysis using DESI DR2 BAO measurements
Dynamical dark energy in light of the DESI DR2 baryonic acoustic oscillations measurements
Modified gravity constraints from the full shape modeling of clustering measurements from DESI 2024
Constraining primordial non-Gaussianity with DESI 2024 LRG and QSO samples
Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO
Production of alternate realizations of DESI fiber assignment for unbiased clustering measurement in data and simulations
Validation of the DESI DR2 measurements of baryon acoustic oscillations from galaxies and quasars
Evidence for large baryonic feedback at low and intermediate redshifts from kinematic Sunyaev-Zel’dovich observations with ACT and DESI photometric galaxies
Fiducial-cosmology-dependent systematics for the DESI 2024 BAO analysis
Characterization of DESI fiber assignment incompleteness effect on 2-point clustering and mitigation methods for DR1 analysis
Validating the galaxy and quasar catalog-level blinding scheme for the DESI 2024 analysis
Measuring σ <sub>8</sub> using DESI Legacy Imaging Surveys Emission-Line galaxies and Planck CMB lensing, and the impact of dust on parameter inference
Cosmological implications of DESI DR2 BAO measurements in light of the latest ACT DR6 CMB data
DESI peculiar velocity survey – Fundamental Plane
Backlighting extended gas halos around luminous red galaxies: Kinematic Sunyaev-Zel’dovich effect from DESI Y1 and ACT data
A sound horizon-free measurement of <i>H</i> <sub>0</sub> in DESI 2024
Positive Neutrino Masses with DESI DR2 via Matter Conversion to Dark Energy
Blinding scheme for the scale-dependence bias signature of local primordial non-Gaussianity for DESI 2024
Exploring the interaction between the MW and LMC with a large sample of blue horizontal branch stars from the DESI survey
Mitigating imaging systematics for DESI 2024 emission Line Galaxies and beyond
DESI DR1 Lyα 1D power spectrum: the optimal estimator measurement
Model-independent measurement of the matter-radiation equality scale in DESI 2024
DESI 2024: reconstructing dark energy using crossing statistics with DESI DR1 BAO data
Overview of the Fiber System for the Dark Energy Spectroscopic Instrument
Changing-look Active Galactic Nuclei from the Dark Energy Spectroscopic Instrument. I. Sample from the Early Data
Optimal 1D Ly α forest power spectrum estimation – III. DESI early data
Baryon acoustic oscillation theory and modelling systematics for the DESI 2024 results
Analysis of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>DESI</mml:mi><mml:mo stretchy="false">×</mml:mo><mml:mi>DES</mml:mi></mml:mrow></mml:math> using the Lagrangian effective theory of LSS
Archetype-based Redshift Estimation for the Dark Energy Spectroscopic Instrument Survey