Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Physics, Astrophysics, Redshift, Galaxy, Baryon, and Baryon acoustic oscillations.
DESI 2024: Constraints on physics-focused aspects of dark energy using DESI DR1 BAO data
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
Semi-analytical covariance matrices for two-point correlation function for DESI 2024 data
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
HOD-dependent systematics in Emission Line Galaxies for the DESI 2024 BAO analysis
Fiducial-cosmology-dependent systematics for the DESI 2024 BAO analysis
Analytical and EZmock covariance validation for the DESI 2024 results
Validating the galaxy and quasar catalog-level blinding scheme for the DESI 2024 analysis
Cosmological implications of DESI DR2 BAO measurements in light of the latest ACT DR6 CMB data
HOD-dependent systematics for luminous red galaxies in the DESI 2024 BAO analysis
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
Unraveling emission line galaxy conformity at <i>z</i> ∼ 1 with DESI early data
Positive Neutrino Masses with DESI DR2 via Matter Conversion to Dark Energy
Characterization of contaminants in the Lyman-alpha forest auto-correlation with DESI
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
Luminosity and Stellar Mass Functions of Faint Photometric Satellites around Spectroscopic Central Galaxies from DESI Year-1 Bright Galaxy Survey
DESI 2024: reconstructing dark energy using crossing statistics with DESI DR1 BAO data
The DESI one-per cent survey: exploring the halo occupation distribution of luminous red galaxies and quasi-stellar objects with <scp>AbacusSummit</scp>
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