Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Physics, Astrophysics, Redshift, Galaxy, Baryon, and Cosmic microwave background.
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
Semi-analytical covariance matrices for two-point correlation function for DESI 2024 data
Comparing Compressed and Full-Modeling analyses with FOLPS: implications for DESI 2024 and beyond
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
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
Characterization of DESI fiber assignment incompleteness effect on 2-point clustering and mitigation methods for DR1 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
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
DESI peculiar velocity survey – Fundamental Plane
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
Blinding scheme for the scale-dependence bias signature of local primordial non-Gaussianity for DESI 2024
Construction of the damped <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:mi>Ly</mml:mi> <mml:mi>α</mml:mi> </mml:mrow> </mml:math> absorber catalog for DESI DR2 <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:mrow> <mml:mrow> <mml:mi>Ly</mml:mi> <mml:mi>α</mml:mi> </mml:mrow> </mml:mrow> </mml:mrow> </mml:math> BAO
Exploring the interaction between the MW and LMC with a large sample of blue horizontal branch stars from the DESI survey
Characterization of contaminants in the Lyman-alpha forest auto-correlation with DESI
Mitigating imaging systematics for DESI 2024 emission Line Galaxies and beyond
Stellar reddening map from DESI imaging and spectroscopy
Selection of high-redshift Lyman-Break Galaxies from broadband and wide photometric surveys
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
Overview of the Fiber System for the Dark Energy Spectroscopic Instrument
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