Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Physics, Astrophysics, Galaxy, Redshift, Astronomy, and Dark energy.
DESI 2024 VI: cosmological constraints from the measurements of baryon acoustic oscillations
DESI DR2 results. II. Measurements of baryon acoustic oscillations and cosmological constraints
DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman alpha forest
DESI 2024 III: baryon acoustic oscillations from galaxies and quasars
DESI 2024 VII: cosmological constraints from the full-shape modeling of clustering measurements
DESI 2024: Constraints on physics-focused aspects of dark energy using DESI DR1 BAO data
Extended dark energy analysis using DESI DR2 BAO measurements
DESI 2024 II: sample definitions, characteristics, and two-point clustering statistics
DESI 2024 V: Full-Shape galaxy clustering from galaxies and quasars
Constraints on neutrino physics from DESI DR2 BAO and DR1 full shape
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
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
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
Constraining the phase shift of relativistic species in DESI BAOs
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
Characterization of contaminants in the Lyman-alpha forest auto-correlation with DESI
Forward modeling fluctuations in the DESI LRGs target sample using image simulations
Stellar reddening map from DESI imaging and spectroscopy
Selection of high-redshift Lyman-Break Galaxies from broadband and wide photometric surveys