BAO Reconstruction Under Redshift Uncertainty
Arizona Cosmology Lab · 2026–present
- Question. Measure how photometric-redshift smearing changes the value of baryon acoustic oscillation reconstruction.
- Data. Simulated galaxy catalogs and Monte Carlo ensembles for Roman and Rubin-like survey conditions.
- Built. Designed the analysis, forward-model framework, covariance cross-checks, and Bayesian inference pipeline.
- Result. Reduced an inference bias by four to six times and mapped where a 20–40% precision benefit becomes statistically insignificant.