BAO from angular clustering: optimization and mitigation of theoretical systematics
K. C. Chan, M. Crocce, A. J. Ross, S. Avila, J. Elvin-Poole, M., Manera, W. J. Percival, R. Rosenfeld, T. M. C. Abbott, F. B. Abdalla, S., Allam, E. Bertin, D. Brooks, D. L. Burke, A. Carnero Rosell, M. Carrasco, Kind, J. Carretero, F. J. Castander, C. E. Cunha, C. B. D'Andrea

TL;DR
This paper evaluates methods for measuring BAO using angular correlation functions, focusing on optimizing the pipeline and mitigating systematic biases in survey data analysis.
Contribution
It compares different BAO fitting estimators, identifies the least biased method, and proposes an eigenmode expansion approach to reduce covariance estimation uncertainties.
Findings
MLE provides the least biased BAO fit results.
Incorrect template assumptions can cause BAO angular shifts.
Eigenmode expansion reduces covariance estimation fluctuations.
Abstract
We study the methodology and potential theoretical systematics of measuring Baryon Acoustic Oscillations (BAO) using the angular correlation functions in tomographic bins. We calibrate and optimize the pipeline for the Dark Energy Survey Year 1 dataset using 1800 mocks. We compare the BAO fitting results obtained with three estimators: the Maximum Likelihood Estimator (MLE), Profile Likelihood, and Markov Chain Monte Carlo. The fit results from the MLE are the least biased and their derived 1- error bar are closest to the Gaussian distribution value after removing the extreme mocks with non-detected BAO signal. We show that incorrect assumptions in constructing the template, such as mismatches from the cosmology of the mocks or the underlying photo- errors, can lead to BAO angular shifts. We find that MLE is the method that best traces this systematic biases, allowing to…
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