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When measuring the Baryon Acoustic Oscillations (BAO) scale from galaxy surveys, one typically assumes a fiducial cosmology when converting redshift measurements into comoving distances and also when defining input parameters for the reconstruction algorithm.
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D. Valcin et al., Combined tracer analysis for DESI 2024 BAO analysis , in preparation (2025)
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O. Alves et al., Analytical covariance matrices of DESI galaxy power spectra , in preparation (2025)
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C. Zhao et al., Mock catalogues with survey realism for the DESI DR1 , in preparation (2025)
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