Abstract
In this work, we develop a theoretical model for the cross-power spectrum of the galaxy density field before and after standard baryonic acoustic oscillation (BAO) reconstruction. Using this model, we extract the redshift-space distortion (RSD) parameter from the cross-power spectrum. The model is validated against a suite of high-resolution $N$-body simulations, demonstrating its accuracy and robustness for cosmological analyses.
Original language | English |
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Journal | The Astrophysical Journal |
Publication status | Accepted for publication - 21 Apr 2025 |
Keywords
- astro-ph.CO
- UKRI
- STFC
- ST/W001225/1