Mapping Lyman-alpha forest three-dimensional large scale structure in real and redshift space
arXiv:2107.07917 · doi:10.3847/1538-4357/ac5112
Abstract
This work presents a new physically-motivated supervised machine learning method, Hydro-BAM, to reproduce the three-dimensional Lyman- forest field in real and in redshift space learning from a reference hydrodynamic simulation, thereby saving about 7 orders of magnitude in computing time. We show that our method is accurate up to in the one- (PDF), two- (power-spectra) and three-point (bi-spectra) statistics of the reconstructed fields. When compared to the reference simulation including redshift space distortions, our method achieves deviations of up to in the monopole, up to in the quadrupole. The bi-spectrum is well reproduced for triangle configurations with sides up to . In contrast, the commonly-adopted Fluctuating Gunn-Peterson approximation shows significant deviations already neglecting peculiar motions at configurations with sides of in the bi-spectrum, being also significantly less accurate in the power-spectrum (within 5 up to ). We conclude that an accurate analysis of the Lyman- forest requires considering the complex baryonic thermodynamical large-scale structure relations. Our hierarchical domain specific machine learning method can efficiently exploit this and is ready to generate accurate Lyman- forest mock catalogues covering large volumes required by surveys such as DESI and WEAVE.
Accepted for publication by ApJ
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- Tracing the high-z cosmic web with Quaia: catalogues of voids and clusters in the quasar distribution
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