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Cited article:

ELG×LRG Distribution through Dark Matter Halo Dynamics

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Investigating the galaxy–halo connection of DESI emission-line galaxies with SHAMe-SF

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Generalized framework for likelihood-based field-level inference of growth rate from velocity and density fields

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DESI Emission-line Galaxies: Clustering Dependence on Stellar Mass and [O II] Luminosity

T. Hagen, K. S. Dawson, Z. Zheng, J. Aguilar, S. Ahlen, S. BenZvi, D. Bianchi, D. Brooks, F. J. Castander, T. Claybaugh, A. Cuceu, A. de la Macorra, P. Doel, S. Ferraro, A. Font-Ribera, J. E. Forero-Romero, E. Gaztañaga, S. Gontcho A Gontcho, V. Gonzalez-Perez, G. Gutierrez, C. Hahn, K. Honscheid, M. Ishak, S. Juneau, R. Kehoe, et al.
The Astrophysical Journal 992 (1) 121 (2025)
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Beyond the two-point correlation: Constraining primordial non-Gaussianity with density-perturbation moments

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Astronomy & Astrophysics 704 A297 (2025)
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