Cosmological Constraints from Dark Energy Survey Year 1 Cluster Lensing and Abundances with Simulation-based Forward-Modeling
Andr’es N. Salcedo, Eduardo Rozo, Hao-Yi Wu, David H. Weinberg, Pranav Chiploonkar, Chun-Hao To, Shulei Cao, Eli S. Rykoff, Nicole Marcelina Gountanis, Conghao Zhou
arXiv:2510.25706v1 Announce Type: new
Abstract: We present a simulation-based forward-modeling framework for cosmological inference from optical galaxy-cluster samples, and apply it to the abundance and weak-lensing signals of DES-Y1 redMaPPer clusters. The model embeds cosmology-dependent optical selection using a counts-in-cylinders approach, while also accounting for cluster miscentering and baryonic feedback in lensing. Applied to DES-Y1, and assuming a flat $Lambda$CDM cosmology, we obtain $Omega_m=0.254^{+0.026}_{-0.020}$ and $sigma_8=0.826^{+0.030}_{-0.034}$, consistent with a broad suite of low-redshift structure measurements, including recent full-shape analyses, the DES/KiDS/HSC 3$times$2 results, and most cluster-abundance studies. Our results are also consistent with textit{Planck}, with the difference being significant at $2.58sigma$. These results establish simulation-based forward-modeling of cluster abundances as a promising new tool for precision cosmology with Stage~IV survey data.arXiv:2510.25706v1 Announce Type: new
Abstract: We present a simulation-based forward-modeling framework for cosmological inference from optical galaxy-cluster samples, and apply it to the abundance and weak-lensing signals of DES-Y1 redMaPPer clusters. The model embeds cosmology-dependent optical selection using a counts-in-cylinders approach, while also accounting for cluster miscentering and baryonic feedback in lensing. Applied to DES-Y1, and assuming a flat $Lambda$CDM cosmology, we obtain $Omega_m=0.254^{+0.026}_{-0.020}$ and $sigma_8=0.826^{+0.030}_{-0.034}$, consistent with a broad suite of low-redshift structure measurements, including recent full-shape analyses, the DES/KiDS/HSC 3$times$2 results, and most cluster-abundance studies. Our results are also consistent with textit{Planck}, with the difference being significant at $2.58sigma$. These results establish simulation-based forward-modeling of cluster abundances as a promising new tool for precision cosmology with Stage~IV survey data.