2023
DOI: 10.1088/1475-7516/2023/04/010
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SimBIG: mock challenge for a forward modeling approach to galaxy clustering

Abstract: Simulation-Based Inference of Galaxies (SimBIG) is a forward modeling framework for analyzing galaxy clustering using simulation-based inference. In this work, we present the SimBIG forward model, which is designed to match the observed SDSS-III BOSS CMASS galaxy sample. The forward model is based on high-resolution Quijote N-body simulations and a flexible halo occupation model. It includes full survey realism and models observational systematics such as angular … Show more

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Cited by 15 publications
(8 citation statements)
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“…Secondly, we perform a high-dimensional numerical integral in order to obtain our theory skew-spectra, which is a time-consuming task and therefore prevents us from varying the full νΛCDM parameters simultaneously in the likelihood analysis. This could be potentially accomplished with help of simulation-based inference methods [82][83][84][85][86]. For example, a related recent work [56] uses the SIMBIG forward modelling framework to perform simulation-based inference with skew-spectra through normalizing flows.…”
Section: Jcap05(2024)011mentioning
confidence: 99%
“…Secondly, we perform a high-dimensional numerical integral in order to obtain our theory skew-spectra, which is a time-consuming task and therefore prevents us from varying the full νΛCDM parameters simultaneously in the likelihood analysis. This could be potentially accomplished with help of simulation-based inference methods [82][83][84][85][86]. For example, a related recent work [56] uses the SIMBIG forward modelling framework to perform simulation-based inference with skew-spectra through normalizing flows.…”
Section: Jcap05(2024)011mentioning
confidence: 99%
“…Although not particular to SBI, forward modeling presents several advantages over other methods, such as the straightforward inclusion of observational effects, including window functions, redshift-space distortions and systematic effects [46,57,[65][66][67][68]. In the context of the EFT forward model employed here, forward modeling at the field-level allows us to reach essentially arbitrary perturbative (loop) order [69].…”
Section: Forward Modelingmentioning
confidence: 99%
“…In the context of galaxy clustering, recent progress has been made by using graphs networks to capture the map information from the galaxy distribution [22,23]. SBI has been widely used in the cosmological inference context, including weak-lensing [24][25][26][27], type IA supernovae [24,25,[28][29][30][31][32], standard sirens [33,34], CMB [35,36], galaxy cluster abundance [37], Gaussian and lognormal fields [38][39][40][41], dark-matter overdensity fields [40,42], voids [43], dark-matter halos [23,44] and galaxies [45][46][47][48].…”
Section: Introductionmentioning
confidence: 99%
“…Therefore, expanding this project to observed galaxy clustering requires first robustly generating realistic galaxies from the properties the SC-SAM produces. This would entail selecting a galaxy sample that CAMELS-SAM is large and resolved enough to simulate (e.g., perhaps the 2D clustering of emission line galaxies in a small but well-studied field like COSMOS; Khostovan et al 2018), as well as a detailed understanding of the selection function and observational systematics for the sample (such as, e.g., Hahn et al 2022Hahn et al , 2023 include in their forward model for BOSS CMASS galaxies). Additionally, expanding to other SAMs (and their unique parameterization of galaxy physics) could improve the neural networks' ability to marginalize over many forms of astrophysical prescriptions and better constrain Ω M and σ 8 for similar galaxy selections.…”
Section: Camels-sam Data Release and Possibilitiesmentioning
confidence: 99%