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CombineHarvesterFlow: Joint Probe Analysis Made Easy with Normalizing Flows

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arxiv 2406.06687 v2 pith:TFT34YZV submitted 2024-06-10 astro-ph.CO

classification astro-ph.CO
keywords jointcombineharvesterflowflowsposteriorexperimentsfindmathcalnormalizing
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

We show how to efficiently sample the joint posterior of two non-covariant experiments with a large set of nuisance parameters. Specifically, we train an ensemble of normalizing flows to learn the posterior distribution of both experiments. Once trained, we can use the flows to reweight $\mathcal{O} (10^9)$ samples from both measurements to compute the joint posterior in seconds -- saving up to $\mathcal{O}(1)$ ton of $\text{CO}_2$ per Monte Carlo run. Using this new technique we find joint constraints between the Dark Energy Survey $3 \times 2$ point measurement, South Pole Telescope and Planck CMB lensing and a BOSS direct fit full shape analyses, for the first time. We find $\Omega_{\rm m} = 0.32^{+0.01}_{-0.01}$ and $S_8 = 0.79 ^ {+0.01}_ {-0.01}$. We release a public package called {\tt CombineHarvesterFlow} (https://github.com/pltaylor16/CombineHarvesterFlow) which performs these calculations.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Growth, geometry, and early-universe split of the matter density parameter $\Omega_{\rm m}$

    astro-ph.CO 2026-07 conditional novelty 5.5 of 10

    Splitting Ω_m into geometry, growth, and early-universe regimes yields mutually compatible values, yet ΔΩ_m^{geo,early} is 2σ from zero under combined DES, Planck (scale-cut), DESI, Pantheon+, and RSD data.

  2. A Sound Horizon-Free Measurement of $H_0$ in DESI 2024

    astro-ph.CO 2024-11 conditional novelty 5.0 of 10

    A sound horizon-free analysis of DESI 2024 full-shape clustering, CMB lensing, uncalibrated supernovae, and Lyman-alpha AP data gives H0 = 66.7 to 67.9 km/s/Mpc at sub-3% precision.

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