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Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$

As of 12 August 2026, this Paper Citation Record lists 41 of 41 outbound references and 0 inbound Pith citation observations for arXiv:2608.08007.

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Outbound references

Observation 29bf134d-7f89-4ad1-9bee-cc0c81840e5e · outbound

This paper cites Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant.

Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant

Reference 1

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Observation dd7ef661-d36f-49e1-9841-e2294ccfa34e · outbound

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Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ Unresolved cited work

Reference 2

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Observation 06ea28e0-6d12-4e33-8037-364314edf2aa · outbound

This paper cites As shown in Fig.

Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ As shown in Fig

Reference 3

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Observation 209ca6b8-a2c4-4dfe-a4e8-29c3e255d5ee · outbound

This paper cites Exploring the expansion history of the uni- verse,.

Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ Exploring the expansion history of the uni- verse,

Reference 4

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Observation 95f2e209-e6a0-4e2a-9e0b-5c42fe7c2632 · outbound

This paper cites Measurements of Ω and Λ from 42 High Redshift Super- novae,.

Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ Measurements of Ω and Λ from 42 High Redshift Super- novae,

Reference 5

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Observation 5746e249-a8cb-4bb3-b38f-40c5a60a8f59 · outbound

This paper cites Accelerating Universes with Scaling Dark Matter.

Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ Accelerating Universes with Scaling Dark Matter

Reference 6

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Observation bf58aa94-152c-4956-9c22-db234f1466e4 · outbound

This paper cites DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints.

Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints

Reference 7

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Observation 9eddac66-670b-4336-a7e6-506c382f3fbf · outbound

This paper cites A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team.

Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team

Reference 8

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This paper cites Planck 2018 results. VI. Cosmological parameters.

Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ Planck 2018 results. VI. Cosmological parameters

Reference 9

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Observation f5ebe790-467c-4af2-a489-770f28888a15 · outbound

This paper cites Reconstruc- tion of dark energy and late-time cosmic expansion using the Weighted Function Regression method,.

Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ Reconstruc- tion of dark energy and late-time cosmic expansion using the Weighted Function Regression method,

Reference 10

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Observation e76830dd-6bfe-4ce7-8e35-22a63e20d0f5 · outbound

This paper cites Reconstruction of dark energy and expansion dynamics using Gaussian processes.

Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ Reconstruction of dark energy and expansion dynamics using Gaussian processes

Reference 11

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Observation af6326a4-4ba9-4be8-b99b-0d7a3cc762e9 · outbound

This paper cites Reconstructing equation of state of dark energy with principal component analysis.

Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ Reconstructing equation of state of dark energy with principal component analysis

Reference 12

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Observation d17eec04-5099-4c1c-8f9a-aa6db2723a23 · outbound

This paper cites Distance Priors from Planck Final Release.

Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ Distance Priors from Planck Final Release

Reference 13

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Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ Reconstructing dark energy with model independent methods after DESI DR2,

Reference 14

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This paper cites How the Dark Energy Can Reconcile \textit{Planck} with Local Determination of the Hubble Constant.

Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ How the Dark Energy Can Reconcile \textit{Planck} with Local Determination of the Hubble Constant

Reference 15

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Observation cbd71bd1-9503-446d-950f-b3c4a3dbe17a · outbound

This paper cites Reconstruction of the Dark Energy equation of state from latest data: the impact of theoretical priors.

Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ Reconstruction of the Dark Energy equation of state from latest data: the impact of theoretical priors

Reference 16

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Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ Dynamical dark energy in light of the latest observations

Reference 17

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Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ Reconstruction of the Dark Energy Equation of State from the Latest Obser- vations,

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Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes

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Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ Dynamical dark energy in light of the DESI DR2 baryonic acoustic oscillations mea- surements,

Reference 20

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Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ The frontier of simulation-based inference

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Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ Exploring Cosmic Origins with CORE: Cosmological Parameters

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Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ Efficient Computation of CMB anisotropies in closed FRW models

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Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ Fast and Credible Likelihood-Free Cosmology with Truncated Marginal Neural Ratio Estimation

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Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ Implicit Likelihood Inference of the Neutrino Mass Hierarchy from Cosmological Data

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Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ Conservative Constraints on Early Cosmology: an illustration of the Monte Python cosmological parameter inference code

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Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ Likelihood methods for the combined analysis of CMB temperature and polarisation power spectra

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Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ The Pantheon+ Analysis: Cosmological Constraints

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Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ Planck 2018 results. VIII. Gravitational lensing

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Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ SBI -- A toolkit for simulation-based inference

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Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ Massive optimal data compression and density estimation for scalable, likelihood-free inference in cosmology

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This paper cites Neural Density Estimation and Likelihood-free Inference.

Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ Neural Density Estimation and Likelihood-free Inference

Reference 36

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unresolved
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Observation 893e6604-40ab-4f17-91ac-00984385fe4e · outbound

This paper cites Accelerated Bayesian SED Modeling using Amortized Neural Posterior Estimation.

Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ Accelerated Bayesian SED Modeling using Amortized Neural Posterior Estimation

Reference 37

Resolution
verified exact
local_arxiv, observed 2026-08-12T00:39:25.300802Z

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No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation ce007824-90ef-4ba4-bead-fb24272b74d3 · outbound

This paper cites ${\rm S{\scriptsize IM}BIG}$: Mock Challenge for a Forward Modeling Approach to Galaxy Clustering.

Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ ${\rm S{\scriptsize IM}BIG}$: Mock Challenge for a Forward Modeling Approach to Galaxy Clustering

Reference 38

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no resolver link, observed 2026-08-12T00:39:25.224063Z

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source=pdf_text observed=2026-08-12T00:39:25.224063Z digest=sha256:ce229938595ecbf9e542b36952411083355cf124d0027884a7f20475626dd212

Observation c5fc1466-cd50-4211-9d4a-bd9ae9ad95d8 · outbound

This paper cites Validating Bayesian Inference Algorithms with Simulation-Based Calibration.

Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ Validating Bayesian Inference Algorithms with Simulation-Based Calibration

Reference 39

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no resolver link, observed 2026-08-12T00:39:25.228990Z

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Observation d066e4b8-fd0e-42a8-905d-0f366a452acd · outbound

This paper cites emcee: The MCMC Hammer.

Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ emcee: The MCMC Hammer

Reference 41

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no resolver link, observed 2026-08-12T00:39:25.238470Z

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Observation 60b497ba-cde2-4c05-ab1c-4a9d2596fc2f · outbound

This paper cites n1701   =L 1701   N1(0,1).

Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ n1701   =L 1701   N1(0,1)

Reference 1701

Resolution
verified fuzzy
raw_fallback, observed 2026-08-12T00:39:26.276368Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Pith citing papers

No inbound Pith citation observations are available.