Imagen de Portada

Evaluating extensions to LCDM: an application of Bayesian model averaging and selection

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Paradiso, S., McGee, G., Percival, W. J.
Formato:	Preprint
Publicado:	2024
Materias:	Cosmology and Nongalactic Astrophysics
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

A convenient approach to characterizing model uncertainty with application to early dark energy solutions of the Hubble tension
por: Paradiso, S., et al.
Publicado: (2023)

Reducing nuisance prior sensitivity via non-linear reparameterization, with application to EFT analyses of large-scale structure
por: Paradiso, S., et al.
Publicado: (2024)

LOO-PIT: A sensitive posterior test
por: Nguyen, Alan B. H., et al.
Publicado: (2024)

Cosmological measurements from the CMB and BAO are insensitive to the tail probability in the assumed likelihood
por: Krywonos, Jordan, et al.
Publicado: (2024)

HOD-informed prior for EFT-based full-shape analyses of LSS
por: Zhang, Hanyu, et al.
Publicado: (2024)

Galaxy and halo angular clustering in LCDM and Modified Gravity cosmologies
por: Drozda, Paweł, et al.
Publicado: (2022)

Testing the framework of the halo occupation distribution with assembly bias modeling and empirical extensions
por: Zhai, Zhongxu, et al.
Publicado: (2024)

The fallacies of LCDM falsifications
por: Blanchard, Alain
Publicado: (2025)

Dynamics of pairwise motions in the fully non-linear regime in LCDM and Modified Gravity cosmologies
por: Jaber, Mariana, et al.
Publicado: (2023)

Number count of Gravitational Waves and Supernovae in Luminosity Distance space for LCDM and Scalar-Tensor theories
por: Balaudo, Anna, et al.
Publicado: (2023)

A Comparative Test of the LCDM and R_h=ct Cosmologies Based on Upcoming Redshift Drift Measurements
por: Melia, Fulvio
Publicado: (2024)

II- A hydrodynamical CLONE of the Virgo cluster to confront observed and synthetic galaxy population twins in a dense environment
por: Sorce, Jenny G., et al.
Publicado: (2026)

Dynamic or Systematic? Bayesian model selection between dark energy and supernova biases
por: Ormondroyd, A. N., et al.
Publicado: (2025)

Planck constraints on the scale dependence of isotropic cosmic birefringence
por: Ballardini, M., et al.
Publicado: (2025)

Tomographic halo model of the unWISE-Blue galaxies using cross-correlations with BOSS CMASS galaxies
por: Krolewski, Alex, et al.
Publicado: (2025)

Measuring the baryon fraction using galaxy clustering
por: Krolewski, Alex, et al.
Publicado: (2024)

Estimating non-gaussian bias using counts of tracers
por: Dalal, Neal, et al.
Publicado: (2025)

Euclid Quick Data Release (Q1). The average far-infrared properties of Euclid-selected star-forming galaxies
por: Euclid Collaboration, et al.
Publicado: (2025)

A new method to determine $H_0$ from cosmological energy-density measurements
por: Krolewski, Alex, et al.
Publicado: (2024)

Constraining Primordial Non-Gaussianity with Density-Split Clustering
por: Morawetz, James, et al.
Publicado: (2024)

The effective volume of supernovae samples and sample variance
por: Zhai, Zhongxu, et al.
Publicado: (2023)

Owl-z: a Bayesian tool to select z \geq 7 quasars
por: Ezziati, Meriam, et al.
Publicado: (2026)

The XXL Survey LIV. X-ray Luminosity Function and Luminosity-Mass Relation of Optically Selected Galaxy Groups
por: Wood, C., et al.
Publicado: (2025)

Effects of anisotropy in an anisotropic extension of $w$CDM model
por: Yadav, Vikrant, et al.
Publicado: (2024)

Super sample covariance and the volume scaling of galaxy survey covariance matrices
por: Schreiner, Greg, et al.
Publicado: (2024)

Self-calibrating BAO measurements in the presence of Small Displacement Interlopers
por: Nguyen, Alan B. H., et al.
Publicado: (2023)

Neural Networks for cosmological model selection and feature importance using Cosmic Microwave Background data
por: Ocampo, I., et al.
Publicado: (2024)

The energy conditions and model selection in the local Universe
por: Chandak, Namit, et al.
Publicado: (2026)

Forward analytical model for the optical selection bias on galaxy cluster lensing profiles
por: Costanzi, M., et al.
Publicado: (2026)

Halo Lightcones with Optimised Orientation and Interpolation in Cosmological Simulations -- an application to mock H$α$ selected galaxies
por: Ramakrishnan, Sujatha, et al.
Publicado: (2025)

Alcock-Paczyński effect on void-finding: Implications for void-galaxy cross-correlation modelling
por: Radinović, Slađana, et al.
Publicado: (2024)

Capturing statistical isotropy violation with rotational averages
por: R, Vaishali, et al.
Publicado: (2026)

Clustering analysis of medium-band selected high-redshift galaxies
por: Ebina, H., et al.
Publicado: (2025)

Bayesian data analysis for sky-averaged 21-cm experiments with contamination from linearly polarised foreground
por: Shen, Emma, et al.
Publicado: (2024)

A general Bayesian model-validation framework based on null-test evidence ratios, with an example application to global 21-cm cosmology
por: Sims, Peter H., et al.
Publicado: (2025)

Euclid: Testing photometric selection of emission-line galaxy targets
por: Cagliari, M. S., et al.
Publicado: (2024)

The FLAMINGO Project: A comparison of galaxy cluster samples selected on mass, X-ray luminosity, Compton-Y parameter, or galaxy richness
por: Kugel, Roi, et al.
Publicado: (2024)

Bayesian analysis of $α$-Starobinsky model with Planck, ACT and DESI data
por: Carrion, Karim, et al.
Publicado: (2026)

Efficient prior sensitivity analysis for Bayesian model comparison
por: Hu, Zixiao, et al.
Publicado: (2026)

Modelling the BOSS void-galaxy cross-correlation function using a neural-network emulator
por: Fraser, Tristan S., et al.
Publicado: (2024)