Imagen de Portada

Modeling the 3-point correlation function of projected scalar fields on the sphere

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Arvizu, Abraham, Aviles, Alejandro, Hidalgo, Juan Carlos, Moreno, Eladio, Niz, Gustavo, Rodriguez-Meza, Mario A., Samario, Sofía, Collaboration, The LSST Dark Energy Science
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

cTreeBalls: a fast 3-point correlation function code for clustering measurements
por: Rodriguez-Meza, Mario A., et al.
Publicado: (2026)

Non-Gaussian statistics in galaxy weak lensing: compressed three-point correlations and cosmological forecasts
por: Samario-Nava, Sofia, et al.
Publicado: (2025)

Analytical Noise Bias Correction for Precise Weak Lensing Shear Inference
por: Li, Xiangchong, et al.
Publicado: (2024)

Generation of realistic input parameters for simulating atmospheric point-spread functions at astronomical observatories
por: Hébert, Claire-Alice, et al.
Publicado: (2023)

Joint Modelling of Astrophysical Systematics for Cosmology with LSST Cosmic Shear
por: Šarčević, Nikolina, et al.
Publicado: (2024)

A direct detection method of galaxy intrinsic ellipticity-gravitational shear correlation in non-linear regimes using self-calibration
por: Bera, Avijit, et al.
Publicado: (2025)

Impact of Large-Scale Structure Systematics on Cosmological Parameter Estimation
por: Awan, Humna, et al.
Publicado: (2024)

Analyzing Line-of-sight selection biases in galaxy-scale strong lensing with external convergence and shear
por: Tang, Xianzhe TZ, et al.
Publicado: (2025)

Astrometric Redshifts of Supernovae
por: Lee, Jaemyoung Jason, et al.
Publicado: (2024)

LSST Strong Lensing Systems Dark Matter Sensitivity Analysis with Neural Ratio Estimators
por: Filipp, Andreas, et al.
Publicado: (2026)

Cluster Catalog Validation with Multiwavelength Data
por: Steelberg, Ethan K., et al.
Publicado: (2025)

YOLO-CL cluster detection in the Rubin/LSST DC2 simulation
por: Grishin, Kirill, et al.
Publicado: (2024)

Optimization of Weak Lensing Lightcone Simulations for Higher-Order Statistics in the LSST era
por: Mena-Fernández, J., et al.
Publicado: (2026)

MADNESS Deblender: Maximum A posteriori with Deep NEural networks for Source Separation
por: Biswas, Biswajit, et al.
Publicado: (2024)

Toward testing gravity with LSST using $E_G$
por: Leonard, C. D., et al.
Publicado: (2025)

Imaging systematics induced by galaxy sub-sample fluctuation: new systematics at second order
por: Kong, Hui, et al.
Publicado: (2025)

Halo Occupation Distribution estimation performance for LSST data
por: Cataldi, P., et al.
Publicado: (2026)

Gravitational-wave and electromagnetic detections in the context of the CosmoDC2 LSST synthetic catalog
por: Menote, Ranier, et al.
Publicado: (2025)

Dark Energy Survey: 2.1% measurement of the Baryon Acoustic Oscillation scale from the final dataset
por: Mena-Fernández, Juan, et al.
Publicado: (2024)

A halo model approach for mock catalogs of time-variable strong gravitational lenses
por: Abe, Katsuya T., et al.
Publicado: (2024)

Impact of survey spatial variability on galaxy redshift distributions and the cosmological $3\times2$-point statistics for the Rubin Legacy Survey of Space and Time (LSST)
por: Hang, Qianjun, et al.
Publicado: (2024)

The impact of environment on size: Galaxies are 50% smaller in the Fornax Cluster compared to the field
por: Chamba, Nushkia, et al.
Publicado: (2023)

Machine Learning LSST 3x2pt analyses -- forecasting the impact of systematics on cosmological constraints using neural networks
por: Boruah, Supranta S., et al.
Publicado: (2024)

$4\times3$ Point Correlation Functions in Galaxy Surveys: Impact of Baryonic Feedback
por: Bera, Avijit, et al.
Publicado: (2026)

An Empirical Model For Intrinsic Alignments: Insights From Cosmological Simulations
por: Van Alfen, Nicholas, et al.
Publicado: (2023)

A Cohesive Deep Drilling Field Strategy for LSST Cosmology
por: Gris, Philippe, et al.
Publicado: (2024)

Improving Photometric Redshift Estimates with Training Sample Augmentation
por: Moskowitz, Irene, et al.
Publicado: (2024)

Simulation-Based Inference Benchmark for Weak Lensing Cosmology
por: Zeghal, Justine, et al.
Publicado: (2024)

Galaxy Clustering with LSST: Effects of Number Count Bias from Blending
por: Levine, Benjamin, et al.
Publicado: (2024)

Simulation-Based Inference for Probabilistic Galaxy Detection and Deblending
por: Mendoza, Ismael, et al.
Publicado: (2026)

Differentiable Forward Modeling for Efficient and Accurate Shear Inference
por: Mendoza, Ismael, et al.
Publicado: (2026)

Propagating data-driven galaxy redshift distribution uncertainties in 3$\times$2-pt analyses
por: Ruiz-Zapatero, Jaime, et al.
Publicado: (2026)

Forecasting the Impact of Source Galaxy Photometric Redshift Uncertainties on the LSST $3\times2$pt Analysis
por: Zhang, Tianqing, et al.
Publicado: (2025)

Recovered SN Ia rate from simulated LSST images
por: Petrecca, Vincenzo, et al.
Publicado: (2024)

Forecast for growth-rate measurement using peculiar velocities from LSST supernovae
por: Rosselli, Damiano, et al.
Publicado: (2025)

Probabilistic Forward Modeling of Galaxy Catalogs with Normalizing Flows
por: Crenshaw, John Franklin, et al.
Publicado: (2024)

Lya2pcf: an efficient pipeline to estimate two- and three-point correlation functions of the Lyman-$α$ forest
por: De-Santiago, Josue, et al.
Publicado: (2025)

On the Reliability of Quasars as Cosmological Distance Indicators
por: Montiel, Ariadna, et al.
Publicado: (2025)

The little coadd that could: Estimating shear from coadded images
por: Armstrong, Robert, et al.
Publicado: (2024)

A Fully Photometric Approach to Type Ia Supernova Cosmology in the LSST Era: Host Galaxy Redshifts and Supernova Classification
por: Mitra, Ayan, et al.
Publicado: (2025)