Image de couverture de livre

Recovering CMB polarization maps with neural networks: Performance in realistic simulations

Fuente: arXiv

Enregistré dans:

Détails bibliographiques
Auteurs principaux:	Casas, J. M., Bonavera, L., González-Nuevo, J., Puglisi, G., Baccigalupi, C., Cabo, S. R., Cueli, M. M., Crespo, D., González-Gutiérrez, C., de Cos, F. J.
Format:	Preprint
Publié:	2023
Sujets:	Cosmology and Nongalactic Astrophysics Instrumentation and Methods for Astrophysics
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

Documents similaires

Recovering the CMB signal with neural networks
par: Casas, J. M., et autres
Publié: (2025)

Methodological refinement of the submillimeter galaxy cross-correlation function measurements and their uncertainty estimation
par: González-Nuevo, J., et autres
Publié: (2023)

Methodological refinement of the submillimeter galaxy magnification bias. II. Cosmological analysis with tomography
par: Bonavera, L., et autres
Publié: (2023)

Toward the measurement of neutrino masses: Performance of cosmic magnification with submillimeter galaxies
par: Cueli, M. M., et autres
Publié: (2024)

Cosmic magnification on high-redshift submillimeter galaxies
par: Cueli, Marcos M., et autres
Publié: (2025)

Cosmic Insights from Galaxy Clusters: Exploring Magnification Bias on Sub-millimeter Galaxies
par: Fernández-Fernández, Rebeca, et autres
Publié: (2024)

Methodological refinement of the submillimeter galaxy magnification bias. I. Cosmological analysis with a single redshift bin
par: Cueli, Marcos M., et autres
Publié: (2023)

Cosmic magnification on multi-catalogue Herschel submillimetre galaxies
par: Fernandez-Fernandez, R., et autres
Publié: (2025)

Spatial Variations of Polarized Synchrotron Emission in the QUIJOTE MFI Data using Neural Networks
par: Casas, J. M., et autres
Publié: (2025)

AtLAST -- A five fold increase in the number of identified Strongly Lensed Galaxies in the sub-millimetre and its consequences
par: González-Nuevo, Joaquín, et autres
Publié: (2025)

Mass density profiles at kiloparsec scales using the sub-millimetre galaxies magnification bias
par: Crespo, D., et autres
Publié: (2024)

ForSE+: Simulating non-Gaussian CMB foregrounds at 3 arcminutes in a stochastic way based on a generative adversarial network
par: Yao, Jian, et autres
Publié: (2024)

CMB Polarization Measurements
par: Carretti, E., et autres
Publié: (2024)

AtLAST -- Determination of Halo Mass Density Profiles at kpc Scales through Magnification Bias
par: González-Nuevo, Joaquín, et autres
Publié: (2025)

BrahMap: A scalable and modular map-making framework for the CMB experiments
par: Anand, Avinash, et autres
Publié: (2025)

AtLAST -- Cosmology with submillimetre galaxies magnification bias
par: Bonavera, Laura, et autres
Publié: (2025)

Improved simulation of non-Gaussian temperature and polarization CMB maps
par: Elsner, Franz, et autres
Publié: (2009)

Interpreting map-based $E$/$B$ spectral properties of CMB foregrounds
par: Weymann-Despres, Gilles, et autres
Publié: (2026)

Recovering unbiased CMB polarization maps using modern ground-based experiments with minimal assumptions about atmospheric emission
par: Biquard, Simon, et autres
Publié: (2025)

Multi-Clustering Needlet-ILC for CMB B-modes component separation
par: Carones, Alessandro, et autres
Publié: (2022)

BICEP/Keck XX: Component-separated maps of polarized CMB and thermal dust emission using Planck and BICEP/Keck Observations through the 2018 Observing Season
par: Keck Collaboration, et autres
Publié: (2025)

Extending Galactic foreground emission with neural networks
par: Puglisi, Giuseppe, et autres
Publié: (2026)

Development of realistic simulations for the polarization of the cosmic microwave background
par: Monelli, Marta
Publié: (2024)

Enhancing CMB map reconstruction and power spectrum estimation with convolutional neural networks
par: Costanza, Belén, et autres
Publié: (2023)

Running the small-correlated-against-large estimator at scale: Applications of small-scale CMB lensing estimators on realistic simulations
par: Chan, Victor C., et autres
Publié: (2024)

Addressing Synchrotron Challenges for CMB Observations: ELFS-SA Collaboration for Robust Foreground Removal
par: de la Hoz, E., et autres
Publié: (2025)

Inference of the optical depth to reionization $τ$ from $\textit{Planck}$ CMB maps with convolutional neural networks
par: Wolz, Kevin, et autres
Publié: (2023)

Little ado about everything II: an `emergent' dark energy from structure formation to rule cosmic tensions
par: Lapi, Andrea, et autres
Publié: (2025)

Signal Drop in Magnification Profiles: Combining Lensing Simulations and Observations
par: Crespo, David, et autres
Publié: (2025)

Systematic effects on lensing reconstruction from a patchwork of CMB polarization maps
par: Nagata, Ryo, et autres
Publié: (2024)

DeepWiener: Neural Networks for CMB polarization maps and power spectrum computation
par: Costanza, Belén, et autres
Publié: (2024)

Modeling beam chromaticity for high-resolution CMB analyses
par: Giardiello, S., et autres
Publié: (2024)

Fast End-to-End Framework for Cosmological Parameter Inference from CMB Data Using Machine Learning
par: Santos, Larissa, et autres
Publié: (2025)

The anomaly of the CMB power with the latest Planck data
par: Billi, M., et autres
Publié: (2023)

Dark Energy Survey Year 3 results: likelihood-free, simulation-based $w$CDM inference with neural compression of weak-lensing map statistics
par: Jeffrey, N., et autres
Publié: (2024)

Recovering the Dust Mass Budget with PRIMA
par: Traina, A., et autres
Publié: (2025)

Methods for CMB map analysis
par: Sullivan, Raelyn Marguerite, et autres
Publié: (2024)

$Ab$ $initio$ modeling of Galactic dust polarized CMB foreground
par: Kritsuk, Alexei G., et autres
Publié: (2026)

Robust CMB B-mode analysis with Needlet-ILC and simulation-based inference
par: Duivenvoorden, Adriaan J., et autres
Publié: (2025)

From few to many maps: A fast map-level emulator for extreme augmentation of CMB systematics datasets
par: Campeti, P., et autres
Publié: (2025)