Imagen de Portada

ForSE+: Simulating non-Gaussian CMB foregrounds at 3 arcminutes in a stochastic way based on a generative adversarial network

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Yao, Jian, Krachmalnicoff, Nicoletta, Foschi, Marianna, Puglisi, Giuseppe, Baccigalupi, Carlo
Formato:	Preprint
Publicado:	2024
Materias:	Cosmology and Nongalactic Astrophysics Instrumentation and Methods for Astrophysics
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

Blind mitigation of foreground-induced biases on primordial $B$ modes for ground-based CMB experiments
por: Mustafa, Aliza, et al.
Publicado: (2026)

Interpreting map-based $E$/$B$ spectral properties of CMB foregrounds
por: Weymann-Despres, Gilles, et al.
Publicado: (2026)

$B$-sure I: Minkowski functionals as robustness test for tensor-to-scalar ratio detection from CMB observations
por: Ranucci, Claudio, et al.
Publicado: (2025)

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

Extending Galactic foreground emission with neural networks
por: Puglisi, Giuseppe, et al.
Publicado: (2026)

BROOM: a python package for model-independent analysis of microwave astronomical data
por: Carones, Alessandro, et al.
Publicado: (2026)

Full-sky Models of Galactic Microwave Emission and Polarization at Sub-arcminute Scales for the Python Sky Model
por: Experiment Galactic Science Group, et al.
Publicado: (2025)

Recovering the CMB signal with neural networks
por: Casas, J. M., et al.
Publicado: (2025)

Is cosmic birefringence due to dark energy or dark matter? Simulation-based inference
por: Carralot, Florie, et al.
Publicado: (2026)

Impact of Galactic non-Gaussian foregrounds on CMB lensing measurements
por: Abril-Cabezas, Irene, et al.
Publicado: (2025)

Multi-Clustering Needlet-ILC for CMB B-modes component separation
por: Carones, Alessandro, et al.
Publicado: (2022)

BrahMap: A scalable and modular map-making framework for the CMB experiments
por: Anand, Avinash, et al.
Publicado: (2025)

Dark matter search with CMB: a study of foregrounds
por: Zhang, Zi-Xuan, et al.
Publicado: (2023)

Implications of scattering for CMB foreground emission modelling
por: Li, Jia-Rui, et al.
Publicado: (2024)

Combining CMB datasets with consistent foreground modelling
por: Tristram, M., et al.
Publicado: (2025)

$Ab$ $initio$ modeling of Galactic dust polarized CMB foreground
por: Kritsuk, Alexei G., et al.
Publicado: (2026)

CMB Polarization Measurements
por: Carretti, E., et al.
Publicado: (2024)

The Simons Observatory: Combining cross-spectral foreground cleaning with multitracer $B$-mode delensing for improved constraints on inflation
por: Hertig, Emilie, et al.
Publicado: (2024)

Probing foreground residuals in cleaned CMB temperature maps from Planck
por: Patel, Sanjeet K., et al.
Publicado: (2025)

Recovering CMB polarization maps with neural networks: Performance in realistic simulations
por: Casas, J. M., et al.
Publicado: (2023)

Inference of $B$-mode polarization in the presence of non-Gaussian foregrounds
por: Li, Sen, et al.
Publicado: (2025)

Optimization of foreground moment deprojection for semi-blind CMB polarization reconstruction
por: Carones, Alessandro, et al.
Publicado: (2024)

Least response method to separate CMB spectral distortions from foregrounds
por: Maillard, J. -P., et al.
Publicado: (2024)

Are CMB derived cosmological parameters affected by foregrounds associated to nearby galaxies?
por: Toscano, Facundo, et al.
Publicado: (2024)

Forecasting the performance of the Minimally Informed foreground cleaning method for CMB polarization observations
por: Leloup, Clément, et al.
Publicado: (2025)

Pixel domain implementation of the Minimally Informed CMB MAp foreground Cleaning method
por: Morshed, Magdy, et al.
Publicado: (2024)

Revisiting the CMB homogeneity scale: low multipoles removal effect and extragalactic foreground masking
por: Shao, Xiaoyun, et al.
Publicado: (2025)

Rotation of the CMB polarisation by foreground lensing
por: Di Dio, Enea, et al.
Publicado: (2019)

Fast End-to-End Framework for Cosmological Parameter Inference from CMB Data Using Machine Learning
por: Santos, Larissa, et al.
Publicado: (2025)

The Simons Observatory: Assessing the Impact of Dust Complexity on the Recovery of Primordial $B$-modes
por: Liu, Yiqi, et al.
Publicado: (2025)

Disentangling CMB $μ$ and $y$ spectral distortions from foregrounds with poorly defined spectral shapes
por: Mihalchenko, A. O.
Publicado: (2025)

Cleaning Galactic foregrounds with spatially varying spectral dependence from CMB observations with \texttt{fgbuster}
por: Rizzieri, Arianna, et al.
Publicado: (2025)

Measuring the diffuse Galactic synchrotron spectral index and curvature between 45 and 2300 MHz
por: Irfan, Melis O., et al.
Publicado: (2025)

Improved simulation of non-Gaussian temperature and polarization CMB maps
por: Elsner, Franz, et al.
Publicado: (2009)

Denoising weak lensing mass maps with diffusion model and generative adversarial network
por: Aoyama, Shohei D., et al.
Publicado: (2025)

CMB polarization non-Gaussianity from accreting primordial black holes
por: Jensen, Trey W., et al.
Publicado: (2024)

The CMB Cold Spot as predicted by foregrounds around nearby galaxies
por: Lambas, Diego Garcia, et al.
Publicado: (2023)

CIBER 4th flight fluctuation analysis: Measurements of near-IR auto- and cross-power spectra on arcminute to sub-degree scales
por: Feder, Richard M., et al.
Publicado: (2025)

Denoising weak lensing mass maps with diffusion model: systematic comparison with generative adversarial network
por: Aoyama, Shohei D., et al.
Publicado: (2025)

Towards detecting Primordial non-Gaussianity in the CMB using Spherical Convolutional Neural Networks
por: Melsen, Jorik, et al.
Publicado: (2024)