Imagen de Portada

Full-sky Models of Galactic Microwave Emission and Polarization at Sub-arcminute Scales for the Python Sky Model

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Experiment Galactic Science Group, Borrill, Julian, Clark, Susan E., Delabrouille, Jacques, Frolov, Andrei V., Ghosh, Shamik, Hensley, Brandon S., Hicks, Monica D., Krachmalnicoff, Nicoletta, Lau, King, Norton, Myra M., Pryke, Clement, Puglisi, Giuseppe, Remazeilles, Mathieu, Russier, Elisa, Thorne, Benjamin, Yao, Jian, Zonca, Andrea
Formato:	Preprint
Publicado:	2025
Materias:	Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

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

Planck CO revisited: Improved CO line emission maps from Planck space mission observations
por: Ghosh, Shamik, et al.
Publicado: (2023)

The case for an all-sky millimetre survey at sub-arcminute resolution
por: Désert, François-Xavier, et al.
Publicado: (2024)

How bad could it be? Modelling the 3D complexity of the polarised dust signal using moment expansion
por: Vacher, Léo, et al.
Publicado: (2024)

Separation of polarized dust emission in Planck observations with Scattering Transforms
por: Tsouros, Alexandros, et al.
Publicado: (2026)

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

Roman Galactic Plane Survey Definition Committee Report
por: Committee, Roman Galactic Plane Survey Definition
Publicado: (2025)

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

Unbiased Primordial Gravitational Wave Inference from the CMB with SMICA
por: Steier, Alexander, 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)

Statistical Analysis of PAHs as a Tracer of Anomalous Microwave Emission Using DIRBE Data
por: Sponseller, Danielle, et al.
Publicado: (2025)

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

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

The Square Kilometer Array as a Cosmic Microwave Background Experiment
por: Zegeye, David, et al.
Publicado: (2024)

Field-level constraints on cosmic birefringence from hybrid ILC maps combining $E$- and $B$-mode channels
por: Remazeilles, Mathieu
Publicado: (2025)

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)

On the Shapes of Interstellar Grains: Modeling Extinction and Polarization by Spheroids and Continuous Distributions of Ellipsoids
por: Draine, B. T., et al.
Publicado: (2017)

Models of the night-sky brightness and the efficiency of searching for exoplanets with the microlensing method
por: Ipatov, S. I.
Publicado: (2025)

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

The Optical Extinction Law Depends on Magnetic Field Orientation: The $R_V$-$ψ$ Relation
por: Hensley, Brandon S.
Publicado: (2024)

Enhanced foreground mitigation in thermal SZ Compton-$y$ maps via polarization and deprojection
por: Chandran, Jyothis, et al.
Publicado: (2026)

Modeling Binary Lenses and Sources with the BAGLE Python Package
por: Bhadra, T. Dex, et al.
Publicado: (2025)

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

Evidence for relativistic Sunyaev-Zeldovich effect in Planck CMB maps with an average electron-gas temperature of $T_{\rm e}\simeq 5$ keV
por: Remazeilles, Mathieu, et al.
Publicado: (2024)

Analyzing PAHs as a Tracer of Anomalous Microwave Emission Near the Galactic Plane Using the COSMOGLOBE DIRBE Reduction
por: Pare, Dylan M., et al.
Publicado: (2026)

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

CONCERTO at APEX -- On-sky performance in continuum
por: Hu, W., et al.
Publicado: (2024)

Characterization of the decametre sky at subarcminute resolution
por: Groeneveld, C., et al.
Publicado: (2024)

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

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

Star clusters in the gamma-ray sky
por: Peron, Giada
Publicado: (2025)

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

The Simons Observatory: component separation pipelines for B-modes
por: Wolz, Kevin, et al.
Publicado: (2024)

An all-sky catalogue of stellar reddening values
por: Paunzen, E., et al.
Publicado: (2024)

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves
por: Bianchini, Federico, et al.
Publicado: (2025)

Planck data revisited: low-noise synchrotron polarisation maps from the WMAP and Planck space missions
por: Delabrouille, Jacques
Publicado: (2024)

Feature Intensity Mapping: Polycyclic Aromatic Hydrocarbon Emission from All Galaxies Across Cosmic Time
por: Cheng, Yun-Ting, et al.
Publicado: (2025)

PAH Emission Spectra and Band Ratios for Arbitrary Radiation Fields with the Single Photon Approximation
por: Richie, Helena M., et al.
Publicado: (2025)

Fast partial-sky spherical harmonic transforms
por: Carron, Julien, et al.
Publicado: (2026)

An updated and improved thermal SZ $y$-map from Planck PR4 data
por: Chandran, Jyothis, et al.
Publicado: (2023)