Imagen de Portada

Characterizing the correlation properties of the atmospheric emission in the 10-20 GHz range with QUIJOTE MFI data

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Chappard, Apolline, Rubiño-Martín, José Alberto, Génova-Santos, Ricardo Tanausú
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

Characterising the properties of the atmospheric emission at Teide Observatory in the 10-20 GHz range with QUIJOTE data
por: Chappard, Apolline, et al.
Publicado: (2025)

Forecasting synchrotron spectral parameters with QUIJOTE-MFI2 in combination with Planck and WMAP
por: Almeida, Ana, et al.
Publicado: (2025)

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

QUIJOTE scientific results XIX. New constraints on the synchrotron spectral index using a semi-blind component separation method
por: Adak, Debabrata, et al.
Publicado: (2025)

QUIJOTE scientific results -- XVIII. New constraints on the polarization of the Anomalous Microwave Emission in bright Galactic regions: $ρ$\,Ophiuchi, Perseus and W43
por: González-González, R., et al.
Publicado: (2024)

Spectral Signatures of Spinning Dust from Grain Ensembles in Diverse Environments: A Combined Theoretical and Observational Study
por: Zhang, Zheng, et al.
Publicado: (2026)

MeerKAT discovery of GHz radio emission extending from Abell 3017 toward Abell 3016
por: Hu, Dan, et al.
Publicado: (2024)

Sensitivity-Improved Polarization Maps at 40 GHz with CLASS and WMAP data
por: Shi, Rui, et al.
Publicado: (2024)

CCAT: LED Mapping and Characterization of the 280 GHz TiN KID Array
por: Middleton, Alicia, et al.
Publicado: (2024)

Characterization of contaminants in the Lyman-alpha forest auto-correlation with DESI
por: Guy, J., et al.
Publicado: (2024)

A high-dynamic-range view of the growth of structure and the warm/hot Universe
por: Di Mascolo, Luca, et al.
Publicado: (2025)

CHEX-MATE: New detections and properties of the radio diffuse emission in massive clusters with MeerKAT
por: Balboni, M., et al.
Publicado: (2025)

Measuring anisotropies in the PTA band with cross-correlations
por: Cusin, Giulia, et al.
Publicado: (2025)

Constraints on CMBR flux due to high-z dust emission
por: Lopez-Corredoira, Martin
Publicado: (2026)

The correlations between galaxy properties in different environments of the cosmic web
por: Nandi, Anindita, et al.
Publicado: (2023)

CLASS Angular Power Spectra and Map-Component Analysis for 40 GHz Observations through 2022
por: Eimer, Joseph R., et al.
Publicado: (2023)

Galaxy-Point Spread Function correlations as a probe of weak-lensing systematics with UNIONS data
por: Guerrini, Sacha, et al.
Publicado: (2024)

Clustering of emission line galaxies with IllustrisTNG -- II. cosmology challenge with anisotropic correlation functions and ELG-halo connections
por: Osato, Ken, et al.
Publicado: (2026)

Forecast of CMB TB and EB correlations for AliCPT-1
por: Dou, Jiazheng, et al.
Publicado: (2024)

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

Tracing correlations between galaxy properties across the Cosmic Web: An IllustrisTNG-based study
por: Nandi, Anindita, et al.
Publicado: (2025)

Cosmoglobe DR2. V. Spatial correlations between thermal dust and ionized carbon emission in Planck HFI and COBE-DIRBE
por: Gjerløw, E., et al.
Publicado: (2026)

Constraints on the variation of the fine-structure constant at 3<z<10 with JWST emission-line galaxies
por: Jiang, Linhua, et al.
Publicado: (2024)

The European Low Frequency Survey on the Simons Array
por: Mennella, Aniello, et al.
Publicado: (2024)

Recovering unbiased CMB polarization maps using modern ground-based experiments with minimal assumptions about atmospheric emission
por: Biquard, Simon, et al.
Publicado: (2025)

First Sardinia Radio Telescope detection of the Sunyaev-Zel'dovich effect at 18.6 GHz
por: Cocchi, S., et al.
Publicado: (2026)

In-Flight Performance of Spider's 280 GHz Receivers
por: Shaw, Elle C., et al.
Publicado: (2024)

Applications of 1.4 GHz diagnostics to Type Ia Supernova host galaxies
por: Ramaiya, S., et al.
Publicado: (2026)

Towards an optimal marked correlation function analysis for the detection of modified gravity
por: Kärcher, Martin, et al.
Publicado: (2024)

Impact of cosmic web on galaxy properties and their correlations: Insights from Principal Component Analysis
por: Nandi, Anindita, et al.
Publicado: (2024)

High significance detection at 4.8 GHz of the radio halo in the Coma galaxy cluster with the Sardinia Radio Telescope
por: Marchegiani, P., et al.
Publicado: (2026)

Modeling spatially-resolved galactic H$α$ emission for galaxy clustering
por: Rapoport, Ivan, et al.
Publicado: (2025)

Observations of the galaxy cluster CL 0217+70 and its surrounding region at 1.4 GHz with the Sardinia Radio Telescope
por: Marchegiani, P., et al.
Publicado: (2024)

On the contributions of extragalactic CO emission lines to ground-based CMB observations
por: Kokron, Nickolas, et al.
Publicado: (2024)

GroundBIRD Telescope: Systematics Modelization of MKID Arrays Response
por: Jo, Yonggil, et al.
Publicado: (2025)

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

X-ray emission in IllustrisTNG circum-cluster environments. II -- Possible origins of the soft X-ray excess emission
por: Gouin, Celine, et al.
Publicado: (2025)

Gravitational waves and galaxies cross-correlations: a forecast on GW biases for future detectors
por: Zazzera, Stefano, et al.
Publicado: (2024)

High-Efficiency and Low-Noise Detectors for the Upgraded CLASS 90 GHz Focal Plane
por: Núñez, Carolina, et al.
Publicado: (2024)

Cosmoglobe DR1. III. First full-sky model of polarized synchrotron emission from all WMAP and Planck LFI data
por: Watts, D. J., et al.
Publicado: (2023)