Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Both sides previous revision Previous revision
Next revision
Previous revision
publications [2025/01/07 10:51]
Déborah Paradis
publications [2025/01/07 11:14] (current)
Déborah Paradis
Line 109: Line 109:
 Fernández-Torreiro,​ M., Rubiño-Martín,​ J. A., López-Caraballo,​ C. H., et al., 2023, 526, 1343, MNRAS, QUIJOTE scientific results - X. Spatial variations of anomalous microwave emission along the galactic plane Fernández-Torreiro,​ M., Rubiño-Martín,​ J. A., López-Caraballo,​ C. H., et al., 2023, 526, 1343, MNRAS, QUIJOTE scientific results - X. Spatial variations of anomalous microwave emission along the galactic plane
  
-Fernández-Torreiro,​ M., Génova-Santos, R. T., Rubiño-Martín, J. A. , et al., 2023, MNRAS52711945QUIJOTE Scientific Results – XVII. Studying ​the Anomalous Microwave Emission in the Andromeda Galaxy ​with QUIJOTE-MFI+Iwashita, R., Kataoka, J., and Sofue, Y., 2023, ApJ958831Broadband Radio Study of the North Polar Spur: Origin of the Spectral Turnover ​with Insights into the X-Ray and Gamma-Ray Spectra ​
  
-FerreiraT.,  Alonso, D., Garcia-GarciaC., ChisariNE., 2023submittedX-ray - cosmic shear cross-correlationsfirst detection and constraints on baryonic effects  ​+KhabibullinII. ,ChurazovE. M., BykovAM., et al.2024MNRAS, 527, 5683, Discovery of a one-sided radio filament of PSR J0538+2817 in S147escape of relativistic PWN leptons into surrounding supernova remnant? ​
  
-Holm-Hansen, C., PutmanM. E., and KimDA., 2023submitted to MNRAS, ​Properties ​of 3D HI Filaments ​in the Smith High Velocity Cloud +López-Caraballo, C. H., Ruiz-GranadosB., Genova SantosR., et al., 2024, MNRAS, ​527, 171, QUIJOTE scientific results – XIII. Intensity and polarization study of supernova remnants ​in the QUIJOTE-MFI wide survey: CTB 80, Cygnus Loop, HB 21, CTA 1, Tycho and HB 9
  
-IwashitaR., KataokaJ., and SofueY., 2023ApJ958831Broadband Radio Study of the North Polar SpurOrigin ​of the Spectral Turnover with Insights ​into the X-Ray and Gamma-Ray Spectra ​+KhabibullinI. I. ,ChurazovE. M., BykovA. M., et al.2024MNRAS5275683, Discovery of a one-sided radio filament ​of PSR J0538+2817 in S147escape ​of relativistic PWN leptons ​into surrounding supernova remnant? ​
  
-López-CaraballoC. H., Ruiz-GranadosB., Genova SantosR., et al., 2024, 527171MNRASQUIJOTE scientific results – XIII. Intensity ​and polarization study of supernova remnants ​in the QUIJOTE-MFI wide survey: CTB 80, Cygnus Loop, HB 21, CTA 1, Tycho and HB 9+ ZhangW., ZhouJ., EsimbekJ., et al., 2024, A&A68899Kinematics ​and star formation ​of hub-filament systems ​in W49A 
  
-KhabibullinII. ,ChurazovE. M., BykovAM., et al., 2024, MNRAS5275683Discovery of a one-sided radio filament of PSR J0538+2817 in S147escape of relativistic PWN leptons into surrounding supernova remnant? ​+FerreiraT.,  Alonso, D., Garcia-GarciaC., ChisariNE., 2024, Physical Review Letters1331001X-ray - cosmic shear cross-correlationsfirst detection and constraints on baryonic effects  ​
  
- ZhangW., ZhouJ., EsimbekJ., et al., 2024, Accepted for publication in A&AKinematics and star formation of hub-filament systems in W49A + Durán-CamachoE., Duarte-CabralA., PettittAR., 2024, MNRAS532, 126, Self-consistent modelling of the Milky Way structure using live potentials ​
  
- ​Durán-CamachoE., Duarte-CabralA., Pettitt, A. R., 2024, Accepted for publication in MNRAS, ​Self-consistent modelling of the Milky Way structure using live potentials ​+Fernández-TorreiroM., Génova-SantosR. T., Rubiño-MartínJ. A. , et al., 2024, MNRAS, ​527, 11945, QUIJOTE Scientific Results – XVII. Studying ​the Anomalous Microwave Emission in the Andromeda Galaxy with QUIJOTE-MFI
  
  ​Paradis,​ D., Mény, C., Noriega-Crespo,​ A., et al., 2024, A&A, 691, 241, Inferring the dust emission at submillimeter and millimeter wavelengths using neural networks  ​Paradis,​ D., Mény, C., Noriega-Crespo,​ A., et al., 2024, A&A, 691, 241, Inferring the dust emission at submillimeter and millimeter wavelengths using neural networks
Line 135: Line 135:
  San, M.; Galloway, M.; Gjerløw, E., et al., 2024, submitted to A&A, Cosmoglobe DR2. III. Improved modelling of zodiacal light with COBE-DIRBE through global Bayesian analysis  San, M.; Galloway, M.; Gjerløw, E., et al., 2024, submitted to A&A, Cosmoglobe DR2. III. Improved modelling of zodiacal light with COBE-DIRBE through global Bayesian analysis
  
-    ​+ ​Holm-Hansen,​ C., Putman, M. E., and Kim, D. A., 2024, accepted ​ in MNRAS, Properties of 3D HI Filaments in the Smith High Velocity Cloud  
 + 
 + ​McCarthy,​ F., 2024arXiv240513470M,​ Large-scale galactic-dust-cleaned cosmic infrared background maps from Planck PR4 and HI4PI with pyilc 
 + 
 + ​Cartechini,​ E., Bartolomei, A., Greco, G., et al., 2024, ASPC, 535, 303, Using galaxy catalogs to localise gravitational-wave sources: a new Virtual Observatory plug-in to esteem their completeness