S14
Astrophysical foregrounds for precision cosmology
Communauté
Contact : soc_s14@sf2a
Main language for discussions : ENGLISH
The quest for precision cosmology has entered a regime where astrophysical systematic uncertainties increasingly dominate over statistical ones. With the unprecedented sensitivity of upcoming cosmological surveys, astrophysical foregrounds have become the new frontier. They simultaneously complicate the extraction of cosmological information and offer new opportunities to deepen our understanding of the Universe. This session aims to bring together researchers working at the interface of cosmology and astrophysics to discuss the characterization, modeling, mitigation, and scientific exploitation of foreground signals.
Foreground emission arises from a wide range of Galactic and extragalactic structures along the line of sight. In the Milky Way, synchrotron radiation from spiraling electrons and thermal dust emission from the interstellar medium (ISM) dominate. Beyond the Galaxy, radio and infrared point sources, the thermal and kinetic Sunyaev-Zel’dovich effects, gravitational lensing, the cosmic infrared background (CIB), and redshifted molecular lines (e.g., CO) all contribute significant signals.
Building on growing cross-disciplinary efforts within the French community, we propose a session organized around four themes.
- Our Galaxy as a foreground
- Extragalactic Foregrounds
- Disentangling the multi-frequency sky – Component separation methods
- Multi-Wavelength Synergies and Joint Inference
We welcome contributions (talks + posters) on any of these four themes. The SOC will seek to bring together experts covering all four themes and to reflect the diversity and dynamism of the French community, including balanced representation across genders and career stages.
Organizing committee : Benjamin Beringue (APC, chair), Clément Leloup (IJCLAB), Adélie Gorce (IAS), Abhishek Maniyar (LAPTh), Margherita Lembo (IAP), Andrea Bracco (LUX), Athanasia Gkogkou (CEA), Giulio Fabbian (IAS)
Programme des présentations orales
| Horaire | Auteur | Titre | Abstract | Présentation (fichier) |
|---|---|---|---|---|
| 14h00 – 14h30 | Désert, F.-X., Sen, A., Macias-Pérez, J.F. | Precision modelling of the millimetre dust emission | Fichier | – |
| 14h30 – 14h50 | Silvia Micheli | Impact of Galactic EB correlation on the calibration of CMB B-modes for future space missions | Fichier | – |
| 14h50 – 15h10 | Vinzl, S., Aumont, J., Vacher, L., Génova-Santos, R.T., Adak, D., Rizzieri, A. | Galactic Science with the LiteBIRD satellite: Spectral characterization of diffuse Galactic polarized emission at the angular power spectrum level | Fichier | – |
| 15h10 – 15h30 | Modeling the Thermal dust with Dust Temperature Ladder Model | |||
| 15h30 – 16h00 | Pause Café | |||
| 16h00 – 16h20 | Mertens, F.G. | ML-Enhanced Foreground Removal Methods for 21-cm Experiments Preparing for the SKA Era | Fichier | – |
| 16h20 – 16h40 | Gilles Weymann-Despres, Léo Vacher, Michael E. Jones, Angela C. Taylor, Carlo Baccigalupi, A.J. Banday, Richard D.P. Grumitt, Nicoletta Krachmalnicoff | An improved characterisation of CMB foregrounds with map-space PE/PB spectral analysis | Fichier | – |
| 16h40 – 17h00 | Douspis, M., BATMAN-ANR team | BATMAN v Foregrounds: Dawn of Coherence | Fichier | – |
| 17h00 – 17h20 | Zagatti, G., Calabrese, E., Chiocchetta, C., Gerbino, M., Negrello, M., Pagano, L. | A halo model approach to describe clustering and emission of the two main star-forming galaxy populations for Cosmic Infrared Background studies | Fichier | – |
| 17h20 – 17h40 | Pamphile, L. | High redshift galaxies unveiled by lensing clusters at millimetre wavelengths | Fichier | – |
| 17h40 – 18h00 | Cléa Millard, Benjamin L’Huillier, Marian Douspis | Model independent test of the FLRW metric and the curvature in light of DESI DR2 | Fichier | – |