Self-supervised component separation for the extragalactic submillimeter sky
A proof of concept on the use of deep learning for CMB component separation
2022, arXiv:2212.02847
Quasi-spherical superclusters
A study of quasi spherical supercclusters in Optical and SZ
2022 A&A, arXiv:2210.13294
Retrieving cosmological information from small-scale CMB foregrounds. II. The kinetic Sunyaev Zel'dovich effect
A new analysis of Planck and SPT using small scale secondary anisotropies (tSZ and kSZ) to get information on reionisation
2022 A&A, arXiv:2202.08698
X-ray emission from cosmic web filaments in SRG/eROSITA data
Detection of cosmic filaments in the eRosita early release data by stacking
2022, arXiv:2206.00084
Constraining the mass and redshift evolution of the hydrostatic mass bias using the gas mass fraction in galaxy clusters
A use of the gas fraction of ESZ galaxy clusters to study cosmology and hydrostatic mass bias evolution
2022, arXiv:2204.12823
Retrieving cosmological information from small-scale CMB foregrounds. I. The thermal Sunyaev Zel'dovich effect
DESCRIPTION
2022 A&A, arXiv:2109.03272
Constraining cosmology with a new all-sky Compton parameter map from the Planck PR4 data
Building and using a news SZ map from Planck PR4 data for cosmological constraints
2022 MNRAS, arXiv:2110.08880
Euclid preparation. XV. Forecasting cosmological constraints for the Euclid and CMB joint analysis
Euclid forecast study using cross correlation between CMB and Euclid Survey
2022 A&A, arXiv:2106.08346
BISOU: a balloon project to measure the CMB spectral distortions
Description of the BISOU balloon
2021 MG16, arXiv:2111.00246
X-ray analysis of the Planck-detected triplet-cluster system PLCK G334.8-38
Analysis of the three components of the Planck supercluster with XMM data
2021 A&A, arXiv:2107.07801
MILCANN: A tSZ map for galaxy cluster detection assessed using a neural network
Machine learning based weighted Planck y-map
2021 A&A, arXiv:1702.00075
High-resolution tomography for galaxy spectroscopic surveys with angular redshift fluctuations
Forecasts of the angular redshift flucuations in future galaxy surveys
2021 A&A, arXiv:2007.14412
PACT. II. Pressure profiles of galaxy clusters using Planck and ACT
New pressure profile from Planck and ACT clusters from the PACT map (combined Planck and ACT SZ map)
2021 A\&A , arXiv:2105.05607
First detection of stacked X-ray emission from cosmic web filaments
Determination of stacked filaments properties from Xray observations and predictions
2021 A&A , arXiv:2011.05343
PACT. I. Combining ACT and Planck data for improved extraction of tSZ signal
First SZ map combining Planck and ACT data with large and small scales
2019, A&A arXiv:1902.00350
Density and temperature of cosmic-web filaments on scales of tens of megaparsecs
Determination of stacked filaments properties from SZ and lensing observations
2020 A&A , arXiv:1911.09706
Impact of systematics on cosmological parameters from future Galaxy Clusters surveys
Forecasts of future surveys depending of the precision on systematics
2020 A&A arXiv:2005.10204
Improved constraints on reionisation from CMB observations: A parameterisation of the kSZ effect
New physical parameterisation of the kSZ for reionisation studies
2020 A&A, arXiv:2004.06616
Mass bias evolution in tSZ cluster cosmology
Investigation of possible mass and redshift evolution of the mass bias of SZ clusters
2019 A&A, arXiv:1901.03096
Star formation rates and stellar masses from machine learning
Galaxy properties from Optical and IR colors with machine learning technique
2019 A&A arXiv:1901.01932
The COSMOS-UltraVISTA stellar-to-halo mass relationship: new insights on galaxy formation efficiency out to $z\sim5$
Stellar-to-halo mass relationship from precise galaxy stellar mass function measurements in the COSMOS field
2019 A&A arXiv:1810.10557
Detection of intercluster gas in superclusters using the thermal Sunyaev-Zel'dovich effect
Detection of misssing baryons in by stacking the SZ signal of superclusters in Planck ymap
2019 A&A arXiv:1805.04555
Constraints from thermal Sunyaev-Zeldovich cluster counts and power spectrum combined with CMB
Constraints on LCDM, nuCDM and wCDM by combining cluster number counts and tSZ power spectrum from Planck with and without CMB.
2018A&A...614A..13S, arXiv:1708.00697
Gas and galaxies in filament between clusters of galaxies: The study of A399-A401
Detection and measure of the SZ effect and galaxy properties in Galaxy Cluster pairs
2018A&A...609A..49B, arXiv:1710.08699
Observational constraints on key-parameters of cosmic reionisation history
Combined analyses of direct reionisation measurements, high redshift galaxie luinosity function and CMB to constrain escape fraction and clumping factor evolution
2018A&A...616A.113G, arXiv:1710.04152
MILCANN : A neural network assessed tSZ map for galaxy cluster detection
Neural network applied for SZ cluster detection
A&A submitted, arXiv:1702.00075
Cosmology with Planck SZ cluster number counts
Cosmological constraints from Planck SZ clusters
A&A 2014, arXiv:1303.5080
Cosmology from Planck tSZ power spectrum
Cosmological constraints from the first power spectrum from Planck tSZ map
A&A 2014, arXiv:1303.5081