Date |
Speaker |
Title |
Arxiv number |
Jan 19 |
Laura Herold |
New Early Dark Energy is compatible with current LSS data |
arXiv:2009.00006 |
Feb 2 |
Andrija Kostić |
The BOSS DR12 Full-Shape Cosmology: LCDM Constraints from the Large-Scale Galaxy Power Spectrum and Bispectrum Monopole |
arXiv:2112.04515 |
Feb 9 |
Andrea Pezotta |
Combined full shape analysis of BOSS galaxies and eBOSS quasars using an iterative emulator |
arXiv:2201.04679 |
Feb 16 |
Daniel Farrow |
AbacusHOD: A highly efficient extended multi-tracer HOD framework and its application to BOSS and eBOSS data |
arXiv:2110.11412 |
Feb 23 |
Alex Barreira |
The clustering of galaxies in the completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Primordial non-Gaussianity in Fourier Space |
arXiv:2106.13725 |
Mar 9 |
Vyoma Muralidhara |
The halo bispectrum as a sensitive probe of massive neutrinos and baryon physics |
arXiv:2202.07680 |
Mar 16 |
Agnė Semėnaitė |
Consistent lensing and clustering in a low-S8 Universe with BOSS, DES Year 3, HSC Year 1 and KiDS-1000 |
arXiv:2202.07440 |
Eiichiro Komatsu |
New physics from polarised light of the cosmic microwave background |
arXiv:2202.13919 |
Mar 23 |
Fabian Schmidt |
Not so fuzzy: excluding FDM with sizes and stellar kinematics of ultra-faint dwarf galaxies |
arXiv:2203.05750 |
Mar 30 |
Sten Delos |
Small-scale structure in vector dark matter |
arXiv:2203.11935 |
Apr 6 |
Paolo Campeti |
Bias on Tensor-to-Scalar Ratio Inference With Estimated Covariance Matrices |
arXiv:2202.05949 |
Apr 13 |
Ippei Obata |
Cosmic Birefringence: Cross-Spectra and Cross-Bispectra with CMB Anisotropies |
arXiv:2202.04584 |
Apr 20 |
Luisa Lucie-Smith |
From Images to Dark Matter: End-To-End Inference of Substructure From Hundreds of Strong Gravitational Lenses |
arXiv:2203.00690 |
May 4 |
Julia Stadler |
Wavelet Moments for Cosmological Parameter Estimation |
arXiv:2204.07646 |
May 11 |
Anik Halder |
JOINT CAMBRIDGE-MUNICH JOURNAL CLUB |
arXiv:2201.05607 |
May 25 |
Beatriz Tucci |
Can we actually constrain fNL using the scale-dependent bias effect? An illustration of the impact of galaxy bias uncertainties using the BOSS DR12 galaxy power spectrum |
arXiv:2205.05673 |
Angelo Caravano |
Cosmological Bootstrap in Slow Motion |
arXiv:2205.10340 |
Jun 1 |
Sam Goldstein |
Determining the Hubble Constant without the Sound Horizon: A 3.6% Constraint on H0 from Galaxy Surveys, CMB Lensing and Supernovae |
arXiv:2204.02984 |
Jun 8 |
Linda Blot |
Galaxy Cluster Statistics in Modified Gravity Cosmologies |
arXiv:2205.13015 |
Jun 15 |
Sherry Suyu |
The AGEL Survey: Spectroscopic Confirmation of Strong Gravitational Lenses in the DES and DECaLS Fields Selected Using Convolutional Neural Network |
arXiv:2205.05307 |
Jun 22 |
Maja Lujan Niemeyer |
HI intensity mapping with MeerKAT: power spectrum detection in cross-correlation with WiggleZ galaxies |
arXiv:2206.01579 |
Jun 29 |
Marta Monelli |
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Jul 6 |
Matteo Esposito |
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