activity
20182022
most citedPrimordial Non-Gaussianity

54 citations · 54 across the 2 of their papers we have counts for

collaborators

7 papers

astro-ph.CO2022

The two-loop bispectrum in the effective theory of large-scale structure

Tobias Baldauf, Mathias Garny, Petter Taule +1

We study the bispectrum of large-scale structure in the EFTofLSS including corrections up to two-loop. We derive an analytic result for the double-hard limit of the two-loop correc…

astro-ph.CO2021

Precise Calibration of the One-Loop Trispectrum in the Effective Field Theory of Large Scale Structure

Theodore Steele, Tobias Baldauf

The Large-Scale Structure (LSS) of the universe has the potential to provide decisive answers to the remaining open questions in cosmology. Early attempts at modelling it analytica…

astro-ph.CO2020

Non-perturbative halo clustering from cosmological density peaks

Tobias Baldauf, Sandrine Codis, Vincent Desjacques +1

Associating the formation sites of haloes with the maxima of the smoothed linear density field, we present non-perturbative predictions for the Lagrangian and evolved halo correlat…

astro-ph.CO2020

Precise Calibration of the One-Loop Bispectrum in the Effective Field Theory of Large Scale Structure

Theodore Steele, Tobias Baldauf

The bispectrum is the leading non-Gaussian statistic in Large-Scale Structure (LSS) clustering and encodes the interactions in the underlying field. It is thus an important diagnos…

astro-ph.CO2020

Projected two- and three-point statistics: Forecasts and mitigation of non-linear RSDs

Oliver Leicht, Tobias Baldauf, James Fergusson +1

The combination of two- and three-point clustering statistics of galaxies and the underlying matter distribution has the potential to break degeneracies between cosmological parame…

astro-ph.CO201954 cited

Primordial Non-Gaussianity

P. Daniel Meerburg, Daniel Green, Muntazir Abidi +175

Our current understanding of the Universe is established through the pristine measurements of structure in the cosmic microwave background (CMB) and the distribution and shapes of…