activity
20152026
most citedBeyond LIMD bias: a measurement of the complete set of third-order halo bias parameters

81 citations · 363 across the 10 of their papers we have counts for

collaborators

12 papers

astro-ph.GA2026

Constraining the density distribution of the cold Circumgalactic Medium of quasars at z>2 through Lya, HeII and Ha emission

Andrea Travascio, Sebastiano Cantalupo, Titouan Lazeyras +16

Extended Lya emission is routinely detected around high-redshift quasars, revealing large reservoirs of cool circumgalactic medium (CGM). Its resonant nature complicates interpreta…

astro-ph.GA2026

Resolving the physics of Quasar Ly Nebulae (RePhyNe): II. The dense and clumpy CGM of Quasars at 3.5

Titouan Lazeyras, Sebastiano Cantalupo, Andrea Travascio +10

The small scale density distribution of the cold circumgalactic medium (CGM) plays a central role in galaxy evolution, yet it is still poorly understood. We provide new constraints…

astro-ph.CO2022★ 39 cited

Assembly bias in the local PNG halo bias and its implication for constraints

Titouan Lazeyras, Alexandre Barreira, Fabian Schmidt +1

We use -body simulations to study halo assembly bias (i.e., the dependence of halo clustering on properties beyond total mass) in the density and primordial non-Gaussianity (PNG…

astro-ph.CO2021

Cosmic voids and BAO with relative baryon-CDM perturbations

Hasti Khoraminezhad, Pauline Vielzeuf, Titouan Lazeyras +2

We study the statistics of various large-scale structure tracers in gravity-only cosmological simulations including baryons and cold dark matter (CDM) initialized with two differen…

astro-ph.CO2021★ 2 cited

Assembly bias in quadratic bias parameters of dark matter halos from forward modeling

Titouan Lazeyras, Alexandre Barreira, Fabian Schmidt

We use the forward modeling approach to galaxy clustering combined with the likelihood from the effective-field theory of large-scale structure to measure assembly bias, i.e. the d…

astro-ph.CO2021★ 57 cited

Galaxy bias from forward models: linear and second-order bias of IllustrisTNG galaxies

Alexandre Barreira, Titouan Lazeyras, Fabian Schmidt

We use field-level forward models of galaxy clustering and the EFT likelihood formalism to study, for the first time for self-consistently simulated galaxies, the relations between…

astro-ph.CO2020★ 9 cited

Quantifying the impact of baryon-CDM perturbations on halo clustering and baryon fraction

Hasti Khoraminezhad, Titouan Lazeyras, Raul E. Angulo +2

Baryons and cold dark matter (CDM) did not comove prior to recombination. This leads to differences in the local baryon and CDM densities, the so-called baryon-CDM isocurvature per…

astro-ph.CO2020★ 11 cited

The impact of massive neutrinos on halo assembly bias

Titouan Lazeyras, Francisco Villaescusa-Navarro, Matteo Viel

Using the publicly available Quijote simulations, we present the first measurements of the assembly bias of dark matter halos in N-body simulations which include massive neutrinos.…

astro-ph.CO2017★ 81 cited

Beyond LIMD bias: a measurement of the complete set of third-order halo bias parameters

Titouan Lazeyras, Fabian Schmidt

We present direct measurements of cubic bias parameters of dark matter halos from the halo-matter-matter-matter trispectrum. We measure this statistic efficiently by cross-correlat…

astro-ph.CO2016★ 66 cited

Large-scale assembly bias of dark matter halos

Titouan Lazeyras, Marcello Musso, Fabian Schmidt

We present precise measurements of the assembly bias of dark matter halos, i.e. the dependence of halo bias on other properties than the mass, using curved "separate universe" N-bo…

astro-ph.CO2016★ 68 cited

Verifying the consistency relation for the scale-dependent bias from local primordial non-Gaussianity

Matteo Biagetti, Titouan Lazeyras, Tobias Baldauf +2

We measure the large-scale bias of dark matter halos in simulations with non-Gaussian initial conditions of the local type, and compare this bias to the response of the mass functi…

astro-ph.CO2015★ 30 cited

Lagrangian bias of generic large-scale structure tracers

Titouan Lazeyras, Marcello Musso, Vincent Desjacques

The dark matter halos that host galaxies and clusters form out of initial high-density patches, providing a biased tracer of the linear matter density field. In the simplest local…