activity
20062026
most citedANTARES: the first undersea neutrino telescope

629 citations · 4.6k across the 75 of their papers we have counts for

collaborators
Showing 2016Show all

8 papers · 1 filter

astro-ph.CO2016★ 65 cited

Halo bias in Lagrangian Space: Estimators and theoretical predictions

Chirag Modi, Emanuele Castorina, Uros Seljak

We present several methods to accurately estimate Lagrangian bias parameters and substantiate them using simulations. In particular, we focus on the quadratic terms, both the local…

astro-ph.CO2016★ 26 cited

Excursion set peaks: the role of shear

Emanuele Castorina, Aseem Paranjape, Oliver Hahn +1

Recent analytical work on the modelling of dark halo abundances and clustering has demonstrated the advantages of combining the excursion set approach with peaks theory. We extend…

astro-ph.CO2016★ 13 cited

Constraints on halo formation from cross-correlations with correlated variables

Emanuele Castorina, Aseem Paranjape, Ravi K. Sheth

Cross-correlations between biased tracers and the dark matter field encode information about the physical variables which characterize these tracers. However, if the physical varia…

astro-ph.CO2016★ 25 cited

Simulating cosmologies beyond CDM with PINOCCHIO

Luca Alberto Rizzo, Francisco Villaescusa-Navarro, Pierluigi Monaco +4

We present a method that extends the capabilities of the PINpointing Orbit-Crossing Collapsed HIerarchical Objects (PINOCCHIO) code, allowing it to generate accurate dark matter ha…

astro-ph.CO2016★ 24 cited

Baryon Acoustic Oscillations reconstruction with pixels

Andrej Obuljen, Francisco Villaescusa-Navarro, Emanuele Castorina +1

Gravitational non-linear evolution induces a shift in the position of the baryon acoustic oscillations (BAO) peak together with a damping and broadening of its shape that bias and…

astro-ph.CO2016★ 77 cited

On the spatial distribution of neutral hydrogen in the Universe: bias and shot-noise of the HI Power Spectrum

Emanuele Castorina, Francisco Villaescusa-Navarro

The spatial distribution of neutral hydrogen (HI) in the Universe contains a wealth of cosmological information. The 21 cm emission line can be used to map the HI up to very high r…