activity
20102025
most citedBeyond BAO: improving cosmological constraints from BOSS with measurement of the void-galaxy cross-correlation

126 citations · 549 across the 33 of their papers we have counts for

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Showing 2019Show all

7 papers · 1 filter

astro-ph.CO2019★ 17 cited

Marked correlation functions in perturbation theory

Alejandro Aviles, Kazuya Koyama, Jorge L. Cervantes-Cota +2

We develop perturbation theory approaches to model the marked correlation function constructed to up-weight low density regions of the Universe, which might help distinguish modifi…

astro-ph.CO2019

Collapse of spherical overdensities in superfluid models of dark matter

S. T. H. Hartman, H. A. Winther, D. F. Mota

We intend to understand cosmological structure formation within the framework of superfluid models of dark matter with finite temperatures. Of particular interest is the evolution…

astro-ph.CO2019

Hybrid : general, unified, non-linear matter power spectrum in redshift space

Benjamin Bose, Hans A. Winther, Alkistis Pourtsidou +4

Constraints on gravity and cosmology will greatly benefit from performing joint clustering and weak lensing analyses on large-scale structure data sets. Utilising non-linear inform…

physics.comp-ph2019

SCALAR: an AMR code to simulate axion-like dark matter models

Mattia Mina, David F. Mota, Hans A. Winther

We present a new code, SCALAR, based on the high-resolution hydrodynamics and N-body code RAMSES, to solve the Schrödinger equation on adaptive refined meshes. The code is intended…

astro-ph.CO2019★ 126 cited

Beyond BAO: improving cosmological constraints from BOSS with measurement of the void-galaxy cross-correlation

Seshadri Nadathur, Paul M. Carter, Will J. Percival +2

We present a measurement of the anisotropic void-galaxy cross-correlation function in the CMASS galaxy sample of the BOSS DR12 data release. We perform a joint fit to the data for…

astro-ph.CO2019

Emulators for the non-linear matter power spectrum beyond CDM

Hans Winther, Santiago Casas, Marco Baldi +4

Accurate predictions for the non-linear matter power spectrum are needed to confront theory with observations in current and near future weak lensing and galaxy clustering surveys.…