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91探花
Black Hole

Lensing of space time around a black hole. At 91探花 we study black holes observationally and theoretically on all size and time scales - it is some of our core work.

Credit: ALAIN RIAZUELO, IAP/UPMC/CNRS. CLICK HERE TO VIEW MORE IMAGES.

Prof. David Alonso

Associate Professor of Cosmology

Sub department

  • Astrophysics

Research groups

  • Beecroft Institute for Particle Astrophysics and Cosmology
  • Rubin-LSST
David.Alonso@physics.ox.ac.uk
Telephone: 01865 (2)288582
Denys Wilkinson Building, room 532B
  • About
  • Publications

Detecting the anisotropic astrophysical gravitational wave background in the presence of shot noise through cross-correlations

PHYSICAL REVIEW D 102:2 (2020) 23002

Authors:

David Alonso, Giulia Cusin, Pedro G Ferreira, Cyril Pitrou

Noise angular power spectrum of gravitational wave background experiments

PHYSICAL REVIEW D 101:12 (2020) ARTN 124048

Authors:

David Alonso, Carlo R Contaldi, Giulia Cusin, Pedro G Ferreira, Arianna I Renzini

The $N_\ell$ of gravitational wave background experiments

(2020)

Authors:

David Alonso, Carlo R Contaldi, Giulia Cusin, Pedro G Ferreira, Arianna I Renzini

Detecting ultra-high energy cosmic ray anisotropies through cross-correlations

(2020)

Authors:

Federico R Urban, Stefano Camera, David Alonso

LYACOLORE: synthetic datasets for current and future Lyman-alpha forest BAO surveys

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS 2020:3 (2020) 68

Authors:

James Farr, Andreu Font-Ribera, Helion du Mas des Bourboux, Andrea Munoz-Gutierrez, F Javier Sanchez, Andrew Pontzen, Alma Xochitl Gonzalez-Morales, David Alonso, David Brooks, Peter Doel, Thomas Etourneau, Julien Guy, Jean-Marc Le Goff, Axel de la Macorra, Nathalie Palanque-Delabrouille, Ignasi Perez-Rafols, James Rich, ArCie Slosar, Gregory Tarle, Duan Yutong, Kai Zhang

Abstract:

© 2020 IOP Publishing Ltd and Sissa Medialab. The statistical power of Lyman-α forest Baryon Acoustic Oscillation (BAO) measurements is set to increase significantly in the coming years as new instruments such as the Dark Energy Spectroscopic Instrument deliver progressively more constraining data. Generating mock datasets for such measurements will be important for validating analysis pipelines and evaluating the effects of systematics. With such studies in mind, we present LyaCoLoRe: A package for producing synthetic Lyman-α forest survey datasets for BAO analyses. LyaCoLoRe transforms initial Gaussian random field skewers into skewers of transmitted flux fraction via a number of fast approximations. In this work we explain the methods of producing mock datasets used in LyaCoLoRe, and then measure correlation functions on a suite of realisations of such data. We demonstrate that we are able to recover the correct BAO signal, as well as large-scale bias parameters similar to literature values. Finally, we briefly describe methods to add further astrophysical effects to our skewers-high column density systems and metal absorbers-which act as potential complications for BAO analyses.

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