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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

Blind foreground subtraction for intensity mapping experiments

Monthly Notices of the Royal Astronomical Society 91探花 University Press 447:1 (2014) 400-416

Authors:

David Alonso, P Bull, Pedro Ferreira, Mg Santos

Abstract:

We make use of a large set of fast simulations of an intensity mapping experiment with characteristics similar to those expected of the Square Kilometre Array in order to study the viability and limits of blind foreground subtraction techniques. In particular, we consider three different approaches: polynomial fitting, principal component analysis (PCA) and independent component analysis (ICA). We review the motivations and algorithms for the three methods, and show that they can all be described, using the same mathematical framework, as different approaches to the blind source separation problem. We study the efficiency of foreground subtraction both in the angular and radial (frequency) directions, as well as the dependence of this efficiency on different instrumental and modelling parameters. For well-behaved foregrounds and instrumental effects, we find that foreground subtraction can be successful to a reasonable level on most scales of interest. We also quantify the effect that the cleaning has on the recovered signal and power spectra. Interestingly, we find that the three methods yield quantitatively similar results, with PCA and ICA being almost equivalent.

Homogeneity and isotropy in the 2MASS Photometric Redshift catalogue

(2014)

Authors:

David Alonso, Ana Isabel Salvador, Francisco Javier S谩nchez, Maciej Bilicki, Juan Garc铆a-Bellido, Eusebio S谩nchez

Cross-correlating 21cm intensity maps with Lyman Break Galaxies in the post-reionization era

(2014)

Authors:

Francisco Villaescusa-Navarro, Matteo Viel, David Alonso, Kanan K Datta, Philip Bull, Mario G Santos

Blind foreground subtraction for intensity mapping experiments

(2014)

Authors:

David Alonso, Philip Bull, Pedro G Ferreira, Mario G Santos

Fast simulations for intensity mapping experiments

Monthly Notices of the Royal Astronomical Society 91探花 University Press 444:4 (2014) 3183-3197

Authors:

David Alonso, Pedro Ferreira, MG Santos

Abstract:

We present a code to generate mock observations of 21 cm intensity mapping experiments. The emphasis of the code is on reducing the computational cost of running a full-blown simulation, trading computational time for accuracy. The code can be used to generate independent realizations of the cosmological signal and foregrounds, which are necessary, for instance, in order to obtain realistic forecasts for future intensity mapping experiments. The code is able to reproduce the correct angular and radial clustering pattern for the cosmological signal, including redshift-space distortions, lightcone evolution and bias. Furthermore, it is possible to simulate a variety of foregrounds, including the potentially problematic polarized synchrotron emission.

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