activity
20102015
most citedBlind foreground subtraction for intensity mapping experiments

151 citations · 426 across the 10 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

7 papers · 1 filter

astro-ph.CO2015★ 7 cited

Model-independent constraints on dark energy and modified gravity with the SKA

Gong-Bo Zhao, David Bacon, Roy Maartens +2

Employing a nonparametric approach of the principal component analysis (PCA), we forecast the future constraint on the equation of state of dark energy, and on the effective…

astro-ph.CO2015★ 10 cited

Measuring redshift-space distortions with future SKA surveys

Alvise Raccanelli, Philip Bull, Stefano Camera +8

The peculiar motion of galaxies can be a particularly sensitive probe of gravitational collapse. As such, it can be used to measure the dynamics of dark matter and dark energy as w…

astro-ph.CO2014★ 81 cited

Einstein's legacy in galaxy surveys

Stefano Camera, Roy Maartens, Mario G. Santos

Non-Gaussianity in the primordial fluctuations that seeded structure formation produces a signal in the galaxy power spectrum on very large scales. This signal contains vital infor…

astro-ph.CO2014★ 86 cited

Cosmological performance of SKA HI galaxy surveys

S. Yahya, P. Bull, M. G. Santos +4

The Square Kilometre Array (SKA) will conduct the biggest spectroscopic galaxy survey ever, by detecting the 21cm emission line of neutral hydrogen (HI) from around a billion galax…

astro-ph.CO2014★ 151 cited

Blind foreground subtraction for intensity mapping experiments

David Alonso, Philip Bull, Pedro G. Ferreira +1

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 (SKA) in order to stu…

astro-ph.CO2014★ 75 cited

Fast simulations for intensity mapping experiments

David Alonso, Pedro G. Ferreira, Mario G. Santos

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 simul…