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19972008
most citedLiving in a Void: Testing the Copernican Principle with Distant Supernovae

143 citations · 423 across the 11 of their papers we have counts for

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26 papers · 1 filter

astro-ph200876 cited

Eddington-Born-Infeld gravity and the large scale structure of the Universe

Máximo Bañados, Pedro G. Ferreira, Constantinos Skordis

It has been argued that a Universe governed by Eddington-Born-Infeld gravity can be compatible with current cosmological constraints. The extra fields introduced in this theory can…

astro-ph200830 cited

Map-making in small field modulated CMB polarisation experiments: approximating the maximum-likelihood method

D. Sutton, B. R. Johnson, M. L. Brown +3

Map-making presents a significant computational challenge to the next generation of kilopixel CMB polarisation experiments. Years worth of time ordered data (TOD) from thousands of…

astro-ph2008143 cited

Living in a Void: Testing the Copernican Principle with Distant Supernovae

Timothy Clifton, Pedro G. Ferreira, Kate Land

A fundamental presupposition of modern cosmology is the Copernican Principle; that we are not in a central, or otherwise special region of the Universe. Studies of Type Ia supernov…

astro-ph20084 cited

Detecting the B-mode Polarisation of the CMB with Clover

C. E. North, B. R. Johnson, P. A. R. Ade +41

We describe the objectives, design and predicted performance of Clover, which is a ground-based experiment to measure the faint ``B-mode'' polarisation pattern in the cosmic microw…

astro-ph200816 cited

Dark Matter, Modified Gravity and the Mass of the Neutrino

P. G Ferreira, C. Skordis, C. Zunckel

It has been suggested that Einstein's theory of General Relativity can be modified to accomodate mismatches between the gravitational field and luminous matter on a wide range of s…

astro-ph200824 cited

Constraining primordial magnetic fields with CMB polarization experiments

Jostein R. Kristiansen, Pedro G. Ferreira

We calculate the effect that a primordial homogeneous magnetic field, $\B_0$, will have on the different CMB power spectra due to Faraday rotation. Concentrating on the ,