activity
20062008
most citedThe angular correlations of galaxies in the COSMOS field

64 citations · 191 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph200818 cited

Topology of non-linear structure in the 2dF Galaxy Redshift Survey

J. Berian James, Matthew Colless, Geraint F. Lewis +1

We study the evolution of non-linear structure as a function of scale in samples from the 2dF Galaxy Redshift Survey, constituting over 221 000 galaxies at a median redshift of z=0…

astro-ph200712 cited

Coordinate Confusion in Conformal Cosmology

Geraint F. Lewis, Matthew J. Francis, Luke A. Barnes +1

A straight-forward interpretation of standard Friedmann-Lemaitre-Robertson-Walker (FLRW) cosmologies is that objects move apart due to the expansion of space, and that sufficiently…

astro-ph200724 cited

Expanding Space: the Root of all Evil?

Matthew J. Francis, Luke A. Barnes, J. Berian James +1

While it remains the staple of virtually all cosmological teaching, the concept of expanding space in explaining the increasing separation of galaxies has recently come under fire…

astro-ph200764 cited

The angular correlations of galaxies in the COSMOS field

H. J. McCracken, J. A. Peacock, L. Guzzo +21

We present measurements of the two-point galaxy angular correlation function w(θ) in the COSMOS field. Independent determinations of w(θ) as a function of magnitude limit are prese…

astro-ph20071 cited

Type Ia supernova diversity: Standardizing the candles

T. M. Davis, J. B. James, B. P. Schmidt +1

Future use of type Ia supernovae for cosmology aims not only to determine the equation of state of dark energy, but also to constrain possible variations in its value. To achieve t…

astro-ph200618 cited

Topology of large-scale structure in the 2dF Galaxy Redshift Survey

J. Berian James, Geraint F. Lewis, Matthew Colless

We investigate the topology of the completed 2dF Galaxy Redshift Survey, drawing two flux-limited samples of the local Universe from the 2dFGRS catalogue, which contains over 220,0…