activity
19992008
most citedNew Hubble Space Telescope Discoveries of Type Ia Supernovae at z > 1: Narrowing Constraints on the Early Behavior of Dark Energy

1.8k citations · 2k across the 11 of their papers we have counts for

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Showing 2003 · astro-phShow all

6 papers · 2 filters

astro-ph2003

Radio Properties of EROs in the Phoenix Deep Survey

J. Afonso, A. M. Hopkins, M. Sullivan +3

Insensitive to dust obscuration, radio wavelengths are ideal to study star-forming galaxies free of dust induced biases. Using data from the Phoenix Deep Survey, we have identified…

astro-ph2003

The Phoenix Deep Survey: Evolution of Star Forming Galaxies

A. M. Hopkins, J. Afonso, A. Georgakakis +3

The Phoenix Deep Survey (PDS) is a multiwavelength survey based on deep 1.4 GHz radio observations used to identify a large sample of star forming galaxies to z=1. Photometric reds…

astro-ph2003

The relation between galactic properties and cluster structure

Bianca M. Poggianti, Terry J. Bridges, M. Yagi +5

A satisfactory understanding of the origin of the dependence of galaxy properties on their environment has remained, so far, out of reach. In the light of numerous observational re…

astro-ph2003

Two formation paths for cluster dwarf galaxies?

Bianca M. Poggianti, Nobunari Kashikawa, Terry Bridges +5

A surprising result of our recent spectroscopic survey of galaxies in the Coma cluster has been the discovery of a possible bimodal distribution in the metallicities of faint galax…

astro-ph2003

Extremely red galaxies in the Phoenix Deep Survey

A. M. Hopkins, J. Afonso, A. Georgakakis +3

The Phoenix Deep Survey (PDS) is a multiwavelength survey based on deep 1.4 GHz radio observations used to identify a large sample of star forming galaxies to z=1. Here we present…

astro-ph200316 cited

A search for the optical and near-infrared counterpart of the accreting millisecond X-ray pulsar XTE J1751-305

P. G. Jonker, G. Nelemans, Z. Wang +14

We have obtained optical and near-infrared images of the field of the accreting millisecond X-ray pulsar XTE J1751-305. There are no stars in the 0.7'' error circle (0.7'' is the o…