activity
20042023
most citedNew Constraints on Cosmic Reionization from the 2012 Hubble Ultra Deep Field Campaign

559 citations · 17.3k across the 183 of their papers we have counts for

collaborators
Showing 2010 · astro-ph.COShow all

5 papers · 2 filters

astro-ph.CO2010★ 19 cited

Star formation trends in high-redshift galaxy surveys: the elephant or the tail?

Martin Stringer, Shaun Cole, Carlos S. Frenk +1

Star formation rate and accummulated stellar mass are two fundamental physical quantities that describe the evolutionary state of a forming galaxy. Two recent attempts to determine…

astro-ph.CO2010★ 347 cited

Early star-forming galaxies and the reionization of the Universe

Brant E. Robertson, Richard S. Ellis, James S. Dunlop +2

Star forming galaxies represent a valuable tracer of cosmic history. Recent observational progress with Hubble Space Telescope has led to the discovery and study of the earliest-kn…

astro-ph.CO2010★ 126 cited

The Emission Line Properties of Gravitationally-lensed 1.5 < z < 5 Galaxies

Johan Richard, Tucker Jones, Richard S. Ellis +3

We present and analyse near-infrared spectroscopy for a sample of 28 gravitationally- lensed star-forming galaxies in the redshift range 1.5 < z < 5, observed mostly with the Keck…

astro-ph.CO2010★ 265 cited

Keck Spectroscopy of Faint 3<z<7 Lyman Break Galaxies:- II. A High Fraction of Line Emitters at Redshift Six

Daniel P. Stark, Richard S. Ellis, Masami Ouchi

As Lyman-alpha photons are scattered by neutral hydrogen, a change with redshift in the Lyman-alpha equivalent width distribution of distant galaxies offers a promising probe of th…

astro-ph.CO2010★ 445 cited

Keck Spectroscopy of Faint 3<z<7 Lyman Break Galaxies: - I. New constraints on cosmic reionisation from the luminosity and redshift-dependent fraction of Lyman-alpha emission

Daniel P. Stark, Richard S. Ellis, Kuenley Chiu +2

We present results from a new Keck spectroscopic survey of UV-faint LBGs in the redshift range 3<z<7. Combined with earlier Keck and published ESO VLT data, our sample contains mor…