Jon Willis | Introduction | September 25th and 29th |
Sara Ellison | Galaxies probed through quasar absorption lines | October 2nd and 6th |
Luc Simard | The formation and evolution of galaxy discs | October 9th and 16th |
David Schade | Galaxy populations in clusters: part 1, part 2, part 3 | October 20th and 23rd |
Chris Willott | Reionization | October 27th and 30th |
Thomas Puzia | Stellar populations, chemical enrichment and galaxy formation: part1, part 2 | November 3rd and 6th |
John Blakeslee | Structure and motions in the nearby universe | Novermber 13th and 17th |
Chris Pritchet | Supernova cosmology: part 1, part 2, part 3, part 4 | November 20th and 24th |
Sara Ellison | Are surveys for damped
Lyman alpha systems biased by dust? |
Luc Simard | What observational properties of galaxy discs tell us that they reside in dark matter haloes? |
David Schade | Nature versus nurture:
are the observed properties of cluster galaxy populations
determined by initial conditions, the effect of the cluster environment, or a combination of the two? |
Chris Willott | Is it possible that AGN provided the dominant source of photons that re-ionized the Universe? |
Thomas Puzia | Can the Milky Way be assembled from dwarf galaxies? |
John Blakeslee | Click here |
Chris Pritchet | Click here |