AGN / Starbursts in the very dusty systems in Bootes
Are galaxies still evolving strongly? Christopher J. Miller
Star Formation in High Redshift Submillimeter Galaxies and QSO Hosts
NIR interferometry of the Seyfert galaxy NGC 1068: present interferometric NIR results and future goals G. Weigelt T. Beckert M. Wittkowski.
Planets in other Galaxies. Most planets we know of are within 0.5 kpc of the sun but our galaxy has a radius > 25 kpc.
T. J. Cox Gurtina Besla (CfA), Tiziana Di Matteo (CMU), Suvendra Dutta (CfA), Loren Hoffman (CfA), Patrik Jonsson (UCSC), Dusan Keres (CfA), Elisabeth.
Star formation and Feedback at z>1 Alice Shapley (UCLA) Collaborators: (UCLA) Daniel Nestor, Robin Mostardi, Kathy Kornei, Kristin Kulas, Kevin Hainline,
Molecular Line Studies and Chemistry in Interacting and Starburst Galaxies Susanne Aalto Department of Radio and Space Science With Onsala Space Observatory.
Are galaxies still evolving strongly? Christopher J. Miller Hubble Heritage Image.
Andrii Elyiv and XMM-LSS collaboration The correlation function analysis of AGN in the XMM-LSS survey.
The Size, Structure & Ionization of the Broad-Line Region in NGC 3227 and NGC 4051
Spatial properties of AGN in hierarchical models