The High Redshift Universe: A Multi-Wavelength View
The goal of this conference is to bring together observers, theorists,
and simulators working on all aspects of the high redshift
universe. Planned topics include galaxy formation and evolution;
chemical and radiative feedback; cosmic reionization; current
observations of high-redshift galaxies at nearIR through radio
wavelengths; and 21-cm cosmology. The central theme will be the major
effect of feedback from early galaxies on the large-scale cosmic
environment at early times.
We received a very large number of applications by the October 31'st, 2009 deadline. Emails were sent on Nov. 23'rd notifying accepted applicants.
 
Please see the  program and speakers page for
information on the conference schedule and a full list
of speakers. 
Please see the  housing page for infomation
on housing options and prices, and instructions for housing
reservations and for paying for registration and the banquet. 
Please see the  travel and funding page for
information on traveling to aspen and other practical information
(registration reception, funding, computer facilities, recreation). 
Note that the opening reception has been moved to 18:30.
Please see the  participants page for a
full list of participants (names and emails).
 
 
For more information, contact:
 barkana@wise.tau.ac.il
Organizers: 
Judd Bowman , Caltech
Marc Kamionkowski , Caltech
Chris Carilli , NRAO
 
Scientific Organizing Committee:
Frank Briggs (ANU)
Richard Ellis (Caltech)
Paul Shapiro (Texas, Austin)
Rogier Windhorst (ASU)
Stuart Wyithe (Melbourne)
Naoki Yoshida (IPMU Tokyo)
Matias Zaldarriaga (IAS)
A PDF conference poster is available here.
Background: NASA, ESA, S. Beckwith (STScI) and the HUDF Team