THIRD ANNUAL GMT COMMUNITY SCIENCE MEETING
Presented by the Giant Magellan Telescope Organization
Asilomar Conference Grounds
in Pacific Grove, CA
For the last 15 years, resolved stellar populations of nearby galaxies have rivaled distant galaxies in terms of their return on our understanding of both dark matter and galaxy formation.
The detailed dynamics, chemical and star formation histories of nearby objects provide a view that is complementary to the average history of the universe that can be stitched together from observing large ensembles of unresolved galaxies. In this conference, we will consider the questions “What can uniquely be learned about dark matter and the physics of galaxy formation from observations of resolved stellar populations?” and “How can we ensure that the next generation of facilities accomplishes this?” Through invited and contributed talks on state-of-the-art, near-field research on dark matter and galaxy formation and evolution, we aim to (i) pinpoint the highest priority open questions and (ii) foster new collaborative connections with an eye on answering these questions with next generation facilities.
Registration deadline: September 1, 2015. No registration fee is required. Travel support is provided for graduate students and post-doctoral researchers. Space is limited. A small number of contributed talks will be accepted. The talk sessions will be complemented by an extensive poster session. Abstracts will be requested via email once you register. Abstract submission deadline: July 1, 2015.
SCIENTIFIC ORGANIZING COMMITTEE
Charlie Conroy, CfA (co-chair)
Beth Willman, Haverford (co-chair)
Rebecca Bernstein, GMTO
Robert Blum, NOAO
Gary Da Costa, Australian National University
Anna Frebel, MIT
Ken Freeman, Australian National University
Jason Kalirai, STScI
Rich Kron, Chicago
Young-Wook Lee, Yonsei
Lucas Macri, Texas A&M
Josh Simon, Carnegie
Matthias Steinmetz, Potsdam
Risa Wechsler, Stanford
Dennis Zaritsky, Arizona
HEADER IMAGE ©2015 Yuri Beletsky (las campanas observatory)