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Giant Segmented Mirror Telescope Science Working Group February, 2004 |
The fifth Science Working Group meeting was held in Honolulu, Hawaii at the Institute for Astronomy on February 12-13, 2004. The meeting was held in the Fern Room of the Institute for Astronomy.
Major Action Items from the meeting are:
Preparation of 2 page summaries of the JWST/GSMT comparisons presented in Honolulu. To meet our goals of (1) discussing the material with our JWST counterparts and (2) having a draft white paper to discuss in May, with input received by March 15. The presenters (Herter; Barton; Najita; Olsen, Strom) are responsible; other SWG members are asked to support the effort by providing critical feedback.
Presentations:
Giant Magellan Telescope Project
Science with the Magellan Telescope
Stellar Populations with GSMT and JWST
Origin and Evolution of Galaxies: GSMT and JWST
Origin of Stellar and Sub-Stellar Mass Objects
Advancing GSMT SWG Recommendations: AURA's Proposal to the NSF
Understanding the Youngest Protostars
Frontier Science Enabled by a Giant Segmented Mirror Telescope
Exosolar Giant Planet Science GSMT vs. JWST (pdf file)
Exosolar Giant Planet Science GSMT vs. JWST (ppt file)
Holly Novack / hnovack@noao.edu / February 19, 2004