'Gemini south' diaporamas de présentation

Light Pollution in the ELT Context.

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Objectives

Objectives. How should Gemini respond in terms of scientific effectiveness to the the current competition from Subaru, ESO and perhaps even Keck? What does the Gemini Science Staff want to see discussed and proposed at Aspen 2003 What is our vision of the Future?.

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NOAO Gemini Science Center (NGSC)

503 views • 37 slides

Australian Astronomy MNRF Symposium

Gemini Local Activities and International Developments. Warrick Couch, UNSW no longer the Australian Gemini Scientist, - not quite yet the Australian Gemini Board member. Australian Astronomy MNRF Symposium. ATNF Marsfield, 7 June 2005. Talk outline. Local Activities AusGO news

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Gemini Observatory Report to the AURA Board 6 th February 2002

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The Gemini Observatory: An Application of High-Performance Networks Tools in Modern Astronomy

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Star formation under extreme conditions: the Galactic center

Revelation of a vast amount of warm (~ 250 K) and diffuse (? 100 cm -3 ) gas and high ionization rate ( ? > 10 -15 s -1 ) in the Central Molecular Zone by the Infrared Spectrum of H 3 + Takeshi Oka Department of Astronomy and Astrophysics and Department of Chemistry

279 views • 21 slides

H 3 + in the Central Molecular Zone of the Galactic Center: Revelation of a New Category of Gas

H 3 + in the Central Molecular Zone of the Galactic Center: Revelation of a New Category of Gas. Takeshi Oka. Department of Astronomy and Astrophysics and Department of Chemistry, The Enrico Fermi Institute, University of Chicago. Tom Geballe Gemini Observatory.

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NOAO Gemini Science Center (NGSC)

302 views • 19 slides

Project Overview

The Gemini Observatory. Project Overview. NSF Grant Proposal Gemini South/AmPATH Connection to Internet2. Project Goal. Establish a high-speed connection from the La Serena base station, Chile, to US National Research Networks (NRNs) and non-US NRNs.

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Gemini Observatory

433 views • 18 slides

Revelation of a vast amount of warm and diffuse gas and high ionization rate

Revelation of a vast amount of warm and diffuse gas and high ionization rate in the Central Molecular Zone of the Galactic center by the Infrared Spectrum of H 3 + Takeshi Oka Department of Astronomy and Astrophysics and Department of Chemistry

265 views • 17 slides

H 3 + , the new probe for ionization rate ?

7. H 3 + , the new probe for ionization rate ?. the cosmic ray. Takeshi Oka Department of Astronomy and Astrophysics and Department of Chemistry The Enrico Fermi Institute, University of Chicago. Tom Geballe Gemini Observatory Nick Indriolo, Ben McCall

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165 views • 1 slides