Science drivers and requirements for an Advanced Technology Large Aperture Space Telescope (ATLAST): Implications for technology development and synergies with other future facilities
Autor: | Marc Postman, Mauro Giavalisco, R. Michael Rich, Thomas M. Brown, William R. Oegerle, Wesley A. Traub, H. Phillip Stahl, Kenneth R. Sembach, Daniela Calzetti, Matt Mountain, Jason Tumlinson, Karl R. Stapelfeldt, Tupper Hyde, Rémi Soummer |
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Jazyk: | angličtina |
Rok vydání: | 2010 |
Předmět: |
Diffraction
Wavefront Earth and Planetary Astrophysics (astro-ph.EP) Cosmology and Nongalactic Astrophysics (astro-ph.CO) Computer science FOS: Physical sciences Large aperture Technology development Astrophysics - Astrophysics of Galaxies Space exploration Space observatory Spitzer Space Telescope Astrophysics - Solar and Stellar Astrophysics Astrophysics of Galaxies (astro-ph.GA) Systems engineering Angular resolution Sensitivity (control systems) Astrophysics - Instrumentation and Methods for Astrophysics Instrumentation and Methods for Astrophysics (astro-ph.IM) Solar and Stellar Astrophysics (astro-ph.SR) Astrophysics - Cosmology and Nongalactic Astrophysics Astrophysics - Earth and Planetary Astrophysics |
Popis: | The Advanced Technology Large-Aperture Space Telescope (ATLAST) is a concept for an 8-meter to 16-meter UVOIR space observatory for launch in the 2025-2030 era. ATLAST will allow astronomers to answer fundamental questions at the forefront of modern astronphysics, including "Is there life elsewhere in the Galaxy?" We present a range of science drivers that define the main performance requirements for ATLAST (8 to 16 milliarcsec angular resolution, diffraction limited imaging at 0.5 {\mu}m wavelength, minimum collecting area of 45 square meters, high sensitivity to light wavelengths from 0.1 {\mu}m to 2.4 {\mu}m, high stability in wavefront sensing and control). We will also discuss the synergy between ATLAST and other anticipated future facilities (e.g., TMT, EELT, ALMA) and the priorities for technology development that will enable the construction for a cost that is comparable to current generation observatory-class space missions. Comment: 12 pages, 4 figures, to appear in "Space Telescopes and Instrumentation 2010: Optical, Infrared, and Millimeter Wave," edited by Jacobus M. Oschmann Jr., Mark C. Clampin, Howard A. MacEwen, Proc. of SPIE, Vol. 7731, 77312K |
Databáze: | OpenAIRE |
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