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Large-Aperture Mirror Array (LAMA): conceptual design for a distributed-aperture 42-meter telescope. Hickson, Paul
Abstract
We propose a high-density coherent array of eighteen 10-meter liquid-mirror telescopes. Each telescope is equipped with a
reflective corrector system that enables it to point and track within an eight-degree diameter accessible field of view
centered on the zenith. Equipped with adaptive optics, each telescope would deliver a diffraction-limited beam to a common
focal plane. There, a dichroic optical-infrared camera will provide simultaneous imaging in six wavelength bands from 0.6 to 2.2 um.
Operating coherently as a Fizeau imaging interferometer, the array would be capable of achieving 4 mas resolution at 1 um and
a point source sensitivity of 40 pJy (IAB = 34.9) in a single 30 min exposure. With incoherent beam recombination it would be
capable of 25 mas resolution and a point-source detection limit of 250 pJy (IAB = 32.9) in a single 30 min exposure. The telescope
uses proven technologies and could be built in a comparatively-short time.
Copyright 2003 Society of Photo-Optical Instrumentation Engineers.
One print or electronic copy may be made for personal use only. Systematic reproduction and distribution,
duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited.
Item Metadata
| Title |
Large-Aperture Mirror Array (LAMA): conceptual design for a distributed-aperture 42-meter telescope.
|
| Creator | |
| Publisher |
Society of Photo-Optical Instrumentation Engineers (SPIE)
|
| Date Issued |
2003
|
| Description |
We propose a high-density coherent array of eighteen 10-meter liquid-mirror telescopes. Each telescope is equipped with a
reflective corrector system that enables it to point and track within an eight-degree diameter accessible field of view
centered on the zenith. Equipped with adaptive optics, each telescope would deliver a diffraction-limited beam to a common
focal plane. There, a dichroic optical-infrared camera will provide simultaneous imaging in six wavelength bands from 0.6 to 2.2 um.
Operating coherently as a Fizeau imaging interferometer, the array would be capable of achieving 4 mas resolution at 1 um and
a point source sensitivity of 40 pJy (IAB = 34.9) in a single 30 min exposure. With incoherent beam recombination it would be
capable of 25 mas resolution and a point-source detection limit of 250 pJy (IAB = 32.9) in a single 30 min exposure. The telescope
uses proven technologies and could be built in a comparatively-short time.
Copyright 2003 Society of Photo-Optical Instrumentation Engineers.
One print or electronic copy may be made for personal use only. Systematic reproduction and distribution,
duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited.
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| Genre | |
| Type | |
| Language |
eng
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| Date Available |
2011-09-20
|
| Provider |
Vancouver : University of British Columbia Library
|
| Rights |
Attribution-NonCommercial-NoDerivatives 4.0 International
|
| DOI |
10.14288/1.0107614
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| URI | |
| Affiliation | |
| Citation |
Hickson, Paul; Lanzetta, Kenneth M. Large-Aperture Mirror Array (LAMA): conceptual design for a distributed-aperture 42-meter telescope. Future Giant Telescopes, edited by J. Roger P. Angel, Roberto Gilmozzi. Proceedings of SPIE Volume 4840, 273, 2003.
|
| Publisher DOI |
10.1117/12.459075
|
| Peer Review Status |
Reviewed
|
| Scholarly Level |
Faculty
|
| Copyright Holder |
Hickson, Paul
|
| Rights URI | |
| Aggregated Source Repository |
DSpace
|
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Item Citations and Data
Rights
Attribution-NonCommercial-NoDerivatives 4.0 International