| HAL: in2p3-00740937, version 1 |
| DOI: 10.1117/12.927257 |
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| Proceedings of the Society of Photo-Optical Instrumentation Engineers 8444 (2012) 84445E |
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| 2.5@C - An Off-Axis Telescope Concept for Antarctic Astronomy |
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| G. Moretto1Nicolas Epchtein2Maud Langlois3Isabelle Vauglin |
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| (2012-09-01) |
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| The Antarctic plateau offers exceptional atmospheric and environmental conditions for astronomical observations over a wide range of wavelengths and uniquely favorable to infrared astronomy. Exceptional low sky brightness throughout the near- and mid-infrared and a telescope facility complying with the highest possible dynamic range for photometry, angular resolution and the wide-field leads to the possibility of a modest-sized 2m off-axis telescope achieving comparable sensitivity to that of a larger ground-based 8-10m class telescope or a same sized space-based ones. |
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| 1: | IPNL - Institut de Physique Nucléaire de Lyon |
| 2: | LAGRANGE - Joseph Louis LAGRANGE |
| 3: | CRAL - Centre de Recherche Astrophysique de Lyon |
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| Subject(s) | : | Physics/Astrophysics/Instrumentation and Methods for Astrophysic Sciences of the Universe/Astrophysics/Instrumentation and Methods for Astrophysic |
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| infrared cases for Antarctica – off-axis telescope – low scattered light – low emissivity |
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| Attached file list to this document: | |||||
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| in2p3-00740937, version 1 | |
| http://hal.in2p3.fr/in2p3-00740937 | |
| oai:hal.in2p3.fr:in2p3-00740937 | |
| From: Gil Moretto | |
| Submitted on: Thursday, 11 October 2012 13:44:07 | |
| Updated on: Monday, 28 January 2013 09:30:15 | |