The brightness of the night sky at an astronomical site is one of the principal factors that determine the quality of available optical observing time. At any site the optical night sky is always brightened with airglow, zodiacal light, integrated starlight, diffuse Galactic light and extra-galactic...
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ftciteseerx:oai:CiteSeerX.psu:10.1.1.147.7097 2023-05-15T14:04:16+02:00 Suzanne L. Kenyon Michael C. B. Ashley Jon Everett Jon S. Lawrence John W. V. Storey The Pennsylvania State University CiteSeerX Archives application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.147.7097 http://www.phys.unsw.edu.au/~mcba/pubs/kenyon06a.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.147.7097 http://www.phys.unsw.edu.au/~mcba/pubs/kenyon06a.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://www.phys.unsw.edu.au/~mcba/pubs/kenyon06a.pdf Site testing Antarctica sky brightness text ftciteseerx 2016-01-07T15:11:11Z The brightness of the night sky at an astronomical site is one of the principal factors that determine the quality of available optical observing time. At any site the optical night sky is always brightened with airglow, zodiacal light, integrated starlight, diffuse Galactic light and extra-galactic light. Further brightening can be caused by scattered sunlight, aurorae, moonlight and artificial sources. Dome C exhibits many characteristics that are extremely favourable to optical and IR astronomy; however, at this stage few measurements have been made of the brightness of the optical night sky. Nigel is a fibre-fed UV/visible grating spectrograph with a thermoelectrically cooled 256 × 1024 pixel CCD camera, and is designed to measure the twilight and night sky brightness at Dome C from 250 nm to 900 nm. We present details of the design, calibration and installation of Nigel in the AASTINO laboratory at Dome C, together with a summary of the known properties of the Dome C sky. Text Antarc* Antarctica Unknown Starlight ENVELOPE(64.483,64.483,-70.200,-70.200) |
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English |
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Site testing Antarctica sky brightness |
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Site testing Antarctica sky brightness Suzanne L. Kenyon Michael C. B. Ashley Jon Everett Jon S. Lawrence John W. V. Storey |
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Site testing Antarctica sky brightness |
description |
The brightness of the night sky at an astronomical site is one of the principal factors that determine the quality of available optical observing time. At any site the optical night sky is always brightened with airglow, zodiacal light, integrated starlight, diffuse Galactic light and extra-galactic light. Further brightening can be caused by scattered sunlight, aurorae, moonlight and artificial sources. Dome C exhibits many characteristics that are extremely favourable to optical and IR astronomy; however, at this stage few measurements have been made of the brightness of the optical night sky. Nigel is a fibre-fed UV/visible grating spectrograph with a thermoelectrically cooled 256 × 1024 pixel CCD camera, and is designed to measure the twilight and night sky brightness at Dome C from 250 nm to 900 nm. We present details of the design, calibration and installation of Nigel in the AASTINO laboratory at Dome C, together with a summary of the known properties of the Dome C sky. |
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The Pennsylvania State University CiteSeerX Archives |
format |
Text |
author |
Suzanne L. Kenyon Michael C. B. Ashley Jon Everett Jon S. Lawrence John W. V. Storey |
author_facet |
Suzanne L. Kenyon Michael C. B. Ashley Jon Everett Jon S. Lawrence John W. V. Storey |
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Suzanne L. Kenyon |
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http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.147.7097 http://www.phys.unsw.edu.au/~mcba/pubs/kenyon06a.pdf |
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ENVELOPE(64.483,64.483,-70.200,-70.200) |
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Starlight |
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Starlight |
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Antarc* Antarctica |
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Antarc* Antarctica |
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http://www.phys.unsw.edu.au/~mcba/pubs/kenyon06a.pdf |
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http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.147.7097 http://www.phys.unsw.edu.au/~mcba/pubs/kenyon06a.pdf |
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Metadata may be used without restrictions as long as the oai identifier remains attached to it. |
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