Photometry of a Sodium Laser Guide Star at the Starfire Optical Range
Measurements of a laser‐pumped sodium guide star produced over the Starfire Optical Range in 2002 November show that the brightness of the spot produced by 11.5 W of linearly polarized power on the sky was equivalent to a \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{a...
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Published in | Publications of the Astronomical Society of the Pacific Vol. 116; no. 817; pp. 278 - 289 |
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Main Authors | , , , , |
Format | Journal Article |
Language | English |
Published |
The University of Chicago Press
01.03.2004
01.03.2004 |
Subjects | |
Online Access | Get full text |
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Summary: | Measurements of a laser‐pumped sodium guide star produced over the Starfire Optical Range in 2002 November show that the brightness of the spot produced by 11.5 W of linearly polarized power on the sky was equivalent to a
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mag star. However, taking into account that the transmission through aVfilter is only 55% at the wavelength of sodium, its corrected magnitude,
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, was 7.4, or 800 photons s−1cm−2at the top of the telescope. In 2003 March, tests with linearly and then circularly polarized beams out of the telescope showed that a circularly polarized beam from 12 W of power out of the telescope produced a spot with
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(1015 photons s−1cm−2at the top of the telescope), 0.7 mag brighter than a linearly polarized beam from 11.1 W of power out of the telescope. Over the 4 nights of experiments over two seasons, the apparent 2σ width of the spot varied between 3
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6 and 4
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6, or 1.6 and 2.0 m at 92 km altitude, and its length through the sodium layer was 4.6–8.5 km, but no variation of spot size with power on the sky was seen. |
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ISSN: | 0004-6280 1538-3873 |
DOI: | 10.1086/382756 |