MSU 高加索山天文台天空的近红外亮度

IF 1.1 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
A. M. Tatarnikov, S. G. Zheltoukhov, G. E. Nikishev, A. N. Tarasenkov, A. V. Sharonova
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引用次数: 0

摘要

摘要 分析了2016-2023年在莫斯科国立大学高加索山天文台进行的近红外波段(J、H、K波段)本底亮度测量结果。结果表明,与望远镜热辐射有关的仪器背景只在\(K\)波段明显,在工作温度下,它的贡献主要决定了该波段的整体背景水平。文中给出了考虑到仪器和大气层外背景贡献的多项式系数。结果表明,天空背景亮度并不依赖于空气温度,但观测到了与水汽含量的微弱依赖关系,接近于模型计算的预期:在(J)和(H)波段,背景亮度以(大约 {\kern 1pt} 1\% {\text{/}}1 )毫米的速率下降,而在(K)波段,它以(大约 {\kern 1pt} 2.5% {text{/}1)毫米。据估计,本底亮度变化在短时间内的最大振幅为(30)分钟:\在(J)和(K)波段大约为10%,在(H)波段大约为30%。大气中散射的月球辐射对总体本底水平的最大贡献已经确定。结果表明,即使在满月期间,在与月球的角距离大于 \( \sim {\kern 1pt} 10^\circ\) 时,这一贡献也可以忽略不计。计算了 J、H 和 (K)波段的平均背景表面亮度 mag/arcsec2:\({{m}_{J}} = 15.7\), \({{m}_{H}} = 13.9\), and\({{m}_{K}} = 13.1\).
本文章由计算机程序翻译,如有差异,请以英文原文为准。

The Brightness of the Sky of the Caucasian Mountain Observatory of MSU in the Near Infrared

The Brightness of the Sky of the Caucasian Mountain Observatory of MSU in the Near Infrared

The Brightness of the Sky of the Caucasian Mountain Observatory of MSU in the Near Infrared

The results of measurements of background brightness in the near-infrared range (J, H, K bands), carried out in 2016–2023 at the Caucasus Mountain Observatory of Moscow State University was analyzed. It is shown that the instrumental background associated with the thermal radiation of the telescope is noticeable only in the \(K\) band, and at operating temperatures its contribution mainly determines the level of the overall background in this band. The coefficients of a polynomial taking into account the contribution of instrumental and extra-atmospheric backgrounds are presented. It is shown that the brightness of the sky background does not depend on air temperature, but a weak dependence on the water vapor content is observed, close to that expected from model calculations: in the \(J\) and \(H\) bands, the background brightness decreases at a rate of \( \approx {\kern 1pt} 1\% {\text{/}}1\) mm, and in the \(K\) band it grows at a rate of \( \approx {\kern 1pt} 2.5\% {\text{/}}1\) mm. The maximum amplitude of background brightness variability on short time scales (\( \sim {\kern 1pt} 30\) min) has been estimated: \( \approx {\kern 1pt} 10\)% in the \(J\) and \(K\) bands and \( \approx {\kern 1pt} 30\)% in the \(H\) band. The maximum contribution of Moon’s radiation scattered in the atmosphere to the overall background level has been determined. It is shown that this contribution can be ignored at an angular distance from the Moon greater than \( \sim {\kern 1pt} 10^\circ \) even during a full moon. The average background surface brightness mag/arcsec2 in the J, H, and \(K\) bands was calculated: \({{m}_{J}} = 15.7\), \({{m}_{H}} = 13.9\), and \({{m}_{K}} = 13.1\).

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来源期刊
Astronomy Reports
Astronomy Reports 地学天文-天文与天体物理
CiteScore
1.40
自引率
20.00%
发文量
57
审稿时长
6-12 weeks
期刊介绍: Astronomy Reports is an international peer reviewed journal that publishes original papers on astronomical topics, including theoretical and observational astrophysics, physics of the Sun, planetary astrophysics, radio astronomy, stellar astronomy, celestial mechanics, and astronomy methods and instrumentation.
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