theeffectsofspectrographslitmodesontheaccuracyofstellarradialvelocitymeasurementandatmosphericparameterestimation
文献类型：期刊论文
| 作者 | Wang Fengfei2; Zhang Haotong2 ; Luo Ali2; Bai Zhongrui2; Du Bing1; Zhao Yongheng2
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| 刊名 | sciencechinaphysicsmechanicsastronomy
 |
| 出版日期 | 2013 |
| 卷号 | 56期号:10页码:1833 |
| ISSN号 | 1674-7348 |
| 英文摘要 | Spectrograph slit is conventionally used to enhance the spectral resolution and manage how much light can be allowed to enter spectrograph. The narrow slit provides a higher resolution but sacrifices efficiency of spectrograph and results in a low signal to noise ratio (S/N) spectra product. We take GuoShouJing telescope as an example and carry out a series of experiments to study how its 2/3 slit mode affects the precision of stellar radial velocity measurement and atmosphere parameters estimate. By transforming the resolution and adding a Gaussian White Noise to the extremely high quality spectra from the Sloan Digital Sky Survey, we generate synthetic stellar spectra of various brightness with different S/Ns. Comparing the measurements on these noise added spectra with the original high quality ones, we summarize the influences of the 2/3 slit mode on the measurement accuracy of stellar radial velocity and atmospheric parameters. |
| 语种 | 英语 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/37580]  |
| 专题 | 光学部_LAMOST运行和发展中心 |
| 作者单位 | 1.中国科学院大学 2.中国科学院国家天文台 |
| 推荐引用方式 GB/T 7714 | Wang Fengfei,Zhang Haotong,Luo Ali,et al. theeffectsofspectrographslitmodesontheaccuracyofstellarradialvelocitymeasurementandatmosphericparameterestimation[J]. sciencechinaphysicsmechanicsastronomy,2013,56(10):1833. |
| APA | Wang Fengfei,Zhang Haotong,Luo Ali,Bai Zhongrui,Du Bing,&Zhao Yongheng.(2013).theeffectsofspectrographslitmodesontheaccuracyofstellarradialvelocitymeasurementandatmosphericparameterestimation.sciencechinaphysicsmechanicsastronomy,56(10),1833. |
| MLA | Wang Fengfei,et al."theeffectsofspectrographslitmodesontheaccuracyofstellarradialvelocitymeasurementandatmosphericparameterestimation".sciencechinaphysicsmechanicsastronomy 56.10(2013):1833. |
入库方式： OAI收割
来源：国家天文台
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