Forecasting the dark energy measurement with baryon acoustic oscillations: prospects for the LAMOST surveys
文献类型：期刊论文
| 作者 | Wang, Xin1; Chen, Xuelei1; Zheng, Zheng2; Wu, Fengquan1; Zhang, Pengjie3; Zhao, Yongheng1 |
| 刊名 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
 |
| 出版日期 | 2009-04-21 |
| 卷号 | 394期号:4页码:1775-1790 |
| 关键词 | cosmological parameters large-scale structure of Universe |
| 英文摘要 | The Large Area Multi-Object Fibre Spectroscopic Telescope (LAMOST) is a dedicated spectroscopic survey telescope being built in China, with an effective aperture of 4 in and equipped with 4000 fibres. Using the LAMOST telescope. one could make redshift survey of the large-scale scale structure (LSS). The baryon acoustic oscillation features in the LSS power spectrum provide standard rulers for measuring dark energy and other cosmological parameters. In this paper, we investigate the measurement precision achievable for a few possible surveys: (1) a magnitude-limited Survey of all galaxies. (2) a survey Of colour-selected luminous red galaxies (LRG) and (3) a magnitude-limited. high-density survey of z < 2 quasars. For each survey, we Use the halo model to estimate the bias of the sample, and calculate the effective volume. We then use the Fisher matrix method to forecast the error on the dark energy equation Of State and other cosmological parameters for different survey parameters. In a few cases, we also use the Markov Chain Monte Carlo method to make the same forecast as a comparison. The fibre time required for each of these Surveys is also estimated. These results Would he useful in designing the surveys for LAMOST. |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | DIGITAL SKY SURVEY ; LUMINOUS RED GALAXIES ; HALO OCCUPATION DISTRIBUTION ; SPECTROSCOPIC TARGET SELECTION ; REDSHIFT-SPACE DISTORTIONS ; POWER-SPECTRUM ANALYSIS ; SURVEY QUASAR CATALOG ; LARGE-SCALE STRUCTURE ; 2DF-SDSS LRG ; RESOLUTION SPECTROGRAPH |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000266549600006 |
| 源URL | [http://119.78.226.72/handle/331011/19580]  |
| 专题 | 上海天文台_星系宇宙学重点实验室 |
| 作者单位 | 1.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China 2.Inst Adv Study, Princeton, NJ 08540 USA 3.Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China |
| 推荐引用方式 GB/T 7714 | Wang, Xin,Chen, Xuelei,Zheng, Zheng,et al. Forecasting the dark energy measurement with baryon acoustic oscillations: prospects for the LAMOST surveys[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2009,394(4):1775-1790. |
| APA | Wang, Xin,Chen, Xuelei,Zheng, Zheng,Wu, Fengquan,Zhang, Pengjie,&Zhao, Yongheng.(2009).Forecasting the dark energy measurement with baryon acoustic oscillations: prospects for the LAMOST surveys.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,394(4),1775-1790. |
| MLA | Wang, Xin,et al."Forecasting the dark energy measurement with baryon acoustic oscillations: prospects for the LAMOST surveys".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 394.4(2009):1775-1790. |
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来源：上海天文台
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