SDSS J013127.34-032100.1: A NEWLY DISCOVERED RADIO-LOUD QUASAR AT z=5.18 WITH EXTREMELY HIGH LUMINOSITY
文献类型：期刊论文
| 作者 | Yi WM(易卫敏)1,2,3 ; Wang, FG4; Wu, XB4,5; Yang, JY4; Bai JM(白金明)1,3; Fan, XH6; Brandt, WN7; Ho, LC4,5; Zuo, WW4,8; Kim, M9
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| 刊名 | ASTROPHYSICAL JOURNAL LETTERS
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| 出版日期 | 2014-11-10 |
| 卷号 | 795期号:2页码:29-33 |
| 关键词 | galaxies: active galaxies: high-redshift quasars: individual (SDSS J0131-0321) |
| ISSN号 | 2041-8205 |
| 产权排序 | 第一完成单位 |
| 通讯作者 | Yi, WM (reprint author), Chinese Acad Sci, Yunnan Observ, Kunming 650011, Peoples R China. |
| 英文摘要 | Very few of the z > 5 quasars discovered to date have been radio-loud, with radio-to-optical flux ratios (radio-loudness parameters) higher than 10. Here we report the discovery of an optically luminous radio-loud quasar, SDSS J013127.34-032100.1 (J0131-0321 in short), at z = 5.18 +/- 0.01 using the Lijiang 2.4 m and Magellan telescopes. J0131-0321 has a spectral energy distribution consistent with that of radio-loud quasars. With an i-band magnitude of 18.47 and a radio flux density of 33 mJy, its radio-loudness parameter is similar to 100. The optical and near-infrared spectra taken by Magellan enable us to estimate its bolometric luminosity to be L-bol similar to 1.1 x 10(48) erg s(-1), approximately 4.5 times greater than that of the most distant quasar known to date. The black hole mass of J0131-0321 is estimated to be 2.7 x 10(9) M-circle dot, with an uncertainty up to 0.4 dex. Detailed physical properties of this high-redshift, radio-loud, potentially super-Eddington quasar can be probed in the future with more dedicated and intensive follow-up observations using multi-wavelength facilities. |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 学科主题 | Astronomy & Astrophysics |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | DIGITAL SKY SURVEY ; ACTIVE GALACTIC NUCLEI ; HOLE MASS ESTIMATORS ; BLACK-HOLE ; DATA RELEASE ; REDSHIFT ; ACCRETION ; EVOLUTION ; CATALOG |
| 收录类别 | SCI |
| 原文出处 | http://iopscience.iop.org/article/10.1088/2041-8205/795/2/L29/meta |
| 语种 | 英语 |
| WOS记录号 | WOS:000345499000005 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/5434]  |
| 专题 | 云南天文台_丽江天文观测站（南方基地） 云南天文台_中国科学院天体结构与演化重点实验室 |
| 作者单位 | 1.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China 2.University of the Chinese Academy of Sciences, Beijing 100049, China 3.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650011, China 4.Department of Astronomy, School of Physics, Peking University, Beijing 100871, China 5.Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, China 6.Steward Observatory, University of Arizona, Tucson, AZ 85721-0065, USA 7.Department of Astronomy and Astrophysics, The Pennsylvania State University, 525 Davey Lab, University Park, PA 16802, USA 8.Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China 9.Korea Astronomy and Space Science Institute, Daejeon 305-348, Korea |
| 推荐引用方式 GB/T 7714 | Yi WM,Wang, FG,Wu, XB,et al. SDSS J013127.34-032100.1: A NEWLY DISCOVERED RADIO-LOUD QUASAR AT z=5.18 WITH EXTREMELY HIGH LUMINOSITY[J]. ASTROPHYSICAL JOURNAL LETTERS,2014,795(2):29-33. |
| APA | Yi WM.,Wang, FG.,Wu, XB.,Yang, JY.,Bai JM.,...&Xin YX.(2014).SDSS J013127.34-032100.1: A NEWLY DISCOVERED RADIO-LOUD QUASAR AT z=5.18 WITH EXTREMELY HIGH LUMINOSITY.ASTROPHYSICAL JOURNAL LETTERS,795(2),29-33. |
| MLA | Yi WM,et al."SDSS J013127.34-032100.1: A NEWLY DISCOVERED RADIO-LOUD QUASAR AT z=5.18 WITH EXTREMELY HIGH LUMINOSITY".ASTROPHYSICAL JOURNAL LETTERS 795.2(2014):29-33. |
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来源：云南天文台
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