The nature of [S III]lambda lambda 9096, 9532 emitters at z=1.34 and 1.23
文献类型：期刊论文
| 作者 | An FangXia1,2 ; Zheng XianZhong2; Meng YanZhi2; Chen Yang3; Wen ZhangZheng2; Lu GuoLiang1
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| 刊名 | SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY
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| 出版日期 | 2013-11-01 |
| 卷号 | 56期号:11页码:2226-2235 |
| 关键词 | galaxies: evolution galaxies: high-redshift galaxies: emission lines [S III] |
| 通讯作者 | Appleton, PN (通讯作者) CALTECH, NASA, Herschel Sci Ctr, Pasadena, CA 91125 USA. |
| 英文摘要 | A study of [S iii]lambda lambda 9096, 9532 emitters at z = 1.34 and 1.23 is presented using our deep narrow-band H (2) S 1 (centered at 2.13 mu m) imaging survey of the Extended Chandra Deep Field South (ECDFS). We combine our data with multi-wavelength data of ECDFS to build up spectral energy distributions (SEDs) from the U to the K (s)-band for emitter candidates selected with strong excess in H (2) S 1 - K (s) and derive photometric redshifts, line luminosities, stellar masses and extinction. A sample of 14 [S iii] emitters are identified with H (2) S 1 < 22.8 and K (s) < 24.8 (AB) over 381 arcmin(2) area, having [S iii] line luminosity L ([SIII]) =similar to 1041.5-42.6 erg s(-1). None of the [S iii] emitters is found to have X-ray counterpart in the deepest Chandra 4Ms observation, suggesting that they are unlikely powered by AGNs. The HST/ACS F606W and HST/WFC3 F160W images show their rest-frame UV and optical morphologies. About half of the [S iii] emitters are mergers and at least one third are disk-type galaxies. Nearly all [S iii] emitters exhibit a prominent Balmer break in their SEDs, indicating the presence of a significant post-starburst component. Taken together, our results imply that both shock heating in post-starburst and photoionization caused by young massive stars are likely to excite strong [S iii] emission lines. We conclude that the [S iii] emitters in our sample are dominated by star-forming galaxies (SFGs) with stellar mass 8.7 < log(M/M (aS (TM))) < 9.9. |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 学科主题 | Astronomy & Astrophysics |
| 类目[WOS] | Physics, Multidisciplinary |
| 研究领域[WOS] | Physics |
| 关键词[WOS] | STAR-FORMING GALAXIES ; DEEP FIELD-SOUTH ; EXTRAGALACTIC LEGACY SURVEY ; NEAR-INFRARED SPECTROSCOPY ; ALPHA LUMINOSITY FUNCTION ; HIGH-REDSHIFT GALAXIES ; YALE-CHILE MUSYC ; FORMATION HISTORY ; HII GALAXIES ; MULTIWAVELENGTH SURVEY |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000326643100032 |
| 公开日期 | 2014-01-08 |
| 源URL | [http://libir.pmo.ac.cn/handle/332002/9787]  |
| 专题 | 紫金山天文台_暗物质和空间天文实验室 |
| 作者单位 | 1.Xinjiang Univ, Sch Phys & Technol, Urumqi 830046, Peoples R China 2.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China 3.Univ Sci & Technol China, Ctr Astrophys, Hefei 230026, Peoples R China |
| 推荐引用方式 GB/T 7714 | An FangXia,Zheng XianZhong,Meng YanZhi,et al. The nature of [S III]lambda lambda 9096, 9532 emitters at z=1.34 and 1.23[J]. SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,2013,56(11):2226-2235. |
| APA | An FangXia,Zheng XianZhong,Meng YanZhi,Chen Yang,Wen ZhangZheng,&Lu GuoLiang.(2013).The nature of [S III]lambda lambda 9096, 9532 emitters at z=1.34 and 1.23.SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,56(11),2226-2235. |
| MLA | An FangXia,et al."The nature of [S III]lambda lambda 9096, 9532 emitters at z=1.34 and 1.23".SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY 56.11(2013):2226-2235. |
入库方式： OAI收割
来源：紫金山天文台
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