Institutional Repository System Of Yunnan Observatories, CAS
| Constraints on cosmic star formation history via a new modeling of the radio luminosity function of star-forming galaxies | |
Wang, Wenjie1,2; Yuan, Zunli1,2; Yu, Hongwei1,2,3; Mao JR(毛基荣)4,5,6
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| 发表期刊 | Astronomy and Astrophysics
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| 2024-03-01 | |
| 卷号 | 683 |
| DOI | 10.1051/0004-6361/202347746 |
| 产权排序 | 第4完成单位 |
| 收录类别 | EI |
| 关键词 | Galaxy: evolution galaxies: luminosity function mass function galaxies: star formation radio continuum: galaxies |
| 摘要 | Context. Radio wavelengths offer a unique possibility to trace the total star-formation rate (SFR) in galaxies, both obscured and unobscured. To probe the dust-unbiased star-formation history, an accurate measurement of the radio luminosity function (LF) for star-forming galaxies (SFGs) is crucial. Aims. We make use of an SFG sample (5900 sources) from the Very Large Array (VLA) COSMOS 3 GHz data to perform a new modeling of the radio LF. By integrating the analytical LF, we aim to calculate the history of the cosmic SFR density (SFRD) from z ∼ 5 onwards. Methods. For the first time, we use both models of the pure luminosity evolution (PLE) and joint luminosity+density evolution (LADE) to fit the LFs directly to the radio data using a full maximum-likelihood analysis, considering the sample completeness correction. We also incorporate updated observations of local radio LFs and radio source counts into the fitting process to obtain additional constraints. Results. We find that the PLE model cannot be used to describe the evolution of the radio LF at high redshift (z > 2). By construct, our LADE models can successfully fit a large amount of data on radio LFs and source counts of SFGs from recent observations. The Akaike information criterion (AIC) also demonstrates that the LADE model is superior to the PLE model. We therefore conclude that density evolution is genuinely indispensable in modeling the evolution of SFG radio LFs. Our SFRD curve shows a good fit to the SFRD points derived by previous radio estimates. In view of the fact that our radio LFs are not biased, as opposed those of previous studies performed by fitting the 1/Vmax LF points, our SFRD results should be an improvement on these previous estimates. Below z ∼ 1.5, our SFRD matches a published multiwavelength compilation, while our SFRD turns over at a slightly higher redshift (2 © 2024 EDP Sciences. All rights reserved. |
| 资助项目 | National Key R&D Program of China[2023YFE0101200]; National Natural Science Foundation of China[12073069]; National Natural Science Foundation of China[12075084]; National Natural Science Foundation of China[12393813]; Xiaoxiang Scholars Programme of Hunan Normal University; China Manned Space Project[CMS-CSST2021-A06]; Yunnan Revitalization Talent Support Program |
| 项目资助者 | National Key R&D Program of China[2023YFE0101200] ; National Natural Science Foundation of China[12073069, 12075084, 12393813] ; Xiaoxiang Scholars Programme of Hunan Normal University ; China Manned Space Project[CMS-CSST2021-A06] ; Yunnan Revitalization Talent Support Program |
| 语种 | 英语 |
| 学科领域 | 天文学 |
| 文章类型 | Article |
| 出版者 | EDP SCIENCES S A |
| 出版地 | 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE |
| ISSN | 0004-6361 |
| URL | 查看原文 |
| WOS记录号 | WOS:001186725700007 |
| WOS研究方向 | Astronomy & Astrophysics |
| WOS类目 | Astronomy & Astrophysics |
| 关键词[WOS] | HUBBLE FRONTIER FIELDS ; GHZ LARGE PROJECT ; FAR-INFRARED/RADIO CORRELATION ; SPECTRAL ENERGY-DISTRIBUTION ; ACTIVE GALACTIC NUCLEI ; FORMATION RATE DENSITY ; SOURCE COUNTS ; BRIGHT END ; RAPID EVOLUTION ; FORMATION RATES |
| EI入藏号 | 20241215790581 |
| EI主题词 | Luminance |
| EI分类号 | 657.2 Extraterrestrial Physics and Stellar Phenomena - 922 Statistical Methods |
| 引用统计 | |
| 文献类型 | 期刊论文 |
| 条目标识符 | http://ir.ynao.ac.cn/handle/114a53/26560 |
| 专题 | 星系类星体研究组 中国科学院天体结构与演化重点实验室 |
| 作者单位 | 1.Department of Physics, School of Physics and Electronics, Hunan Normal University, Changsha, 410081, China; 2.Key Laboratory of Low Dimensional Quantum Structures and Quantum Control, Hunan Normal University, Changsha, 410081, China; 3.Synergetic Innovation Center for Quantum Effects and Applications, Institute of Interdisciplinary Studies, Hunan Normal University, Hunan, Changsha, 410081, China; 4.Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650216, China; 5.Center for Astronomical Mega-Science, Chinese Academy of Sciences, Beijing, 100012, China; 6.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming, 650216, China |
| 推荐引用方式 GB/T 7714 | Wang, Wenjie,Yuan, Zunli,Yu, Hongwei,et al. Constraints on cosmic star formation history via a new modeling of the radio luminosity function of star-forming galaxies[J]. Astronomy and Astrophysics,2024,683. |
| APA | Wang, Wenjie,Yuan, Zunli,Yu, Hongwei,&毛基荣.(2024).Constraints on cosmic star formation history via a new modeling of the radio luminosity function of star-forming galaxies.Astronomy and Astrophysics,683. |
| MLA | Wang, Wenjie,et al."Constraints on cosmic star formation history via a new modeling of the radio luminosity function of star-forming galaxies".Astronomy and Astrophysics 683(2024). |
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| Constraints on cosmi（3404KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 | |
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