Scientific Objectives of the Hot Universe Baryon Surveyor (HUBS) Mission
The Hot Universe Baryon Surveyor (HUBS) is a proposed space-based X-ray telescope for detecting X-ray emissions from the hot gas content in our universe. With its unprecedented spatially-resolved high-resolution spectroscopy and large field of view, the HUBS mission will be uniquely qualified to mea...
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| creator | Bregman, Joel Cen, Renyue Chen, Yang Cui, Wei Fang, Taotao Guo, Fulai Hodges-Kluck, Edmund Huang, Rui Ho, Luis C Li, Ji Ji, Suoqing Kang, Xi Lai, Xiaoyu Li, Hui Li, Jiangtao Li, Miao Li, Xiangdong Li, Yuan Li, Zhaosheng Liang, Guiyun Liu, Helei Liu, Wenhao Lu, Fangjun Mao, Junjie Ponti, Gabriele Qu, Zhijie Shan, Chenxi Shao, Lijing Shi, Fangzheng Shu, Xinwen Sun, Lei Sun, Mouyuan Tong, Hao Wang, Junfeng Wang, Junxian Wang, Q Daniel Wang, Song Wang, Tinggui Wang, Weiyang Wang, Zhongxiang Xu, Dandan Xu, Haiguang Xu, Heng Xu, Renxin Xu, Xiaojie Xue, Yongquan Yang, Hang Yuan, Feng Zhang, Shuinai Zhang, Yuning Zhang, Zhongli Zhao, Yuanyuan Zhou, Enping Zhou, Ping |
| description | The Hot Universe Baryon Surveyor (HUBS) is a proposed space-based X-ray telescope for detecting X-ray emissions from the hot gas content in our universe. With its unprecedented spatially-resolved high-resolution spectroscopy and large field of view, the HUBS mission will be uniquely qualified to measure the physical and chemical properties of the hot gas in the interstellar medium, the circumgalactic medium, the intergalactic medium, and the intracluster medium. These measurements will be valuable for two key scientific goals of HUBS, namely to unravel the AGN and stellar feedback physics that governs the formation and evolution of galaxies, and to probe the baryon budget and multi-phase states from galactic to cosmological scales. In addition to these two goals, the HUBS mission will also help us solve some problems in the fields of galaxy clusters, AGNs, diffuse X-ray backgrounds, supernova remnants, and compact objects. This paper discusses the perspective of advancing these fields using the HUBS telescope. |
| doi_str_mv | 10.48550/arxiv.2307.05672 |
| format | Article |
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With its unprecedented spatially-resolved high-resolution spectroscopy and large field of view, the HUBS mission will be uniquely qualified to measure the physical and chemical properties of the hot gas in the interstellar medium, the circumgalactic medium, the intergalactic medium, and the intracluster medium. These measurements will be valuable for two key scientific goals of HUBS, namely to unravel the AGN and stellar feedback physics that governs the formation and evolution of galaxies, and to probe the baryon budget and multi-phase states from galactic to cosmological scales. In addition to these two goals, the HUBS mission will also help us solve some problems in the fields of galaxy clusters, AGNs, diffuse X-ray backgrounds, supernova remnants, and compact objects. This paper discusses the perspective of advancing these fields using the HUBS telescope.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.2307.05672</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Active galactic nuclei ; Baryons ; Chemical properties ; Galactic clusters ; Galactic evolution ; Galaxies ; Hubs ; Intergalactic media ; Interstellar chemistry ; Interstellar gas ; Interstellar matter ; Physics - Astrophysics of Galaxies ; Physics - Cosmology and Nongalactic Astrophysics ; Physics - High Energy Astrophysical Phenomena ; Physics - Instrumentation and Methods for Astrophysics ; Physics - Solar and Stellar Astrophysics ; Spaceborne telescopes ; Supernova remnants ; Universe ; X ray telescopes ; X-ray astronomy</subject><ispartof>arXiv.org, 2023-07</ispartof><rights>2023. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). 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With its unprecedented spatially-resolved high-resolution spectroscopy and large field of view, the HUBS mission will be uniquely qualified to measure the physical and chemical properties of the hot gas in the interstellar medium, the circumgalactic medium, the intergalactic medium, and the intracluster medium. These measurements will be valuable for two key scientific goals of HUBS, namely to unravel the AGN and stellar feedback physics that governs the formation and evolution of galaxies, and to probe the baryon budget and multi-phase states from galactic to cosmological scales. In addition to these two goals, the HUBS mission will also help us solve some problems in the fields of galaxy clusters, AGNs, diffuse X-ray backgrounds, supernova remnants, and compact objects. This paper discusses the perspective of advancing these fields using the HUBS telescope.</description><subject>Active galactic nuclei</subject><subject>Baryons</subject><subject>Chemical properties</subject><subject>Galactic clusters</subject><subject>Galactic evolution</subject><subject>Galaxies</subject><subject>Hubs</subject><subject>Intergalactic media</subject><subject>Interstellar chemistry</subject><subject>Interstellar gas</subject><subject>Interstellar matter</subject><subject>Physics - Astrophysics of Galaxies</subject><subject>Physics - Cosmology and Nongalactic Astrophysics</subject><subject>Physics - High Energy Astrophysical Phenomena</subject><subject>Physics - Instrumentation and Methods for Astrophysics</subject><subject>Physics - Solar and Stellar Astrophysics</subject><subject>Spaceborne telescopes</subject><subject>Supernova remnants</subject><subject>Universe</subject><subject>X ray telescopes</subject><subject>X-ray astronomy</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><sourceid>BENPR</sourceid><sourceid>GOX</sourceid><recordid>eNotj0FLwzAcxYMgOOY-gCcDXvTQmfzTpOnRDWeFyQ7dziWJCaZoM5N2uG9v3Tw9eO_xeD-EbiiZ55Jz8qjijz_MgZFiTrgo4AJNgDGayRzgCs1SagkhMAacswmqauNt13vnDd7o1preH2zCweH-w-Iq9HjXjU5MFi9UPIYO10M82GOI-L7aLeoH_OZT8qG7RpdOfSY7-9cp2q6et8sqW29eXpdP60yVHDJNlTTaacgLYojRecGoEznjwFT5Ti0Y55Q2BGipC2ZySYiRWilhrQBOSzZFt-fZE2azj_5rvNX84TYn3LFxd27sY_gebOqbNgyxGz81IJkQglIp2S-folcq</recordid><startdate>20230711</startdate><enddate>20230711</enddate><creator>Bregman, Joel</creator><creator>Cen, Renyue</creator><creator>Chen, Yang</creator><creator>Cui, Wei</creator><creator>Fang, Taotao</creator><creator>Guo, Fulai</creator><creator>Hodges-Kluck, Edmund</creator><creator>Huang, Rui</creator><creator>Ho, Luis C</creator><creator>Li, Ji</creator><creator>Ji, Suoqing</creator><creator>Kang, 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; Li, Ji ; Ji, Suoqing ; Kang, Xi ; Lai, Xiaoyu ; Li, Hui ; Li, Jiangtao ; Li, Miao ; Li, Xiangdong ; Li, Yuan ; Li, Zhaosheng ; Liang, Guiyun ; Liu, Helei ; Liu, Wenhao ; Lu, Fangjun ; Mao, Junjie ; Ponti, Gabriele ; Qu, Zhijie ; Shan, Chenxi ; Shao, Lijing ; Shi, Fangzheng ; Shu, Xinwen ; Sun, Lei ; Sun, Mouyuan ; Tong, Hao ; Wang, Junfeng ; Wang, Junxian ; Wang, Q Daniel ; Wang, Song ; Wang, Tinggui ; Wang, Weiyang ; Wang, Zhongxiang ; Xu, Dandan ; Xu, Haiguang ; Xu, Heng ; Xu, Renxin ; Xu, Xiaojie ; Xue, Yongquan ; Yang, Hang ; Yuan, Feng ; Zhang, Shuinai ; Zhang, Yuning ; Zhang, Zhongli ; Zhao, Yuanyuan ; Zhou, Enping ; Zhou, Ping</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a952-b1a8cbfb2470c0cb4731f643523a9d1e2cffabc0219b73c4800c8baa6ee625193</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2023</creationdate><topic>Active galactic nuclei</topic><topic>Baryons</topic><topic>Chemical properties</topic><topic>Galactic clusters</topic><topic>Galactic evolution</topic><topic>Galaxies</topic><topic>Hubs</topic><topic>Intergalactic media</topic><topic>Interstellar chemistry</topic><topic>Interstellar gas</topic><topic>Interstellar matter</topic><topic>Physics - Astrophysics of Galaxies</topic><topic>Physics - Cosmology and Nongalactic Astrophysics</topic><topic>Physics - High Energy Astrophysical Phenomena</topic><topic>Physics - Instrumentation and Methods for Astrophysics</topic><topic>Physics - Solar and Stellar Astrophysics</topic><topic>Spaceborne telescopes</topic><topic>Supernova remnants</topic><topic>Universe</topic><topic>X ray telescopes</topic><topic>X-ray astronomy</topic><toplevel>online_resources</toplevel><creatorcontrib>Bregman, Joel</creatorcontrib><creatorcontrib>Cen, Renyue</creatorcontrib><creatorcontrib>Chen, Yang</creatorcontrib><creatorcontrib>Cui, Wei</creatorcontrib><creatorcontrib>Fang, Taotao</creatorcontrib><creatorcontrib>Guo, 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With its unprecedented spatially-resolved high-resolution spectroscopy and large field of view, the HUBS mission will be uniquely qualified to measure the physical and chemical properties of the hot gas in the interstellar medium, the circumgalactic medium, the intergalactic medium, and the intracluster medium. These measurements will be valuable for two key scientific goals of HUBS, namely to unravel the AGN and stellar feedback physics that governs the formation and evolution of galaxies, and to probe the baryon budget and multi-phase states from galactic to cosmological scales. In addition to these two goals, the HUBS mission will also help us solve some problems in the fields of galaxy clusters, AGNs, diffuse X-ray backgrounds, supernova remnants, and compact objects. This paper discusses the perspective of advancing these fields using the HUBS telescope.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.2307.05672</doi><oa>free_for_read</oa></addata></record> |
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| subjects | Active galactic nuclei Baryons Chemical properties Galactic clusters Galactic evolution Galaxies Hubs Intergalactic media Interstellar chemistry Interstellar gas Interstellar matter Physics - Astrophysics of Galaxies Physics - Cosmology and Nongalactic Astrophysics Physics - High Energy Astrophysical Phenomena Physics - Instrumentation and Methods for Astrophysics Physics - Solar and Stellar Astrophysics Spaceborne telescopes Supernova remnants Universe X ray telescopes X-ray astronomy |
| title | Scientific Objectives of the Hot Universe Baryon Surveyor (HUBS) Mission |
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