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中国科学院近代物理研究所
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Astronomy Department, Faculty of Science, King Abdulaziz University, P. O. Box 80203, Jeddah 21589, Saudi Arabia
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BIPAC, Department of Physics, University of Oxford, Keble Road, Oxford OX1 3RH, UK
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Center for Astrophysics, Guangzhou University, 510006 Guangzhou, People’s Republic of China
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Centre for Extragalactic Astronomy, Department of Physics, Durham University, South Rd, Durham, DH1 3LE, UK
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Centre for Extragalactic Astronomy, Department of Physics, Durham University, South Road, Durham DH1 3LE, UK
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Centro de Astronom´ıa (CITEVA), Universidad de Antofagasta, Avenida Angamos 601, Antofagasta, Chile
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College of Physics Science and Technology, Hebei University, Baoding 071002, China
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Department of Astronomy and Astrophysics, 525 Davey Lab, The Pennsylvania State University, University Park, PA 16802, USA
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Department of Astronomy, School of Physics, Peking University, Beĳing 100871, People’s Republic of China
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Department of Astronomy, University of Florida, PO Box 112055, USA
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Department of Mathematics, Presidency University, 86/1 College Street, Kolkata 700073, India
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Department of Physics and Astronomy, Texas A&M University, College Station, TX 77843-4242, USA
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Department of Physics and Astronomy, The Johns Hopkins University Homewood Campus, Baltimore, MD 21218, USA
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Department of Physics, 104 Davey Laboratory, The Pennsylvania State University, University Park, PA 16802, USA
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Department of Physics, Liaoning Normal University, Dalian, 116029, P. R. China
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Galileo Galilei Institute for theoretical physics, Centro Nazionale INFN di Studi Avanzati Largo Enrico Fermi 2, I-50125, Firenze, Italy
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George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, TX 77843-4242, USA
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Hebei Key Lab of Optic-Electronic Information and Materials, Hebei University, Baoding 071002, China
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INFN Sezione di Roma, P.le A. Moro 2, I-00185, Roma, Italy
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Institut d’Astrophysique de Paris (UMR7095: CNRS & UPMC- Sorbonne Universities), F-75014, Paris, France
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Institute for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh, EH9 3HJ, UK
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Institute for Computational Cosmology, Department of Physics, Durham University, South Road, Durham DH1 3LE, UK
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Institute for Gravitation and the Cosmos, The Pennsylvania State University, University Park, PA 16802, USA
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Institute of Systems Science, Durban University of Technology, PO Box 1334, Durban 4000, Republic of South Africa
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Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA
1
Kapteyn Astronomical Institute, University of Groningen, P.O. Box 800, 9700 AV Groningen, The Netherlands
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Kavli Institute for Astronomy and Astrophysics, Peking University, Beĳing 100871, People’s Republic of China
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Key Laboratory of High-pricision Computation and Application of Quantum Field Theory of Hebei Province, Hebei University, Baoding 071002, China
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Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
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National Astronomical Observatories, Chinese Academy of Sciences, 20A Datun Road,Chaoyang District, Beĳing 100012, China
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National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
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National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903-2475, USA
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National-Local Joint Engineering Laboratory of New Energy Photoelectric Devices, Hebei University, Baoding 071002, China
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Physics Department and INFN, Universit`a di Roma “La Sapienza”, Ple Aldo Moro 2, 00185, Rome, Italy
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Research School of Astronomy and Astrophysics, Australian National University, Canberra ACT 2601, Australia
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SRON Netherlands Institute for Space Research, Postbus 800, 9700 AV Groningen, The Netherlands
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School of Astronomy and Space Science, University of Chinese Academy of Sciences, Beĳing 100049, China
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School of Mathematics and Statistics, University of Sheffield, Hounsfield Road, Sheffield S3 7RH, United Kingdom
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Scuola Normale Superiore, Piazza dei Cavalieri 7, I-56126 Pisa, Italy
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Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, People’s Republic of China
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University of Chinese Academy of Sciences, 19A Yuquan Road, Beĳing 100049, People’s Republic of China
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Xinjiang Astronomical Observatory, Chinese Academy of Sciences, 830011 Urumqi, PR China
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Zhejiang University
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兰州大学物理学院
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杭州师范大学
1

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1. ChinaXiv:202305.00221
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Possible evidences from H(z) parameter data for physics beyond Lambda CDM

分类：天文学 >> 星系和宇宙学提交时间： 2023-05-24

Yang, Rong-Jia

摘要： Calculus. We find that: (1) there exists at least one decelerated phase at 1 $ sigma$ confidence level in

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点击量 1703 下载量 160 评论 0
2. ChinaXiv:202302.00235
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Galaxy-galaxy strong lens perturbations: line-of-sight haloes versus lens subhaloes

分类：天文学 >> 星系和宇宙学提交时间： 2023-02-21

Qiuhan He Ran Li Carlos S. Frenk James Nightingale Shaun Cole Nicola C. Amorisco Richard Massey Andrew Robertson Amy Etherington Aristeidis Amvrosiadis Xiaoyue Cao

摘要：We rederive the number density of intervening line-of-sight haloes relative to lens subhaloes in

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3. ChinaXiv:202302.00238
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Revealing the effects of curvature on the cosmological models

分类：天文学 >> 星系和宇宙学提交时间： 2023-02-21

Weiqiang Yang William Giare Supriya Pan Eleonora Di Valentino Alessandro Melchiorri Joseph Silk

摘要：In this paper we consider the effects of adding curvature in extended cosmologies involving a free-

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4. ChinaXiv:202302.00240
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X-ray Emission from the Interstellar and Circumgalactic Medium of Elliptical Galaxies based on

分类：天文学 >> 星系和宇宙学提交时间： 2023-02-21

Aditi Vijayan Bocheng Zhu Miao Li Feng Yuan Luis C. Ho

摘要： has been linked to the AGN feedback occurring in the host. Upcoming telescopes such as HUBS, with ~ 1

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5. ChinaXiv:202302.00241
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Discovery of non-metastable ammonia masers in Sagittarius B2

分类：天文学 >> 星系和宇宙学提交时间： 2023-02-21

Y. T. Yan C. Henkel K. M. Menten Y. Gong H. Nguyen J. Ott A. Ginsburg T. L. Wilson A. Brunthaler A. Belloche J. S. Zhang N. Budaiev D.Jeff

摘要：We report the discovery of widespread maser emission in non-metastable inversion transitions of NH_

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6. ChinaXiv:202302.00242
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Does the lockstep growth between black holes and bulges create their mass relation?

分类：天文学 >> 星系和宇宙学提交时间： 2023-02-21

Guang Yang W. N. Brandt David M. Alexander Médéric Boquien Qingling Ni Casey Papovich Justin S. Spilker Fabio Vito Jonelle L. Walsh Chengpeng Zhang

摘要： correlation observed in the local universe. To understand further BH-bulge coevolution, we present ALMA CO(2-1

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7. ChinaXiv:201610.00003
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相对的时空标度和绝对的时空背景

分类：物理学 >> 地球物理学、天文学和天体物理学分类：物理学 >> 电磁学、光学、声学、传热、经典力学和流体动力学分类：天文学 >> 星系和宇宙学提交时间： 2022-11-03

陈驰一

摘要：本文以物理学中标准钟和标准尺的定义实质和爱因斯坦的相对论物理为基础，从自然哲学层次出发讨论了物理的时空观。提出在已有的时空标度的概念基础上，应该进一步明确区分时空标度和时空背景。根据爱因斯坦相对论的

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8. ChinaXiv:202009.00012
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Shadows of rotating Hayward-de Sitter black holes with astrometric observables

分类：物理学 >> 地球物理学、天文学和天体物理学分类：天文学 >> 星系和宇宙学提交时间： 2020-09-09

Peng-Zhang He Qi-Qi Fan Hao-Ran Zhang Jian-Bo Deng

摘要： Motivated by recent work on rotating black hole shadow [Phys. Rev. D101,

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点击量 18757 下载量 1861 评论 0
9. ChinaXiv:201804.02356
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Some correlations in CLASH clusters

分类：天文学 >> 星系和宇宙学提交时间： 2018-04-25

李希国

摘要：本文是[1]对冲突簇的延续和推广。我们研究冲突子群中的总、暗物质密度分布和关联。就像我们对纽曼星系团所做的那样。就像Newman星系团一样，我们发现密度分布受重子相互作用和能量的影响很大。角动量通过

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10. ChinaXiv:201804.00472
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On the dwarf galaxies rotation curves diversity problem

分类：天文学 >> 星系和宇宙学提交时间： 2018-03-27

李希国

摘要：在本文中，我们将展示重子物理是如何解决矮星中惊人的多样性问题的。星系旋转曲线形状。为此，我们比较了SPARC样本的星系分布。平面V2kpc-V最后(V2kpc是星系在2 kpc时的旋转速度，V是

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11. ChinaXiv:201803.01555
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Deviations from spherical symmetry, typical parameters of the spherical collapse model, and dark

分类：天文学 >> 星系和宇宙学提交时间： 2018-03-27

李希国

摘要：我们研究了由角动量和切向应力产生的偏离系统球对称性的方法。修正了球崩溃模型，作为非相对论成分(δc)及其病毒过密度(∆V)崩溃的线性密度阈值，在爱因斯坦-德西特和ΛCDM模型中。我们修改球面考虑切向

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12. ChinaXiv:201605.00850
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South Galactic Cap u-band Sky Survey (SCUSS): Data Release

分类：天文学 >> 星系和宇宙学提交时间： 2016-05-05

Hu Zou

摘要：The South Galactic Cap u-band Sky Survey (SCUSS) is a deep u-band imaging survey in the south

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点击量 3358 下载量 1787 评论 0

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