{"id":2,"date":"2009-10-06T19:50:52","date_gmt":"2009-10-06T11:50:52","guid":{"rendered":"http:\/\/astronomy.lamost.org\/blog\/?page_id=2"},"modified":"2024-06-12T16:56:01","modified_gmt":"2024-06-12T14:56:01","slug":"%e5%85%b3%e4%ba%8e","status":"publish","type":"page","link":"http:\/\/astronomy.lamost.org\/blog\/?page_id=2","title":{"rendered":"about me"},"content":{"rendered":"

Fan XiLong \u8303\u9521\u9f99<\/a><\/p>\n

Wuhan University <\/a><\/p>\n

LIGO@Tsinghua<\/a><\/p>\n

University of Glasgow<\/a>\u00a0 \u00a0Newton International Fellowships<\/a><\/p>\n

Research\u300b gravitational wave<\/a> \uff0c galaxy evolution<\/a> by\u00a0Galactic\u00a0Chemical Evolution<\/a> model<\/a> and SED evolution model<\/a><\/p>\n

My current work focus on mutil-messenger (GW-EM) astrophysics and cosmology [13,29].\u00a0 With the help of EM data (such as galaxy catalog) and GW-EM theoretical prediction (such GW-GRB relation), I try to improve the gravitational waves signals detection with the LIGO\uff0dVirgo\u00a0 instruments. In particular\uff0c I work on a Bayesian\u00a0 approach to multi-messenger astronomy, with special interest on GW-EM source\u00a0 sky localization\uff0c GW parameter estimation\u00a0 [8,9]\u00a0 and EM counterpart properties\u00a0 [15,24].<\/p>\n

I have spent 3 years understanding the EM data during\u00a0 my Ph.D\u00a0 phase, in particular galaxy properties by galactic chemical and SED models [ 4,5,6]. Before that,\u00a0 I spent 3 years\u00a0 understanding GW research during\u00a0 my Master degreed phase.<\/p>\n

I also work on GW burst sky localization [2],\u00a0 stochastic\u00a0 GW background detection [1,3,19,21,32,38, 39] ,\u00a0 continuous GW detection ([ 10,22]) ,GW echo [28] , EMRIs or IMRIs[20], GW waveform [34].<\/p>\n

To help students building their own research, I contribute myself to\u00a0 the research of\u00a0 GRB offset [7].<\/p>\n

Very recently,\u00a0 I am\u00a0 also \u00a0interested in the\u00a0 lensed\u00a0 GW-EM system and\u00a0 their applications\u00a0 on\u00a0 fundamental questions (e.g. the speed of GW [12] , the wave nature of GW [23 ,27\uff0c31] , the\u00a0 Hubble constant [14,42] cosmic curvature [16, 25], dark matter substructure [25] ) and astrophysics questions (e.g. measuring\u00a0 the mass of\u00a0 lens [33,35] ).\u00a0 \u00a0You could get an idea of those work in my review [43], except for lensed event rate [40,41]<\/p>\n

The machine learning approach [17,18] is on the way of rewriting\u00a0 all my work………….\u6df1\u6df1\u7684\ud83d\ude31<\/p>\n

Publication<\/a>\uff08ads\u6301\u7eed\u66f4\u65b0\uff09<\/p>\n

1. Fan,\u00a0Xi-Long<\/span>; Zhu,\u00a0Zong-Hong,\u00a0 The optimal approach of detecting stochastic gravitational wave from string cosmology using multiple detectors, 2008PhLB..663…17F<\/a><\/p>\n

2. Wen,\u00a0L.; Fan,\u00a0X.<\/span>; Chen,\u00a0Y., Geometrical expression of the angular resolution of a network of gravitational-wave detectors and improved localization methods, 2008JPhCS.122a2038W<\/a><\/p>\n

3.\u00a0 Zhu,\u00a0Xing-Jiang; Fan,\u00a0Xi-Long<\/span>; Zhu,\u00a0Zong-Hong, Stochastic Gravitational Wave Background from Neutron Star r-mode Instability Revisited,2011ApJ…729…59Z
\n<\/a>
\n4.\u00a0 Fan,\u00a0X.\u00a0L.<\/span>; Yin,\u00a0J.; Matteucci,\u00a0F., The nature of long-GRB host galaxies from chemical abundances, 2010A&A…521A..73F<\/a><\/p>\n

5. Pipino,\u00a0A.; Fan,\u00a0X.\u00a0L.<\/span>; Matteucci,\u00a0F.; Calura,\u00a0F.; Silva,\u00a0L.; Granato,\u00a0G.; Maiolino,\u00a0R., The chemical evolution of elliptical galaxies with stellar and QSO dust production,2011A&A…525A..61P<\/a><\/p>\n

6.\u00a0 Fan,\u00a0X.\u00a0L.<\/span>; Pipino,\u00a0A.; Matteucci,\u00a0F., The Dust Properties of z ~ 3 MIPS-LBGs from Photochemical Models, 2013ApJ…768..178F<\/a><\/p>\n

7. C. Boylan, Y. Li, X.L. Fan<\/span>, I.S. Heng, Short gamma ray bursts: formation and offsets,\u00a0 arxiv:1401.7851<\/a><\/p>\n

8. Fan,\u00a0XiLong<\/span>; Messenger,\u00a0Christopher; Heng,\u00a0Ik\u00a0Siong, A Bayesian approach to multi-messenger astronomy: Identification of gravitational-wave host galaxies, http:\/\/adsabs.harvard.edu\/abs\/2014ApJ…795…43F<\/a><\/p>\n

9. Fan,\u00a0Xilong<\/span>; Messenger,\u00a0Christopher; Heng,\u00a0Ik\u00a0Siong, Enhancing gravitational wave astronomy with galaxy catalogues, 2014arXiv1406.2151F<\/a><\/p>\n

10.\u00a0\u00a0 Fan, Xilong; Chen, Yanbei; Messenger, Christopher<\/span><\/span>\uff0c Method to detect gravitational waves from an ensemble of known pulsars\uff0c https:\/\/arxiv.org\/abs\/1607.06735<\/a><\/p>\n

11. Fan, Xilong<\/span>\uff0c The detection of gravitational waves and the new era of multi-messenger astronomy\uff0c http:\/\/phys.scichina.com:8083\/sciGe\/CN\/abstract\/abstract510225.shtml<\/a><\/p>\n

12. Fan, Xilong<\/span>\uff0cKai Liao, Marek Biesiada\uff0cAleksandra Piorkowska-Kurpas, and ZhongHong Zhu\uff0c The speed of gravitational waves from strong lensed gravitational wave-electromagnetic signals \uff0c\u00a0 https:\/\/arxiv.org\/abs\/1612.04095<\/a><\/p>\n

13 , XiLong Fan<\/span>, Martin Hendry\uff0c Multimessenger astronomy \uff0c https:\/\/arxiv.org\/abs\/1509.06022<\/a><\/p>\n

14,\u00a0 Kai Liao, Xi-Long Fan,<\/span> Xu-Heng Ding, Marek Biesiada, Zong-Hong Zhu\uff0c Precision Cosmology from Future Time Delays of Lensed Gravitational Wave and Electromagnetic Signals\uff0c https:\/\/arxiv.org\/abs\/1703.04151<\/a><\/p>\n

15\uff0cXilong Fan<\/span>, Christopher Messenger, Ik Siong Heng\uff0c \u00a0 Probing intrinsic properties of short gamma-ray bursts with gravitational waves\u00a0 http:\/\/adsabs.harvard.edu\/abs\/2017PhRvL.119r1102F<\/a><\/p>\n

16, Kai Liao, Zhengxiang Li, Guo-Jian Wang, Xi-Long Fan\uff0c<\/span> Test of the FLRW metric and curvature with strong lens time delays\uff0c https:\/\/arxiv.org\/abs\/1704.04329<\/a><\/p>\n

17 Xilong Fan<\/span>, Jin Li* ,Xin Li, Yuanhong Zhong, Cao Junwei , “Applying deep neural networks to the detection and space parameter estimation of compact binary coalescence with a network of gravitational wave detectors\u201d, LIGO Document P1700289, 2017 arxiv.org\/abs\/1811.01380<\/a><\/p>\n

18, Xiangru Li*, Woliang Yu,and Xilong Fan*, <\/span>\u201cA Method Of Detecting Gravitational Wave Based On Time-frequency Analysis And Convolutional Neural Networks, LIGO Document P1700391, https:\/\/arxiv.org\/abs\/1712.00356<\/a> \uff0c2017<\/p>\n

19,Wei-Wei Tan, Xi-Long Fan<\/span>, F. Y. Wang, “Short Gamma-Ray Bursts and Gravitational-Wave Observations from Eccentric Compact Binaries” , arXiv:1712.04641, 2017<\/a><\/p>\n

20 , Wen-Biao Han\uff0cXi-Long Fan*<\/span>\uff0c\u201cOn the equations of states of white dwarfs from low-frequency gravitational waves\u201d, arXiv:1711.08628<\/a>,\u00a0 2017<\/p>\n

21, Fan, Xilong*<\/span>; Chen, Yanbei \u201cStochastic gravitational-wave background from spin loss of black holes\u201d, ligo dcc LIGO P1700409-v1<\/a>, http:\/\/arxiv.org\/abs\/1712.00784<\/a> , 2017<\/p>\n

22, M. Pitkin*, C. Messenger*, X. Fan*<\/span>, A hierarchical Bayesian method for detecting continuous gravitational waves from an ensemble of pulsars,https:\/\/arxiv.org\/abs\/1807.06726<\/a><\/p>\n

23\u00a0 Zhang Hongsheng, Fan Xilong*, Poisson-Arago spot for gravitational waves, http:\/\/export.arxiv.org\/abs\/1809.06511<\/a><\/span><\/span><\/p>\n

24\u00a0B.-B. Zhang, B. Zhang, H. Sun, W.-H. Lei, H. Gao, Y. Li, L. Shao, Y. Zhao, Y.-D. Hu, H.-J. L\u00fc, X.-F. Wu, X.-L. Fan<\/span>, G. Wang, A. J. Castro-Tirado, S. Zhang, B.-Y. Yu, Y.-Y. Cao, E.-W. Liang,\u00a0 A peculiar low-luminosity short gamma-ray burst from a double neutron star merger progenitor,\u00a0 https:\/\/www.nature.com\/articles\/s41467-018-02847-3<\/a><\/p>\n

25\u00a0 Kai Liao, Xuheng Ding, Marek Biesiada, Xi-Long Fan<\/span>, Zong-Hong Zhu,\u00a0 Anomalies in Time Delays of Lensed Gravitational Waves and Dark Matter Substructures,\u00a0 https:\/\/arxiv.org\/abs\/1809.07079\uff0c\u00a02018, ApJ, 867, 69<\/a><\/p>\n

26\u00a0 Yufeng Li<\/span>, Xilong Fan*<\/span>, and Lijun Gou\uff0cConstraining Cosmological Parameters in the FLRW Metric with Lensed GW+EM Signals\uff0c The Astrophysical Journal<\/a><\/span>, Volume 873<\/a><\/span>, Number 1<\/a><\/span>., https:\/\/arxiv.org\/abs\/1901.10638v1<\/a>
\n<\/span><\/p>\n

27 Kai Liao, Marek Biesiada, Xi-Long Fan* , The wave nature of continuous gravitational waves from microlensing, https:\/\/arxiv.org\/abs\/1903.06612<\/a><\/span><\/span><\/p>\n

28 Kai Lin, Wei-Liang Qian, Xilong Fan<\/span>, Hongsheng Zhang\uff0c Tail wavelets in the merger of binary compact objects\uff0c https:\/\/arxiv.org\/abs\/1903.09039<\/a><\/p>\n

https:\/\/doi.org\/10.1088\/1674-1137\/44\/7\/071001<\/a><\/p>\n

29 B.S. Sathyaprakash, Enis Belgacem , Daniele Bertacca (Universita degli Studi di Padova), Chiara Caprini , Giulia Cusin , Yves Dirian , Xilong Fan<\/span> ,Daniel Figueroa, Stefano Foffa , Evan Hall , Jan Harms , Michele Maggiore , Vuk Mandic , Andrew Matas, Tania Regimbau, Mairi Sakellariadou , Nicola Tamanini , Eric Thrane ,Cosmology and the Early Universe ,\u00a0https:\/\/arxiv.org\/abs\/1903.09260<\/a><\/p>\n

30 Cheng, Quan; Zhang, Shuang-Nan; Zheng, Xiao-Ping; Fan, Xi-Long, <\/span>What can PSR J1640-4631 tell us about the internal physics of this neutron star?\u00a0 http:\/\/adsabs.harvard.edu\/abs\/2019arXiv190406570C<\/a><\/p>\n

31\u00a0 Hou, Shaoqi; Fan, Xi-Long*<\/span>; Zhu, Zong-Hong\uff0c Gravitational lensing of gravitational waves: Rotation of polarization plane\uff0c10.1103\/PhysRevD.100.064028<\/a><\/p>\n

32\u00a0 Yufeng Li, Xilong Fan*<\/span>, Lijun Gou\uff0c Constraining the stochastic gravitational wave from string cosmology with current and future high frequency detectors\uff0c https:\/\/arxiv.org\/abs\/1910.0831<\/a><\/p>\n

33. Dongze Sun, Xilong Fan*<\/span>, Pattern of lensed chirp gravitational wave signal and its implication on the mass and position of lens\u00a0 https:\/\/arxiv.org\/abs\/1911.08268<\/a><\/p>\n

34 Shaoqi Hou, Xi-Long Fan*<\/span>, Zong-Hong Zhu, Corrections to the gravitational wave phasing, https:\/\/arxiv.org\/abs\/1911.04182<\/a><\/p>\n

35 Shaoqi Hou, Xi-Long Fan*<\/span>, Kai Liao, Zong-Hong Zhu, Gravitational Wave Interference via Gravitational Lensing: Measurements of Luminosity Distance, Lens Mass, and Cosmological Parameters, https:\/\/arxiv.org\/abs\/1911.02798<\/a><\/p>\n

36 Eda Gjergo<\/a>,<\/span><\/span>\u00a0Marco Palla<\/a>,<\/span><\/span>\u00a0Francesca Matteucci<\/a>,<\/span><\/span>\u00a0Elena Lacchin<\/a>,<\/span><\/span>\u00a0Andrea Biviano<\/a>,<\/span><\/span>\u00a0Xilong Fan<\/a> \uff0c <\/span>On the origin of dust in galaxy clusters at low-to-intermediate redshift\uff0c https:\/\/doi.org\/10.1093\/mnras\/staa431<\/a><\/p>\n

37\u00a0 M. Palla ,\u00a0 F. Calura , F. Matteucci, X. L. Fan<\/span> ,\u00a0 F. Vincenzo and E. Lacchin\uff0c The influence of a top-heavy integrated galactic IMF and dust on the
\nchemical evolution of high-redshift starbursts\uff0chttps:\/\/doi.org\/10.1093\/mnras\/staa848<\/a><\/p>\n

38\u00a0 Hongguang Zhang, Xilong Fan*<\/span>, Yufeng Li, Minglei Tong, Hongsheng Zhang,\u00a0 String length constraining from stochastic gravitational waves background\u00a0https:\/\/arxiv.org\/abs\/2105.05027<\/a><\/p>\n

39 Hongguang Zhang, Xilong Fan*<\/span>, Yihui Lai, Gravitons probing from stochastic gravitational waves background,\u00a0https:\/\/arxiv.org\/abs\/2105.05083<\/a><\/p>\n

40 Aleksandra Pi\u00f3rkowska-Kurpas, Shaoqi Hou, Marek Biesiada, Xuheng Ding, Shuo Cao, Xilong Fan<\/span>, Seiji Kawamura, Zong-Hong Zhu,\u00a0 Inspiraling Double Compact Object Detection and Lensing Rate: Forecast for DECIGO<\/p>\n

and B-DECIGO,http:\/\/10.3847\/1538-4357\/abd482<\/a><\/p>\n

41 Shaoqi Hou (\u4faf\u7ecd\u9f50), Pengbo Li (\u674e\u9e4f\u535a), Hai Yu (\u4f59\u6d77), Marek Biesiada, Xi-Long Fan (\u8303\u9521\u9f99)<\/span>, Seiji Kawamura, and Zong-Hong Zhu (\u6731\u5b97\u5b8f), Lensing rates of gravitational wave signals displaying beat patterns detectable by DECIGO and B-DECIGO,\u00a0https:\/\/journals.aps.org\/prd\/abstract\/10.1103\/PhysRevD.103.044005<\/a><\/p>\n

42. Shaoqi Hou ,Xi-Long Fan*<\/span> and Zong-Hong Zhu, Constraining cosmological parameters from strong lensing with DECIGO and B-DECIGO sources,\u00a0http:\/\/10.1093\/mnras\/stab2221<\/a><\/p>\n

43 \u8303\u9521\u9f99*<\/span>\uff0c \u900f\u955c\u5316\u5f15\u529b\u6ce2\u7684\u6563\u5c04\u95ee\u9898\u53ca\u5176\u5e94\u7528,\u00a0 https:\/\/www.sciengine.com\/publisher\/scp\/journal\/CSB\/66\/20\/10.1360\/TB-2020-1170?slug=fulltext<\/a><\/p>\n

44\u00a0 Zhuotao Li, Xilong Fan*<\/span>\u00a0<\/span>and Gang Yu., Reconstruction of Supernova Gravitational Waves Waveforms: Comparing Three Time-frequency, Transform Methods,\u00a0https:\/\/arxiv.org\/abs\/2010.14409<\/a><\/p>\n

\u79d1\u666e<\/p>\n

\u91cf\u5b50\u529b\u5b66\u4e0e\u76f8\u5bf9\u8bba\u7fe9\u7fe9\u8d77\u821e, \u79d1\u5b66\u5bb6\u5728\u5b87\u5b99\u91d1\u77ff\u6316\u8bba\u6587\u91d1\u77ff | \u5f15\u529b\u6ce2\u91cd\u78c5<\/a>\u00a0 \u77e5\u793e\uff0c\u4f5c\u8005\uff1a\u9648\u96c1\u5317\uff0c \u8303\u9521\u9f99<\/h4>\n

\u9648\u96c1\u5317\u3001\u8303\u9521\u9f99\uff1a\u7231\u56e0\u65af\u5766\u90fd\u4e0d\u6562\u60f3\u8c61\uff0c\u6211\u4eec\u771f\u7684\u63a2\u6d4b\u5230\u5f15\u529b\u6ce2\uff01\u00a0\u00a0<\/a>\u77e5\u793e\uff0c\u4f5c\u8005\uff1a\u9648\u96c1\u5317\uff0c \u8303\u9521\u9f99<\/h4>\n

\u6253\u5f00\u5b87\u5b99\u65f6\u7a7a\u5f2f\u66f2\u7684\u5927\u95e8<\/a>\uff0c \u300a\u4eba\u6c11\u65e5\u62a5\u300b\u00a0 \u4f5c\u8005\uff1a \u6731\u5b97\u5b8f\uff0c\u8303\u9521\u9f99<\/h4>\n

\u6df1\u5ea6\u89e3\u8bfb\u4eba\u7c7b\u9996\u6b21\u76f4\u63a5\u63a2\u6d4b\u5230\u5f15\u529b\u6ce2\u4e8b\u4ef6<\/a>\uff0c \u817e\u8baf\u7f51\uff0c\u4f5c\u8005\uff1a\u660e\u955c\uff0c\u8303\u9521\u9f99<\/p>\n

\u53cc\u9ed1\u6d1e, \u4f60\u4eec\u597d: \u4eba\u7c7b\u518d\u6b21\u63a2\u6d4b\u5230\u5f15\u529b\u6ce2!<\/a>\u00a0\u00a0 \u77e5\u793e\uff0c \u4f5c\u8005\uff1a\u8303\u9521\u9f99<\/h4>\n

\u53c8\u201c\u542c\u201d\u9ed1\u6d1e\u5e76\u5408\uff0c\u201c\u7334\u5e74\u9a6c\u6708\u201d\u5e76\u4e0d\u9065\u8fdc <\/a>\u300a\u79d1\u6280\u65e5\u62a5\u300b 2016-06-16 01\u7248<\/h4>\n

My review-style talks:<\/h3>\n