个人简介

舒新文，男，1982年生，安徽安庆人，理学博士，教授，理论物理硕士研究生导师。研究方向为黑洞及引力物理，高红移星系，X-射线、光学和太赫兹望远镜光谱和成像应用研究。中国科学院爱因斯坦探针卫星、X射线偏振卫星科学组成员。《MNRAS》,《RAA》,《天文学进展》等杂志审稿人。已在Nature,ApJS,ApJ,AJ,A&A等国际知名杂志上发表论文45篇，被引用1188次(NASA/ADS统计),SCIH-index16。主要学习和工作经历：2004.9-2010.6中国科学技术大学天文与应用物理系，硕士/博士2007.9-2009.7美国约翰霍普金斯大学联合培养博士2010.6-2012.4中国科学技术大学物理学院，博士后2012.4-2013.6中国科学技术大学副研究员2013.6-2015.3法国原子能中心，博士后2016.7-至今安徽师范大学，物理与电子信息学院教授

研究领域

黑洞及引力物理，高红移星系，X-射线、光学和太赫兹望远镜光谱和成像应用研究

1、黑洞及强引力场下的极端天体物理过程；检验广义相对论理论；2、利用引力透镜效应寻找和研究宇宙早期天体；3、多波段深场巡天数据的统计分析；4、X-射线、光学和太赫兹望远镜光谱和成像应用研究。

近期论文

1. Wang, T.; Schreiber, C.; Elbaz, D.; Yoshimura, Y.; Kohno, K.; Shu, X.;Yamaguchi, Y.; Pannella, M.; Franco, M.; Huang, J.; Lim, C. -F.; Wang, W. -H., A dominant population of optically invisible massive galaxies in the early Universe, Nature, 2019, 572, 211 (JCR一区)2. Liu, Bo ; Zhou, Hongyan*;Shu, Xinwen*;Zhang, Shaohua ;Ji, Tuo ;Pan, Xiang ;Jiang, Peng, Broad Emission and Absorption Line Outflows in the Quasar SDSS J163345.22+512748.4, The Astrophysical Journal, 2019, 879, 123 (JCR一区)3. Shu, X. W. ，Xue, Y. Q.; Liu, D. Z.; Wang, T.; Han, Y. K.; Chang, Y. Y.; Liu, T.;Huang, X. X.; Wang, J. X.; Zheng, X. Z.; et al., A unique distant submillimeter galaxy with an X-ray-obscured radio-luminous active galactic nucleus, Astronomy and Astrophysics, 2018, 619 , 76 (JCR二区)4. Shu, X. W. ，Wang, S. S.; Dou, L. M.; Jiang, N.; Wang, J. X.; Wang, T. G.，A LongDecay of X-Ray Flux and Spectral Evolution in the Supersoft Active Galactic Nucleus GSN 069，Astrophysical Journal Letters, 2018，857, 16-22 (JCR二区)5. Shu, X. W. ，Wang, T. G., Jiang, N., Wang, J. X., Sun, L. M., Zhou, H. Y.,CENTER ENGEINE AND HOST GALAXY OF RXJ1301.9+2747: A MULTI-WAVELENGTH VIEW OF A LOW-MASS BLACK HOLE ACTIVE GALACTIC NUCLEI WITH ULTRASOFT X-RAY EMISSION, Astrophysical Journal, 2017, 837, 3-18 (JCR二区).6. Shu, X. W. ，Elbaz, D.，Bourne, N.，Schreiber, C.，Wang, T.，et al. C.IDENTIFICATION OF z~>2 Herschel 500 MICRON SOURCES USING COLOR DECONFUSION，Astrophysical Journal Supplement Series，2016，222（1）：4-32 (JCR一区)。7. Shi, Xiheng，Zhou, Hongyan，Shu, Xinwen，Zhang, Shaohua，Ji, Tuo，Pan,Xiang，Sun, Luming，Zhao, Wen，Hao, Lei，BROAD BALMER ABSORPTION LINE VARIABILITY: EVIDENCE OF GAS TRANSVERSE MOTION IN THE QSO SDSS J125942.80+121312.6，The Astrophysical Journal，2016，819（2）：99-107 (JCR二区)。8. Zheng, Wei，Shu, Xinwen，Moustakas, John，Zitrin, Adi，Ford, Holland C.，Huang, Xingxing，Broadhurst, Tom，Molino, Alberto，Diego, Jose M.，Infante, Leopoldo，Bauer, Franz E.，Kelson, Daniel D.，Smit, Renske，YOUNG GALAXY CANDIDATES IN THE HUBBLE FRONTIER FIELDS. I. A2744，Astrophysical Journal，2014，795（1）：93-103 (JCR二区)。9. Zitrin, Adi，Zheng, Wei，Broadhurst, Tom，Moustakas, John，Lam, Daniel，Shu, Xinwen，Huang, Xingxing，Diego, Jose M.，et al.，A GEOMETRICALLY SUPPORTED z similar to 10 CANDIDATE MULTIPLY IMAGED BY THE HUBBLE FRONTIER FIELDS CLUSTER A2744，Astrophysical Journal Letters，2014，793（1）：L12-17 ((JCR二区，selected as NASA press release)。10. Sun, Luming，Shu, Xinwen，Wang, Tinggui，RX J1301.9+2747: A HIGHLYVARIABLE SEYFERT GALAXY WITH EXTREMELY SOFT X-RAY EMISSION，Astrophysical Journal，2013，768（2）：167-173 (JCR二区)。11. Coe, Dan，Zitrin, Adi，Carrasco, Mauricio，Shu, Xinwen，Zheng, Wei，Postman,Marc，et al.，CLASH: THREE STRONGLY LENSED IMAGES OF A CANDIDATE z approximate to 11 GALAXY，Astrophysical Journal，2013，762（1）：32-52 ((JCR二区，selected as NASA press release and one of 15 most important papers published by AAS in 2012-2015 )12. Zheng, Wei，Postman, Marc，Zitrin, Adi，Moustakas, John，Shu, Xinwen，Jouvel,Stephanie et al. A MAGNIFIED YOUNG GALAXY FROM ABOUT 500 MILLION YEARS AFTER THE BIG BANG，Nature，2012，489（7416）：406-408 (JCR一区，selected as NASA and ESA press release)。13. Shu, Xin-Wen，Wang, Jun-Xian，Liu, Teng，Zheng, Wei，THE X-RAYNATUREOF THE NUCLEUS IN SEYFERT 2 GALAXY NGC7590，Research in Astronomy and Astrophysics，2012，12（9）：1247-1254。14. Shu, X. W. ，Wang, J. X.，Yaqoob, T.，Jiang, P.，Zhou, Y. Y.，ON THE X-RAYBALDWIN EFFECT IN ACTIVE GALACTIC NUCLEI OBSERVED BY THE CHANDRA HIGH-ENERGY GRATING，Astrophysical Journal Letters，2012，744（2）：L21-26 (JCR二区)。15. Tan, Y. ，Wang, J. X.，Shu, X. W.，Zhou, Youyuan，A POSSIBLE ULTRASTRONG AND BROAD Fe K alpha EMISSION LINE IN SEYFERT 2 GALAXY IRAS 00521-7054，Astrophysical Journal Letters，2012，747（1）：L11-15 (JCR二区)。16. Shu, X. W. ，Yaqoob, T.，Wang, J. X.，CHANDRA HIGH-ENERGY GRATINGOBSERVATIONS OF THE Fe K alpha LINE CORE IN TYPE II SEYFERT GALAXIES: A COMPARISON WITH TYPE I NUCLEI，Astrophysical Journal，2011，738（2）：147-155 (JCR二区)。17. Jiang Peng，Wang JunXian，Shu XinWen，WEIGHING SUPER-MASSIVEBLACK HOLES WITH NARROW FE K ALPHA LINE，Science China Physics,Mechanics & Astonomy，2011，54（7）：1354-135818. Shu, X. W.，Liu, T.，Wang, J. X.，XMM-NEWTON OBSERVATIONS OF THESEYFERT 2 GALAXY NGC 7590: THE NATURE OF X-RAY ABSORPTION，Astrophysical Journal，2010，722（1）：96-101 (JCR二区)。19. Shu, X. W. ，Yaqoob, T.，Murphy, K. D.，Braito, V.，Wang, J.X.，Zheng, W.，NGC 2992 IN AN X-RAY HIGH STATE OBSERVED BY XMM- NEWTON: RESPONSE OF THE RELATIVISTIC Fe K alpha LINE TO THE CONTINUUM，Astrophysical Journal，2010，713（2）：1256-1265 (JCR二区)。20. Shu, X. W. ，Yaqoob, T.，Wang, J. X.，THE CORES OF THE Fe K alphaLINES IN ACTIVE GALACTIC NUCLEI: AN EXTENDED CHANDRA HIGH ENERGY GRATING SAMPLE，The Astrophysical Journal Supplement Series，2010，187（2）：581-606 (JCR一区)。21. Cai, Hong-Bing，Shu, Xin-Wen，Zheng, Zhen-Ya，Wang, Jun-Xian，THESTUDY OF SEYFERT 2 GALAXIES WITH AND WITHOUT INFRARED BROAD LINES，Research in Astronomy and Astrophysics，2010，10（5）：427-437。22. Overzier, Roderik A. , Shu, Xinwen，Zheng, Wei，Rettura, Alessandro，Zirm,Andrew，Bouwens, Rychard J.，Ford, Holland，Illingworth, Garth D.，Miley, George K.，Venemans, Bram，White, Richard L.，STELLAR MASSES OF LYMAN BREAK GALAXIES, LY ALPHA EMITTERS, AND RADIO GALAXIES IN OVERDENSE REGIONS AT z=4-6，Astrophysical Journal，2009，704（1）：548-563 (JCR二区)。23. Shu, Xin-Wen，Wang, Jun-Xian，Jiang, Peng，ARE SYEFERT 2 GALAXIESWITHOUT POLARIZED BROAD EMISSION LINES MORE OBSCURED?，Chinese Journal of Astronomy and Astrophysics，2008，8（2）：204-210。24. Shu, X. W. ，Wang, J. X.，Jiang, P.，Fan, L. L.，Wang, T. G.，INVESTIGATING THE NUCLEAR OBSCURATION IN TWO TYPES SEYFERT 2 GALAXIES，Astrophysical Journal，2007，657（1）：167-176 (JCR二区)。