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舒新文

作者:王亚青 时间:2016-03-10 点击数: 审核者:王亚青

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-index 16。

联系方式:xwshu@ mail.ahnu.edu.cn

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

研究领域和方向:

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。

讲授课程:

《理论力学》,《普通物理续论》,《概率论与数理统计》,《大学物理》

获奖情况:

2004:安徽省优秀毕业生

2006:中国科技大学光华奖学金

2007:中国航天科技集团奖学金

2010:中国科学院院长奖学金

2011:中国科学院优秀博士学位论文

2012:全国百篇优秀博士学位论文题名论文

2013:安徽省自然科学优秀学术论文一等奖

2016:安徽师范大学青年教师教学基本功大赛一等奖

承担科研项目:

(1)国家自然科学基金面上项目(11573001),赫歇尔深度巡天中高红移500微米源的多波段研究(2016.1-2019.12),主持

(2)国家基础研究计划973项目(2015CB857005),暗能量观测:基于大规模红移巡天的精确测量宇宙膨胀历史和结构增长率(2015.1-2019.12),学术骨干

(3)国家自然科学基金重点项目(11233002),大质量黑洞的活动和演化(2013.1- 2017.12),子课题负责人

(4)安徽省自然科学基金(1608085QA06),活动星系特殊X射线辐射及相关极端天体物理过程的研究(2016.7-2018.6),主持

(5)中国科学院空间天文与技术重点实验室开放课题(KLSAT201601),极软X射线辐射活动星系核的黑洞吸积模式和辐射机制探索(2016.5-2017.5),主持

(6)国家自然科学基金青年项目(11103017),活动星系核核区遮蔽和高分辨率窄铁Ka荧光发射线的研究(2012.1-2014.12),主持

(7)中国博士后基金特别资助(201104332),活动星系核核区遮蔽和尘埃环X射线波段的研究, 2011.9-2012.9,主持

(8)中国博士后基金一等资助(20100480046),利用Chandra高能光栅研究活动星系核窄铁Ka荧光发射线, 2010.12-2012.6,主持

教学论文:

1.舒新文,许新胜,姚关心,侯长健,一种绳约束两质点的运动的研究,《大学物理》,2017,inpress.

主要学术论文:

1. 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, in press (JCR二区).

2. 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)。

3. 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)。

4. Zhang, Shaohua,Zhou, Hongyan,Shi, Xiheng,Shu, Xinwen,Liu, Wenjuan,

Ji, Tuo,Jiang, Peng,Sun, Luming,Zhou, Junyan,Pan, Xiang,DISCOVERYOF EXTREMELY BROAD BALMER ABSORPTION LINES IN SDSS J152350.42+391405.2,Astrophysical Journal,2015,815(2):113-123 (JCR二区)。

5. 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)。

6. 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)。

7. Sun, Luming,Shu, Xinwen,Wang, Tinggui,RX J1301.9+2747: A HIGHLY

VARIABLE SEYFERT GALAXY WITH EXTREMELY SOFT X-RAY EMISSION,Astrophysical Journal,2013,768(2):167-173 (JCR二区)。

8. Jiang, Peng,Zhou, Hongyan,Ji, Tuo,Shu, Xinwen,Liu, Wenjuan,Wang,

Jianguo,Dong, Xiaobo,Bai, Jinming,Wang, Huiyuan,Wang, Tinggui,ANOMALOUSLY STEEP REDDENING LAW IN QUASARS: AN EXCEPTIONAL EXAMPLE OBSERVED IN IRAS 14026+4341,Astronomical Journal,2013,145(6):157-165。

9. 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 )

10. 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)。

11. Shu, Xin-Wen,Wang, Jun-Xian,Liu, Teng,Zheng, Wei,THE X-RAYNATURE

OF THE NUCLEUS IN SEYFERT 2 GALAXY NGC7590,Research in Astronomy and Astrophysics,2012,12(9):1247-1254。

12. Shu, X. W.,Wang, J. X.,Yaqoob, T.,Jiang, P.,Zhou, Y. Y.,ON THE X-RAY

BALDWIN EFFECT IN ACTIVE GALACTIC NUCLEI OBSERVED BY THE CHANDRA HIGH-ENERGY GRATING,Astrophysical Journal Letters,2012,744(2):L21-26 (JCR二区)。

13. Tan, Y. ,Wang, J. X.,Shu, X. W.,Zhou, Youyuan,A POSSIBLE ULTRA

STRONG 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)。

14. Shu, X. W.,Yaqoob, T.,Wang, J. X.,CHANDRA HIGH-ENERGY GRATING

OBSERVATIONS 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)。

15. Jiang Peng,Wang JunXian,Shu XinWen,WEIGHING SUPER-MASSIVE

BLACK HOLES WITH NARROW FE K ALPHA LINE,Science China Physics,Mechanics & Astonomy,2011,54(7):1354-1358

16. Shu, X. W.,Liu, T.,Wang, J. X.,XMM-NEWTON OBSERVATIONS OF THE

SEYFERT 2 GALAXY NGC 7590: THE NATURE OF X-RAY ABSORPTION,Astrophysical Journal,2010,722(1):96-101 (JCR二区)。

17. 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)。

18. Shu, X. W.,Yaqoob, T.,Wang, J. X.,THE CORES OF THE Fe K alpha

LINES IN ACTIVE GALACTIC NUCLEI: AN EXTENDED CHANDRA HIGH ENERGY GRATING SAMPLE,Astrophysical Journal, The – Supplement Series,2010,187(2):581-606 (JCR一区)。

19. Cai, Hong-Bing,Shu, Xin-Wen,Zheng, Zhen-Ya,Wang, Jun-Xian,THE

STUDY OF SEYFERT 2 GALAXIES WITH AND WITHOUT INFRARED BROAD LINES,Research in Astronomy and Astrophysics,2010,10(5):427-437。

20. 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)。

21. Shu, Xin-Wen,Wang, Jun-Xian,Jiang, Peng,ARE SYEFERT 2 GALAXIES

WITHOUT POLARIZED BROAD EMISSION LINES MORE OBSCURED?,Chinese Journal of Astronomy and Astrophysics,2008,8(2):204-210。

22. 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)。

For more publications please see

http://adsabs.harvard.edu/cgi-bin/nph-abs_connect?library&libname=adspaper&libid=5767b61d43

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