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HFW: Postdoctoral Fellow of Yunnan University (2018-present), LAMOST Fellow of Chinese Academy of Sciences (2018-present), Ph.D in Astrophysics of National Astronomical Observatories, Chinese Academy of Sciences (2013-2018).

 

Research Interests: Chemo-Dynamical Structures of the Milky Way, Near-Field Cosmology, Connection between multiple populations of star cluster and Its host galaxies, Astronomical big data reduction and analysis, and etc.

Contact: (+86) 17380084576, hfwang@bao.ac.cn, orcid: 0000-0001-8459-1036

DOB: 1990.09, Born in Sichuan, China West

WORK EXPERIENCE

LAMOST Fellow, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100101,

P.R.China, 2018.7-present

Post−doc, South−Western Institute for Astronomy Research, Yunnan University, Kunming, 650500, P.R.China, 2018.7-present

Post−doc, School of Information, Yunnan University, Kunming, 650500, P.R.China, 2018.7-present 

PROJECTS&SPONSORSHIPS

Principal Investigator:

LAMOST Fellow initial funding, National Astronomical Observatories, Chinese Academy of Sciences; 50000 RMB∼7100 Dollars∼6400 Euros, 2018

 

China Postdoctoral Science General Foundation, Ministry of Human Resources and Social Security of

the People’s Republic of China; 80000 RMB, 2019

 

LAMOST Fellow Assessment rewards, Center for Astronomical Mega−Science, Chinese Academy of Sciences; 80000 RMB, 2019

 

Yunnan province postdoctoral Directed culture foundation, Department of Human Resources

and Social Security of Yunnan Province, China; 160000 RMB, 2019

 

LAMOST Scientific Payoff and Research Achievement Cultivation projects funding, National Astronomical Observatories, Chinese Academy of Sciences; 50000 RMB, 2019

China Postdoctoral Science Special Foundation, Ministry of Human Resources and Social Security of

the People’s Republic of China; 180000 RMB, 2020

LAMOST Scientific Payoff and Research Achievement Cultivation projects funding, Center for Astronomical Mega−Science, Chinese Academy of Sciences; 60000 RMB, 2020

Youth Program of National Natural Science Foundation of China; 240000 RMB, 2020

 

Outstanding achievement award of post-doc (Third prize), Department of Human Resources and Social Security of Yunnan Province, China; 10000 RMB, 2020

LAMOST Fellow Assessment rewards, Center for Astronomical Mega−Science, Chinese Academy of Sciences; 90000 RMB, 2020

Participant:

National Key Basic Research Program of China, Ministry of Science and Technology of China;

29.33 million RMB (180000 RMB for me), 2019

RESEARCH FIELDS

1. Milky Way Chemo-Dynamical Structures

 

2. Near−Field Cosmology and Low-z disk galaxy

3. Star Cluster Multiple Populations


4. Time domain stellar astronomy 


5. Large Sky surveys and Astronomical statistics

MEMBERSHIP&MEMBER 

Membership of China Astronomical Society

Junior Member of International Astronomical Union 

Member of LengHu observatory


Member of CSST(China Space Station Telescope)Near-Field cosmology 

SUPERVISING(CO-SUPERVISING) STUDENTS

Liqing(Master, 2019), Liqida(Master, 2019), Lixiang(Master, 2020), Yangpeng(Master, 2020)

 

Sunweixiang(Master)

PUBLIC OUTREACH

China West Normal University, Nanchong in China, Learning Our Milky Way, 2019

 

Guizhou University, Guiyang in China, What do we know about Our Milky Way, 2019

High School of Yaan-Chengdu experimental foreign languages, Yaan in China, Learning Our Milky Way, 2020

Awards&Honors

Outstanding graduates of Sichuan Province, China; 2013

Nubian scholarship of National Astronomical Observatories of Chinese Academy of Sciences, China; 2018 

Outstanding achievement award of post-doc (Third prize) of Yunnan Province, China; 2020

SELECTED PUBLICATIONS

Full publications: https://ui.adsabs.harvard.edu/publiclibraries/

1. Wang H.-F., et al., 3D Asymmetrical motions of the Galactic outer disc with LAMOST K giant

stars, 2018a, MNRAS, 477, 2858

2. Wang H.-F., et al., Mapping the Milky Way with LAMOST- III. Complicated spatial structure in the outer disc, 2018b, MNRAS, 478, 3367

3. Wang H.-F., et al., The Spatial Structure of the Galactic outer disk with LAMOST DR3 K giant stars, 2018c, in C. Chiappini, I. Minchev, E. Starkenberg, M. Valentini, eds., proc. IAU Symposium 334: Rediscovering our Galaxy, Cambridge Univ. Press, Cambridge, p. 378

4. Wang H.-F., et al., Mapping the Galactic disk with the LAMOST and Gaia Red clump sample. III. A new velocity substructure and time stamps of the Galactic disk asymmetry in the disk between 12−15 kpc, 2019, APJ, 884, 135

5. Wang H.-F., et al., Mapping the Galactic disk with the LAMOST and Gaia Red clump sample. II. 3D asymmetrical kinematics of mono-age populations in the disk between 6−14 kpc, 2020a, MNRAS, 491, 2104

6. Wang H.-F., et al., 3D asymmetrical kinematics of mono-age populations from LAMOST and Gaia common red clump stars, 2020b, in J. Shen, M. Valluri, & J. A. Sellwood, eds., proc. IAU Symposium 353: Galactic Dynamics in the Era of Large Surveys, Cambridge Univ. Press, Cambridge, p. 19

7. Wang H.-F., et al., Mapping the Galactic disk with the LAMOST and Gaia Red clump sample. VI. Evidence for the long lived Nonsteady warp of Nongravitational scenarios, 2020c, APJ,  897, 119

8. Wang H.-F., et al., Diagonal Ridge pattern of different age populations found in Gaia DR2 with LAMOST Main-Sequence-Turn-Off and OB type Stars, 2020d, APJ, 902, 70

9. Sun W.-X., *Huang Y., *Wang H.-F., et al., Mapping the Galactic disk with the LAMOST and Gaia Red clump sample. IV. On the origin of the “young [α/Fe]” enhanced stars, 2020, 903, 12

10. Liu, C., Xu Y., Wang H.-F., et al., Rediscovering the Galactic outer disk with LAMOST data, 2018, in C. Chiappini, I. Minchev, E. Starkenberg, M. Valentini, eds., proc. IAU Symposium 334: Rediscovering our Galaxy, Cambridge Univ. Press, Cambridge, p. 109

11. López-Corredoira, M., Garzón, F.,Wang H.-F., et al., Gaia-DR2 extended kinematical maps Part II: Dynamics in the Galactic disk explaining radial and vertical velocities, 2020, A&A, 634, A66

12. Chrobáková, Ž, López-Corredoira, M., Sylos Labini, F., Wang H.-F., et al., Gaia-DR2 extended kinematical maps Part III: Rotation curves analysis, dark matter, and Modified Newtonian dynamics tests, 2020, A&A, 642, A95

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