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Name: Fangxia An Gender:
Highest Education: Ph.D. Academic Title: Associate Professor
Subject Categories: Astrophysics Research Field:

Galaxies formation and evolution, galaxy cluster/proto-cluster, and the large-scale structures of galaxies


Email: Phone:
Fax: Postal Code: 650011
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CV:
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Title: “Preparing for the Square Kilometre Array (SKA): Studies of formation and evolution of galaxies and galaxy clusters by using high-quality radio data from the precursors of the SKA”Funder: National Science Foundation of China (NSFC)Role: Principal Investigator Duration: January 2024 – December 2026

Title: “Exploring the Cosmic Star Formation History Using Precursors of the Square Kilometre Array”Funder: Applied Basic Research Programs of Science and Technology Commission Foundation of Jiangsu Province Role: Principal InvestigatorDuration: September 2024 August 2027

Articles:

1. An, F.~X., Vaccari M.; Best P.~N., Ocran E.~F., Ishwara-Chandra C.~H., Taylor A.~R., Leslie S.~K.; et al., 2024, “Radio spectral properties of star-forming galaxies between 150 and 5000 MHz in the ELAIS-N1 field”, MNRAS, 528(3), 5346-5363. doi:10.1093/mnras/stae364

2. Wen, R., An, F.~X., Zheng, X.~Z., Shi D.~D., Qin J., Gonzalez V., Bian F., et al. 2022, “The Physical Properties of Star-Forming Galaxies with Strong [OIII] Lines at z=3.25”, ApJ, 933, 50. doi:10.3847/1538-4357/ac7392

3. An, F.~X., M. Vaccari, Ian Smail, Jarvis M.~J., Whittam I.~H., Hale C.~L., Jin S., et al. 2021, “Radio spectral properties of star-forming galaxies in the MIGHTEE-COSMOS field and their impact on the far-infrared-radio correlation”, MNRAS, 507(2): 2643-2658. doi:10.1093/mnras/stab2290

4. Zheng, X.~Z., Cai, Z., An, F.~X., Fan X., Shi D.~D., et al. 2021, “MAMMOTH: confirmation of two massive galaxy overdensities at z = 2.24 with Hα emitters”, MNRAS, 500, 4354. doi:10.1093/mnras/staa2882

5. An, F.~X., Simpson, J. M., Small, I., Swinbank A.~M., Ma C., Liu D., Lang P., et al., 2019, “Multi-wavelength properties of radio and machine-learning identified counterparts of submillimeter sources from S2COSMOS”, ApJ, 886, 48. doi:10.3847/1538-4357/ab4d53

6. An, F.~X., Stach, S. M., Small, I., Swinbank A.~M., Almaini O., Simpson C., Hartley W., et al. 2018, “A machine-learning method for identifying multi-wavelength counterparts of submillimeter galaxies: training and testing using AS2UDS and ALESS”, ApJ, 862, 101. doi:10.3847/1538-4357/835/2/116

7. An, F.~X., Zheng, X.~Z., Hao, C.-N., Huang J.-S., Xia X.-Y., 2017, “ Extinction Correction Significantly Influences the Estimate of the Ly-alpha Escape Fraction”, ApJ 835, 116. doi:10.3847/1538-4357/835/2/116

8. An, F.~X., Zheng, X.~Z., Wang, W.-H., Huang J.-S., Kong X., Wang J.-X., Fang G.~W., et al., 2014, “The properties of Hα emission-line galaxies at z = 2.24, ApJ, 784, 152. doi:10.1088/0004-637X/784/2/152

9. Wen, Z.~Z., Zheng, X.~Z., An, F.~X., 2014, “Probing asymmetric structures in the outskirts of galaxies, ApJ, 787, 130. doi:10.1088/0004-637X/787/2/130

10. An, F.~X., Zheng, X.~Z., Meng, Y.~Z., Chen Y., Wen Z., Lv G., 2013, “The nature of [S III]λλ9096, 9532 emitters at z = 1.34 and 1.23, SCIENCE CHINA, Physics, Mechanics & Astronomy, 56, 2226. doi:10.1007/s11433-013-5331-y

Other(non-academic) Jobs/Positions:
Personal Website: https://orcid.org/0000-0001-7943-0166
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