Curriculum Vitae for XMUM Official Website

BIOGRAPHY

Siyi Feng obtained PhD degree from Heidelberg University. She joined Xiamen University China in 2021.

Siyi Feng is an expert in submillimeter interferometry and astrochemistry.She has more than 2000 hrs’ observational data as principal investigator and co-investigator. Using the world’s leading interferometers and single-dish telescopes, she is currently leading an international team for several multi-wavelength line-image survey large projects (>100hr each). These observation projects are in the aim of characterizing the dynamo-chemical properties of the star and planetary forming systems, at a spatial scale from 20 pc down to 50 AU, throughout the Galaxy.
Siyi Feng has been a reviewer for ApJ, A&A, and Elsevier since 2015, has been a TAC member for JCMT since 2020.

Homepage: Siyi Feng

RESEARCH INTERESTS

• Star and Planet Formation

• Astrochemistry

• Radio Astronomy

EDUCATIONAL BACKGROUND

• Ph.D Degree, Department of Physics, Heidelberg University (2015)

• Master Degree, Department of Astronomy, Nanjing University (2011)

• Bachelor Degree, Department of Astronomy, Nanjing University (2008)

WORKING EXPERIENCE

•  Associate Professor, Xiamen University, China (2021 - )

•  EACOA Fellow, East Asian Core Observatories Association (2017 - 2021).

•  Postdoc, Max-Planck-Institute for Extraterrestrial Physics, Germany (2015 - 2017).

•  Visiting Scholar, Harvard-Smithsonian Center for Astrophysics, USA (2013-2014).

•  Marie Curie Early Stage Researcher, Max Planck Institute for Astronomy, Germany (2011-2015)

RESEARCH EXPERIENCE / GRANTS

• East Asian Core Observatories Association Fellow, 2017-2021.

• Marie Curie Early Stage Researcher, 2011-2015

REPRESENTATIVE PUBLICATIONS

Full list: NASA/ADS (harvard.edu)

[8] Feng, S.,  et al.,  “The Chemical Structure of Young High-mass Star-forming Clumps. II. Parsec-scale CO Depletion and Deuterium Fraction of HCO+”, 2020, ApJ, 901, 145.

doi:10.3847/1538-4357/abada3

[7] Feng, S.,  et al., “Chemical segregation of SO and SO2 in the bow shock region L1157-B1 and B2”, 2020, ApJ, 896, 37.

doi:10.3847/1538-4357/ab8813

[6] Feng, S.,  et al., “The chemical structure of young high-mass star-forming clumps: (I) Deuteration”, 2019, ApJ, 883, 202.

doi:10.3847/1538-4357/ab3a42

[5] Feng, S.,  et al., “Inferring the evolutionary stages of the internal structures of NGC 7538 S and IRS1 from chemistry”, 2016, A&A, 593, A46.

doi:10.1051/0004-6361/201424912

[4] Feng, S.,  et al., “Outflow detection in a 70 μm dark high-mass core”, 2016, ApJ, 828, 100.

doi:10.3847/0004-637X/828/2/100

[3] Feng, S.,  “Are infrared dark clouds really quiescent?”, 2016, A&A, 592, A21.

doi:10.1051/0004-6361/201526864

[2] Feng, S.,  “Resolving the chemical substructure of Orion-KL”, 2015, A&A, 581, A71.

doi:10.1051/0004-6361/201322725

[1] Feng, S.-Y., Dai, Z.-G., “Multiband fitting to three long GRBs with Fermi/LAT data: structured ejecta sweeping up a density-jump medium”, 2011, RAA, 11, 1046.

doi:10.1088/1674-4527/11/9/004

• As supervisor/co-supervisor:

[3] Luo, Gan, Feng, Siyi, +6,  “Sulfur chemistry in the Orion-KL”, 2019, ApJ, 885, 82.

doi:10.3847/1538-4357/ab45ef

[2] Peng, Yaping, +8+ Feng, Siyi, +4, “ALMA Observations of Vibrationally Excited HC3N Lines Toward Orion KL”, 2017, ApJ, 837, 49.

doi:10.3847/1538-4357/aa5c81

[1] Punanova, A. Caselli, P. Feng, S., +41 “Seeds of Life in Space (SOLIS). III. Zooming Into the Methanol Peak of the Prestellar Core L1544”,2018, ApJ, 855, 112.

doi:10.3847/1538-4357/aaad09