S605B, MongManWai Building,
Beijing 100084, China
shuang [at] tsinghua.edu.cn
This website is still under-construction!!
My primary research interest is the observational study of galaxy evolution and galaxy-halo connection. Most of my works take advantage of today’s multi-band imaging data, spectroscopic surveys, and hydrodynamic simulations to probe the structure assembly and star formation history of different classes of galaxies.
My recent works focus on both the most massive (elliptical galaxies) and most abundant (dwarf galaxies) galaxies in our universe. With the help of weak gravitational lensing and statistical modeling techniques, I also aspire to deepen our understanding of galaxy-halo connection models and explore the applications of such models in observational cosmology.
I am a member of the Subaru Strategic Program (SSP) using the Hyper-Suprime Camera (HSC) on the 8.2-meter Subaru Telescope and the Merian Survey - an intermediate-band survey of the HSC footprint using the Dark Energy Camera (DECam). Currently, I am applying to become a member of the Dark Energy Spectroscopic Instrument (DESI) spectroscopic survey project. I am also helping organize the development of MUltiplexed Survey Telescope (MUST), a new 6.5-meter telescope in China for the next-generation spectroscopic survey, and its scientific collaboration.
I am always happy to discuss science and collaborate with people. Feel free to contact me if you are interested in my research or have any questions about my work.
- Reaching for the Edge I: probing the outskirts of massive galaxies with HSC, DECaLS, SDSS, and DragonflyMNRAS, Oct 2022
- The outer stellar mass of massive galaxies: a simple tracer of halo mass with scatter comparable to richness and reduced projection effectsMNRAS, Oct 2022
- Weak lensing reveals a tight connection between dark matter halo mass and the distribution of stellar mass in massive galaxiesMNRAS, Mar 2020
- A detection of the environmental dependence of the sizes and stellar haloes of massive central galaxiesMNRAS, Oct 2018
- Individual stellar haloes of massive galaxies measured to 100 kpc at 0.3 < z < 0.5 using Hyper Suprime-CamMNRAS, Apr 2018
- Characterization and photometric performance of the Hyper Suprime-Cam Software PipelinePASJ, Jan 2018
- Fossil Evidence for the Two-phase Formation of Elliptical GalaxiesApJl, May 2013
- The Carnegie-Irvine Galaxy Survey. III. The Three-component Structure of Nearby Elliptical GalaxiesApJ, Mar 2013