About Me

Bio: Zili was born in Beijing, China and graduated from the University of Texas at Austin in 2019. She became interested in extragalactic astronomy and loved going to observatories. At UT, she studied the star formation history of dwarf galaxies with her research advisor Dr. Kristen McQuinn. Zili continued to study galaxies at Yale, now focusing on the enigmatic "Dark-matter-free" galaxies NGC1052-DF2 and DF4. Particularly, she hopes to find clues of how these galaxies formed and evolved from their unusual population of globular clusters. Apart from research, she writes about science. She published articles on Astrobites and works at the Yale Graduate Writing Lab as a writing consultant.

Publications:

ORCID iD iconOrcID: 0000-0002-5120-1684
ADS link

Research

Ongoing Project:
KCWI velocity dispersion measurement of NGC1052-DF4 and its brightest GC.
NGC1052-DF4 has been proposed to have little to no dark matter based on the low velocity dispersion of its globular clusters. However, this velocity dispersion could also be explained if the galaxy has a cored dark matter profile. To distinguish between the stars-only model (which predicts a dispersion of 6-10 km/s) and a cored DM profile (larger than 10 km/s), we need to accurately measure the internal velocity dispersion of the galaxy. The other mystery about NGC1052-DF2 and DF4 is their overly-luminous globular clusters. To get an independent mass estimate, we can use the spectral lines of the brightest GC to find its internal velocity dispersion.
To answer both of these questions, we obtained 12 hours of observations using the KCWI spectrograph on the Keck II telescope. From the high-resolution spectrum, we will measure the velocity dispersion with less than 2 km/s error.
Stay tuned for the updates on this project!

Past Projects:

4. TRGB Distance to NGC1052-DF2.
Shen, Z., Danieli, S., van Dokkum, P., et al., 2021, ApJ, 914, L12
As the first "dark matter deficient" galaxy, NGC1052-DF2 sparked many debates. Some argue that the apparent lack of dark matter and the overly luminous globular clusters can both be explained if the galaxy was much closer to us, compared to the canonical distance of 20 Mpc. Here we present 40 orbits of HST ACS data for NGC 1052–DF2 and use these data to measure the Tip of the Red Giant Branch (TRGB). The TRGB is readily apparent in the color-magnitude diagram. Using a forward model that incorporates photometric uncertainties, we find a distance of 22.1 Mpc. In addition to confirming the unusual properties of NGC1052-DF2, we also find a well-determined 2.1 Mpc separation between NGC1052-DF2 and NGC1052-DF4. The relative distance may be the key to understanding the origin of both galaxies. 3. Globular cluster luminosity function in NGC1052-DF2 and DF4.
Shen, Z., van Dokkum, P., & Danieli, S., 2021, ApJ, 909, 179
The dark matter deficient galaxies NGC1052-DF2 and NGC1052-DF4 also have unusually luminous globular clusters (GCs). In the luminosity function shown above, we combine the GC samples in both galaxies and compare it to the near-universal GC luminosity function. The GCs in these galaxies are almost 2 magnitudes brighter than the expected peak. 2. Discovery of a recent starburst in the dwarf galaxy KDG 215.
Cannon, J. M., Shen, Z., McQuinn, K. B. W., et al. 2018, ApJ, 864, L14
Dwarf galaxies like KDG 215 probe the low-mass end of galaxy formation. Although KDG 215 is unusually gas-rich, it is currently inactive in star formation. To investigate its evolution, we used HST archival images to construct color-magnitude diagrams (CMDs). I restructured and streamlined the data analysis process. I also managed the extensive GitHub repository for our CMD matching tool. With the Wrangler supercomputer at the Texas Advanced Computing Center, I reconstructed the star formation history of KDG 215 by matching the observed CMD to synthetic CMDs from stellar evolution models. The result of the best fit revealed a surprisingly unusual star formation history for this galaxy. While most galaxies form stars early on and continue to form stars, KDG 215 only formed around 40% of its total stellar mass until one billion years ago. Then, it experienced an active episode of star formation followed by a gradual decline to its current inactive state. We discovered an extreme case of stellar feedback suppressing star formation. 1. Solar chromosphere data calibration pipeline.
Shen, Z., Diercke, A., Denker, C.. 2018, Astron. Nachr., 339, 661
In the summer of 2018, I developed a method to remove instrumental artifacts from solar images and incorporated it into the reduction pipeline. I joined the optical solar physics group at the Leibniz Institute of Astrophysics Potsdam, under Prof. Carsten Denker. We studied the migration of solar filaments which revealed the cyclic variation of the magnetic field. Measuring the kinematics of solar filaments required accurate full-disk Doppler maps. In our dataset, uneven filter transmission left a systematic yin-yang pattern and significantly impaired velocity calculation. I developed a method using Zernike polynomials to characterize and remove the image artifacts. After removing the artifacts, I calibrated the obtained Doppler maps with high-resolution spectrograph data. The pipeline was implemented in IDL and optimized to re-process archival data taken in the past six years. The pipeline has been added to the sTools solar data reduction pipeline for all future data processing. This new method can be applied generally to calibrate full-disk solar images, and it will facilitate studies of solar filament migration.

Community

Science Writing:
  • Read my astrobite articles here.
  • I work at the Yale Poorvu Center as a Graduate Writing Fellow, offering one-on-one writing consultations and leading workshops.
Press and Outreach:
  • My project on the distance to NGC1052-DF2 has been covered by STScI, Yale, and IAS.
  • Austin has the largest Astronomy on Tap audience in the country, and I was invited to give a talk in my last year of college. You can watch it on Youtube.
Leadership:
  • I represent the Astronomy Department at the Yale Graduate Student Assembly.
  • I serve as a mentor in the Yale Astronomy Department grad-undergrad mentor program.