My research uses large astronomical surveys to study AGN and galaxy evolution, pursue cosmological applications, and develop reliable methods for astronomical inference and discovery. I work with heterogeneous datasets across wavelengths to build source samples and investigate active galaxies and their environments.
The two pages below give an overview of the research programme and the papers behind it.
Our paper “Euclid Quick Data Release (Q1): XXXVIII. Euclid spectroscopy of quasars. 1. Identification and redshift determination of 3500 bright quasars” has been published by Astronomy & …
AIMS-z is an astrophysics-informed machine-learning project for reliable quasar redshifts, reusable spectral representations, and multimodal inference, with an initial focus on Euclid slitless spectra.
BEIJING, April 18 (Xinhua) – A group of astronomers has found over 1,300 new quasars behind the Galactic plane by using China’s Large Sky Area Multi-Object Fiber Spectroscopic …
Reposted from KIAA-PKU The Kavli Institute for Astronomy and Astrophysics at Peking University announces an advancement in cosmic exploration with the release of the CatNorth quasar …
We are located at the edge of the Galactic disk, and see our Galaxy as a hazy band of light made of countless stars in the night sky. Looking for extragalactic objects like quasars through …
