collaborators

7 papers

astro-ph.CO2026

Filtering Interlopers with Photometry and Diagnostic Features: A Machine Learning Framework Validated with CSST Slitless Spectroscopy

Hui Peng, Yu Yu, Yiyang Guo +13

The slitless spectroscopic method employed by missions such as Euclid and the Chinese Space-station Survey Telescope (CSST) faces a fundamental challenge: spectroscopic redshifts d…

astro-ph.GA2025

Evolution of the Physical Properties of the Most Massive Galaxies in Clusters and their Protohalos

Qingyang Li, Xiaohu Yang, Antonios Katsianis +7

We investigated the evolution of the physical properties of the brightest galaxies in clusters and their protohalos from to . Galaxy clusters and groups are identifi…

astro-ph.CO2025

Future Cosmology: New Physics and Opportunity from the China Space Station Telescope (CSST)

Yan Gong, Haitao Miao, Xingchen Zhou +12

The China Space Station Telescope (CSST) is the next-generation Stage~IV survey telescope. It can simultaneously perform multi-band imaging and slitless spectroscopic wide- and dee…

astro-ph.CO2025

CSST Large Scale Structure Analysis Pipeline: III. Emission-line Redshift Measurement for Slitless Spectra

Jipeng Sui, Hu Zou, Xiaohu Yang +21

The China Space Station Telescope (CSST) is a forthcoming space-based optical telescope designed to co-orbit with the Chinese Space Station. With a planned slitless spectroscopic s…

astro-ph.GA2025

From Halos to Galaxies. X: Decoding Galaxy SEDs with Physical Priors and Accurate Star Formation History Reconstruction

Zeyu Gao, Yingjie Peng, Kai Wang +18

The spectral energy distribution (SED) of galaxies is essential for deriving fundamental properties like stellar mass and star formation history (SFH). However, conventional method…

astro-ph.GA2025

From Halos to Galaxies. VI. Improved halo mass estimation for SDSS groups and measurement of the halo mass function

Dingyi Zhao, Yingjie Peng, Yipeng Jing +18

In CDM cosmology, galaxies form and evolve in their host dark matter (DM) halos. Halo mass is crucial for understanding the halo-galaxy connection. The abundance matching (AM)…