most citedThe Mini-SiTian Array: first-two-year operation

12 citations · 12 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2025

A Morpho-kinematic Study of Galactic High-ADF PNe Based on the VLT/UVES Deep Spectroscopy

Haomiao Huang, Xuan Fang, Jorge Garcia-Rojas +3

We report detailed analyses of deep, high-resolution spectra of three Galactic planetary nebulae (PNe) with high abundance discrepancy factors (ADFs), Hf2-2, M1-42 and NGC6153, obt…

astro-ph.SR2025

PyEMILI: A New Generation Computer-aided Spectral Line Identifier -- II. Emission-line Identification and Plasma Diagnostics of a Sample of Gaseous Nebulae

Zhijun Tu, Xuan Fang, Jorge García-Rojas +2

In order to test the robustness and reliability of the new generation spectral-line identifier PyEMILI, as initially introduced in Paper I, in line identification and establish a r…

astro-ph.SR2025

A Large Sample of JWST/NIRSpec Brown Dwarfs: New Distant Discoveries

Zhijun Tu, Shu Wang, Xiaodian Chen +1

Brown dwarfs are essential probes of stellar and planetary formation, yet their low luminosities pose challenges for detection at large Galactic distances. The James Webb Space Tel…

astro-ph.IM202512 cited

The Mini-SiTian Array: first-two-year operation

Min He, Hong Wu, Liang Ge +70

The SiTian project, designed to utilize 60 telescopes distributed across multiple sites in China, is a next-generation time-domain survey initiative. As a pathfinder for the SiTian…

astro-ph.SR2025

Three Brown Dwarfs Masquerading as High-Redshift Galaxies in JWST Observations

Zhijun Tu, Shu Wang, Xiaodian Chen +1

We report the spectroscopic identification of three brown dwarf candidates -- o005_s41280, o006_s00089, and o006_s35616 -- discovered in the RUBIES using James Webb Space Telescope…

astro-ph.SR2025

PyEMILI: A New Generation Computer-aided Spectral Line Identifier

Zhijun Tu, Xuan Fang, Robert Williams +1

Deep high-dispersion spectroscopy of Galactic photoionized gaseous nebulae, mainly planetary nebulae and HII regions, has revealed numerous emission lines. As a key step of spectra…