Y. J. Xiao

ORCID: 0009-0004-2243-8289
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About
Contact & Profiles
Research Areas
  • Quantum Chromodynamics and Particle Interactions
  • Stellar, planetary, and galactic studies
  • Astronomical Observations and Instrumentation
  • Particle physics theoretical and experimental studies
  • CCD and CMOS Imaging Sensors
  • Calibration and Measurement Techniques
  • Astronomy and Astrophysical Research
  • Computational Physics and Python Applications
  • Black Holes and Theoretical Physics
  • Gamma-ray bursts and supernovae
  • Galaxies: Formation, Evolution, Phenomena
  • Medical Imaging Techniques and Applications
  • Atomic and Subatomic Physics Research

National Astronomical Observatories
2025

Chinese Academy of Sciences
2025

Astronomy and Space
2025

University of Chinese Academy of Sciences
2020-2025

Institute of High Energy Physics
2020

Abstract The China Space Station Telescope (CSST) is a forthcoming space-based optical telescope designed to co-orbit with the Chinese Station. With planned slitless spectroscopic survey spanning broad wavelength range of 255 − 1000 nm and an average spectral resolution exceeding 200, CSST holds significant potential for cosmic large-scale structure analysis. In this study, we focus on redshift determinations from spectra through emission line analysis within framework. Our tailored...

10.1093/mnras/staf304 article EN cc-by Monthly Notices of the Royal Astronomical Society 2025-02-19

Abstract In this study, we present the construction of a new proper-motion catalog utilizing photometric data from Sloan Digital Sky Survey (SDSS) and Dark Energy Spectroscopic Instrument (DESI) imaging surveys, with median time baseline about 13 yr. To mitigate systematic errors, DESI galaxy positions are employed to establish reference frame correct position-, magnitude-, color-dependent discrepancies between SDSS sets. Spanning 12,589 deg 2 , encompasses 223.7 million non-Gaia objects...

10.3847/1538-3881/adb72c article EN cc-by The Astronomical Journal 2025-03-06

Abstract We present the identification of changing-look active galactic nuclei (CL-AGNs) from Dark Energy Spectroscopic Instrument First Data Release and Sloan Digital Sky Survey 16 at z ≤ 0.9. To confirm CL-AGNs, we utilize spectral flux calibration assessment via an [O iii ]-based calibration, pseudophotometry examination, visual inspection. This rigorous selection process allows us to compile a statistical catalog 561 encompassing 527 H β , 149 α 129 Mg ii CL behaviors. In this sample,...

10.3847/1538-4365/adc124 article EN cc-by The Astrophysical Journal Supplement Series 2025-05-01
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