activity
19932024
most citedA New Dark Matter Candidate: Non-thermal Sterile Neutrinos

799 citations · 1.3k across the 31 of their papers we have counts for

collaborators

31 papers

astro-ph.SR2024★ 7 cited

A catalog of new slowly pulsating B-type stars

Xiang-dong Shi, Sheng-bang Qian, Li-ying Zhu +1

This paper reports the discovery of new slowly pulsating B-type stars. Based on the photometric, spectral, and astrometric data of TESS, LAMOST, and Gaia surveys, we have found 286…

astro-ph.SR2023★ 15 cited

New evidence for the precession of tilted disk in SDSS J081256.85+191157.8

Qi-Bin Sun, Sheng-Bang Qian, Li-Ying Zhu +5

Super-orbital signals and negative superhumps are thought to be related to the reverse precession of the nodal line in a tilted disk, but the evidence is lacking. Our results provi…

astro-ph.SR2023★ 17 cited

First discovery of QPOs in the dwarf nova HS 2325+8205 based on TESS photometry

Qi-Bin Sun, Sheng-Bang Qian, Li-Ying Zhu +9

HS 2325+8205 is a long-period eclipsing dwarf nova with an orbital period above the period gap (Porb>3 h) and is reported to be a Z Cam-type dwarf nova. Based on the photometry of…

astro-ph.GA2022★ 3 cited

Chemically Peculiar Stars in Integrated Light Stellar Population Models and Local Group Galaxies

Guy Worthey, Xiang Shi

Integrated-light models that incorporate common types of chemically peculiar (CP) stars are assembled using synthetic spectra. Selected spectral features encode significant age inf…

astro-ph.GA2022★ 6 cited

Individual element sensitivity for stellar evolutionary isochrones

Guy Worthey, Xiang Shi, Tathagata Pal +2

Stellar evolution calculations with variable abundance ratios were used to gauge the effects on temperatures, luminosities, and lifetimes in various phases. Individual elements C,…

astro-ph.SR2020★ 8 cited

ASAS J174406+2446.8 is identified as a marginal-contact binary with a possible cool third body

Xiang-Dong Shi, Sheng-Bang Qian, Lin-Jia +2

ASAS J174406+2446.8 was originally found as a Scuti-type pulsating star with the period P=0.189068 by ASAS survey. However, the LAMOST stellar parameters reveal that it…