73 citations
- Tsinghua UniversityCN68 papers
- Chinese Academy of SciencesCN67 papers
- National Astronomical ObservatoriesCN60 papers
- Beijing Academy of Science and TechnologyCN51 papers
- University of Chinese Academy of SciencesCN47 papers
- Yunnan ObservatoriesCN37 papers
- Beijing Normal UniversityCN32 papers
- University of California, BerkeleyUS26 papers
- Tel Aviv UniversityIL19 papers
- Las Cumbres Observatory Global Telescope NetworkUS18 papers
- University of California, Santa BarbaraUS18 papers
- Purple Mountain ObservatoryCN16 papers
100 papers
Spectral Dataset of Stripped-Envelope Supernovae from the Tsinghua Supernova Group
Danfeng Xiang, Xiaofeng Wang, Jujia Zhang +40
The extent of envelope stripping in the progenitor stars is directly reflected in the diversity of spectral features observed in stripped-envelope supernovae (SESNe). Through exten…
Automated Identification of the Tip of the Red Giant Branch in Globular Clusters with Gaia Data
Yi Yang, Zhenzhen Shao, Xiaofeng Wang +1
This study introduces an automated approach for identifying the tip of the red giant branch (TRGB) in globular clusters, combining astronomical data with algorithmic methods. Using…
Thermal emission spectra of the ultra-hot Jupiter WASP-33 b
Qianyi Zou, Meng Zhai, Wei Wang +12
Observations of exoplanetary atmospheres provide critical insights into their chemical composition, formation and evolution history. Ultra-hot Jupiters serve as excellent targets f…
SN 2022acko: a low-luminosity SNe IIP with signs of early circumstellar interaction
Lin Han, Zhang Jujia, Wang Xiaofeng +13
We present optical-ultraviolet photometry and optical spectra for the type II supernova (SN) 2022acko. The spectroscopic observations span phases from 1.5 to 60 days…
Measuring the magnetic fields in the chromospheres of low-mass stars
Tianqi Cang, Pascal Petit, Jean-François Donati +11
Magnetic fields in the upper atmospheres of solar-like stars are believed to provide an enormous amount of energy to power the hot coronae and drive large-scale eruptions that coul…
SN 2024iss: A Double-peaked Type IIb Supernova with Evidence of Circumstellar Interaction
Liyang Chen, Xiaofeng Wang, Qinyu Wu +54
We present optical, ultraviolet, and X-ray observations of supernova (SN) 2024iss, a Type IIb SN that shows a prominent double-peaked light curve. We modeled the first peak with a…