C
Chen-Wei Yang
Researcher at California Institute of Technology
Publications - 2
Citations - 443
Chen-Wei Yang is an academic researcher from California Institute of Technology. The author has contributed to research in topics: Star formation & Galaxy. The author has an hindex of 2, co-authored 2 publications receiving 395 citations. Previous affiliations of Chen-Wei Yang include Chinese Academy of Sciences.
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A continuum of H- to He-rich tidal disruption candidates with a preference for E+A galaxies
Iair Arcavi,Iair Arcavi,Iair Arcavi,Avishay Gal-Yam,Mark Sullivan,Yen-Chen Pan,S. Bradley Cenko,S. Bradley Cenko,Assaf Horesh,Eran O. Ofek,Annalisa De Cia,Lin Yan,Chen-Wei Yang,Chen-Wei Yang,Dale Andrew Howell,Dale Andrew Howell,D. Tal,Shrinivas R. Kulkarni,Shriharsh P. Tendulkar,Sumin Tang,Sumin Tang,Dong Xu,Assaf Sternberg,Judith G. Cohen,Joshua S. Bloom,Joshua S. Bloom,Peter Nugent,Peter Nugent,Mansi M. Kasliwal,Mansi M. Kasliwal,Daniel A. Perley,Robert M. Quimby,Adam A. Miller,Christopher A. Theissen,Russ R. Laher +34 more
TL;DR: The results of a Palomar Transient Factory (PTF) archival search for blue transients that lie in the magnitude range between "normal" corecollapse and superluminous supernovae (i.e., with −21 ≤ M_(R (peak)) ≤ − 19) were presented in this article.
Journal ArticleDOI
A Continuum of H- to He-Rich Tidal Disruption Candidates With a Preference for E+A Galaxies
Iair Arcavi,Iair Arcavi,Iair Arcavi,Avishay Gal-Yam,Mark Sullivan,Yen-Chen Pan,S. Bradley Cenko,S. Bradley Cenko,Assaf Horesh,Eran O. Ofek,Annalisa De Cia,Lin Yan,Chen-Wei Yang,Chen-Wei Yang,Dale Andrew Howell,Dale Andrew Howell,D. Tal,Shrinivas R. Kulkarni,Shriharsh P. Tendulkar,Sumin Tang,Sumin Tang,Dong Xu,Assaf Sternberg,Judith G. Cohen,Joshua S. Bloom,Joshua S. Bloom,Peter Nugent,Peter Nugent,Mansi M. Kasliwal,Mansi M. Kasliwal,Daniel A. Perley,Robert M. Quimby,Adam A. Miller,Christopher A. Theissen,Russ R. Laher +34 more
TL;DR: In this article, the results of a Palomar Transient Factory (PTF) archival search for blue transients which lie in the magnitude range between "normal" corecollapse and superluminous supernovae (i.e. with $-21\,{\leq}M{R\,(peak)}\,{\LEq}-19$) were presented.