A CONTINUUM OF H- TO He-RICH TIDAL DISRUPTION CANDIDATES WITH A PREFERENCE FOR E+A GALAXIES
I. Arcavi(Las Cumbres Observatory Global Telescope Network), Russ R. Laher(California Institute of Technology), Adam A. Miller(University of California, Berkeley), Shriharsh P. Tendulkar(Tata Institute of Fundamental Research), Judith G. Cohen(California Institute of Technology), A. Horesh(Weizmann Institute of Science), A. Gal‐Yam(Weizmann Institute of Science), R. Quimby(California Institute of Technology), S. R. Kulkarni(California Institute of Technology), Christopher A. Theissen(University of California San Diego), Lin Yan(California Institute of Technology), D. Tal(Weizmann Institute of Science), D. A. Perley(Liverpool John Moores University), D. Xu(Zhejiang Chinese Medical University), J. S. Bloom(University of California, Berkeley), S. B. Cenko(University of California, Berkeley), Chen‐Wei Yang(California Institute of Technology), P. Nugent(Lawrence Berkeley National Laboratory), E. O. Ofek(California Institute of Technology), A. De(Weizmann Institute of Science), D. A. Howell(Las Cumbres Observatory Global Telescope Network), M. Sullivan(University of Oxford), M. M. Kasliwal(California Institute of Technology), Sumin Tang(California Institute of Technology), A. Sternberg(Max Planck Institute for Astrophysics), Y. C. Pan(University of Oxford)
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