SN 2020bqj: A Type Ibn supernova with a long-lasting peak plateau
Erik C. Kool(Stockholm University), Lin Yan(California Institute of Technology), J. Nordin(Humboldt-Universität zu Berlin), E. S. Phinney(California Institute of Technology), Itai Sfaradi(Hebrew University of Jerusalem), Kishalay De(California Institute of Technology), J. Sollerman(Stockholm University), Y. Sharma(California Institute of Technology), D. R. Williams(Hitachi (United Kingdom)), R. Lunnan(Stockholm University), Frank J. Masci, A. Horesh(Weizmann Institute of Science), Dmitry A. Duev(California Institute of Technology), C. Fremling(California Institute of Technology), Russ R. Laher(California Institute of Technology), T. Reynolds(University of Turku), C. Barbarino(Stockholm University), L. Tartaglia(Stockholm University), D. A. Perley(Liverpool John Moores University), K. Taggart(University of California, Santa Cruz), E. Karamehmetoglu(Aarhus University), Jan van Roestel, S. Schulze(Northwestern University), Eric C. Bellm(University of Washington), Héctor Rodríguez(California Institute of Technology), M. L. Graham(Las Cumbres Observatory Global Telescope Network), David A. Green(Columbia University), B. Rusholme(California Institute of Technology), V. Z. Golkhou(University of Washington), Maayane T. Soumagnac(Bar-Ilan University), Stephen Kaye(California Institute of Technology), Young-Lo Kim(Université Claude Bernard Lyon 1), Dan Reiley(California Institute of Technology), Michael Porter(California Institute of Technology)
Cited by 19
Related Papers
The Zwicky Transient Facility: System Overview, Performance, and First Results
|Publications of the Astronomical Society of the Pacific|2018|2.1k
The Palomar Transient Factory: System Overview, Performance, and First Results
|Publications of the Astronomical Society of the Pacific|2009|1.2k
The Zwicky Transient Facility: Science Objectives
|Publications of the Astronomical Society of the Pacific|2019|845
The Emergence of a Lanthanide-rich Kilonova Following the Merger of Two Neutron Stars
|The Astrophysical Journal Letters|2017|762
A γ-ray burst at a redshift of z ≈ 8.2
|Nature|2009|639