Luminous Type II Short-Plateau Supernovae 2006Y, 2006ai, and 2016egz: A Transitional Class from Stripped Massive Red Supergiants
2021
We are grateful to Viktoriya Morozova, Anthony L.
Piro, Lars Bildsten, Bill Paxton, J. J. Eldridge, Eva
Laplace, Sergei I. Blinnikov, Ken'ichi Nomoto, Masaomi
Tanaka, and Nozomu Tominaga for their comments and
discussions.
D.H., D.A.H., G.H., C.M., and J.B. were supported
by NSF grants AST-1313484 and AST-1911225, as well
as by NASA grant 80NSSC19kf1639. D.H. is thankful
for support and hospitality by the National Astronomical
Observatory of Japan where many discussions
of this work took place. J.A.G. is supported by
the NSF GRFP under grant number 1650114. I.A.
is a CIFAR Azrieli Global Scholar in the Gravity and
the Extreme Universe Program and acknowledges support
from that program, from the European Research
Council (ERC) under the European Union's Horizon
2020 research and innovation program (grant agreement
number 852097), from the Israel Science Foundation
(grant numbers 2108/18 and 2752/19), from the United
States - Israel Binational Science Foundation (BSF), and
from the Israeli Council for Higher Education Alon Fellowship.
C.P.G acknowledges support from EU/FP7-
ERC grant number 615929. Research by S.V. is supported
by NSF grant AST{1813176. Q.F. acknowledges
support from the JSPS Kakenhi grant (20J23342).
K. Maeda acknowledges support by JSPS KAKENHI
grants JP20H00174, JP20H04737, JP18H04585,
JP18H05223, and JP17H02864. G.F. acknowledges the support from CONICET through grant PIP-2015-2017-
11220150100746CO and from ANPCyT through grant
PICT-2017-3133. M.D.S. acknowledges support from
a project grant (8021-00170B) from the Independent
Research Fund Denmark and a generous grant (28021)
from the VILLUM FONDEN. M.G. is supported by the
Polish NCN MAESTRO grant 2014/14/A/ST9/00121.
K. Maguire is funded by the EU H2020 ERC grant
number 758638. T.M.B. was funded by the CONICYT
PFCHA/DOCTORADOBECAS CHILE/2017-
72180113.
This paper made use of data from the Las Cumbres
Observatory global network of telescopes through the
Supernova Key Project and Global Supernova Project.
This paper includes data gathered with the 6.5 meter
Magellan Telescopes located at Las Campanas Observatory,
Chile. The CSP-I was supported by the NSF under
grants AST-0306969, AST-0607438 and AST-1008343.
This research has made use of the NASA/IPAC Extragalactic
Database (NED), which is funded by NASA
and operated by the California Institute of Technology,
as well as IRAF, which is distributed by NOAO (operated
by AURA, Inc.), under cooperative agreement with
NSF.
The authors wish to recognize and acknowledge the
very signi cant cultural role and reverence that the summit
of Haleakal a has always had within the indigenous
Hawaiian community. We are most fortunate to have the
opportunity to conduct observations from the mountain.
Funding for SDSS-III has been provided by the Alfred
P. Sloan Foundation, the Participating Institutions, the
National Science Foundation, and the U.S. Department
of Energy O ce of Science. The SDSS-III website is
http://www.sdss3.org/.
SDSS-III is managed by the Astrophysical Research
Consortium for the Participating Institutions of the
SDSS-III Collaboration, including the University of Arizona,
the Brazilian Participation Group, Brookhaven
National Laboratory, Carnegie Mellon University, University
of Florida, the French Participation Group,
the German Participation Group, Harvard University,
the Instituto de Astro sica de Canarias, the Michigan
State/Notre Dame/JINA Participation Group, Johns
Hopkins University, Lawrence Berkeley National Laboratory,
Max Planck Institute for Astrophysics, Max
Planck Institute for Extraterrestrial Physics, New Mexico
State University, New York University, Ohio State
University, Pennsylvania State University, University of
Portsmouth, Princeton University, the Spanish Participation
Group, University of Tokyo, University of Utah,
Vanderbilt University, University of Virginia, University
of Washington, and Yale University.
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