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Four (Super)Luminous Supernovae From the First Months of the ZTF Survey

Lunnan, R. and Yan, Lin and Perley, D. A. and Schultze, S. and Taggart, K. and Gal-Yam, A. and Fremling, C. and Soumagnac, Maayane T. and Ofek, E. O. and Adams, S. M. and Barbarino, C. and Bellm, E. C. and De, K. and Fransson, C. and Frederick, S. and Golkhou, V. Zach and Graham, Matthew J. and Hallakoun, N. and Ho, A. Y. Q. and Kasliwal, Mansi M. and Kaspi, S. and Kulkarni, S. R. and Laher, R. R. and Masci, Frank J. and Pozo Nunez, F. and Rusholme, B. and Quimby, R. M. and Shupe, D. L. and Sollerman, J. and Taddia, F. and van Roestel, J. and Yang, Y. and Yao, Yuhan (2019) Four (Super)Luminous Supernovae From the First Months of the ZTF Survey. . (Unpublished) https://resolver.caltech.edu/CaltechAUTHORS:20191121-151009371

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Abstract

We present photometry and spectroscopy of four hydrogen-poor luminous supernovae discovered during the two-month science commissioning and early operations of the Zwicky Transient Facility (ZTF) survey. Three of these objects, SN2018bym (ZTF18aapgrxo), SN2018avk (ZTF18aaisyyp) and SN2018bgv (ZTF18aavrmcg) resemble typical SLSN-I spectroscopically, while SN2018don (ZTF18aajqcue) may be an object similar to SN2007bi experiencing considerable host galaxy reddening, or an intrinsically long-lived, luminous and red SN Ic. We analyze the light curves, spectra, and host galaxy properties of these four objects and put them in context of the population of SLSN-I. SN2018bgv stands out as the fastest-rising SLSN-I observed to date, with a rest-frame g-band rise time of just 10 days from explosion to peak -- if it is powered by magnetar spin-down, the implied ejecta mass is only ~1 M⊙. SN2018don also displays unusual properties -- in addition to its red colors and comparatively massive host galaxy, the light curve undergoes some of the strongest light curve undulations post-peak seen in a SLSN-I, which we speculate may be due to interaction with circumstellar material. We discuss the promises and challenges of finding SLSNe in large-scale surveys like ZTF given the observed diversity in the population.


Item Type:Report or Paper (Discussion Paper)
Related URLs:
URLURL TypeDescription
https://arxiv.org/abs/1910.02968arXivDiscussion Paper
ORCID:
AuthorORCID
Lunnan, R.0000-0001-9454-4639
Yan, Lin0000-0003-1710-9339
Perley, D. A.0000-0001-8472-1996
Gal-Yam, A.0000-0002-3653-5598
Fremling, C.0000-0002-4223-103X
Soumagnac, Maayane T.0000-0001-6753-1488
Ofek, E. O.0000-0002-6786-8774
Adams, S. M.0000-0001-5855-5939
Bellm, E. C.0000-0001-8018-5348
Fransson, C.0000-0001-8532-3594
Golkhou, V. Zach0000-0001-8205-2506
Graham, Matthew J.0000-0002-3168-0139
Ho, A. Y. Q.0000-0002-9017-3567
Kasliwal, Mansi M.0000-0002-5619-4938
Kulkarni, S. R.0000-0001-5390-8563
Laher, R. R.0000-0003-2451-5482
Masci, Frank J.0000-0002-8532-9395
Rusholme, B.0000-0001-7648-4142
Quimby, R. M.0000-0001-9171-5236
Sollerman, J.0000-0003-1546-6615
Taddia, F.0000-0002-2387-6801
van Roestel, J.0000-0002-2626-2872
Yao, Yuhan0000-0001-6747-8509
Additional Information:Based on observations obtained with the Samuel Oschin Telescope 48-inch and the 60- inch Telescope at the Palomar Observatory as part of the Zwicky Transient Facility project. ZTF is supported by the National Science Foundation under Grant No. AST-1440341 and a collaboration including Caltech, IPAC, the Weizmann Institute for Science, the Oskar Klein Center at Stockholm University, the University of Maryland, the University of Washington, Deutsches Elektronen-Synchrotron and Humboldt University, Los Alamos National Laboratories, the TANGO Consortium of Taiwan, the University of Wisconsin at Milwaukee, and Lawrence Berkeley National Laboratories. Operations are conducted by COO, IPAC, and UW. The Liverpool Telescope is operated on the island of La Palma by Liverpool John Moores University in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias with financial support from the UK Science and Technology Facilities Council. This research has made use of data obtained through the High Energy Astrophysics Science Archive Research Center Online Service, provided by the NASA/Goddard Space Flight Center. The ZTF forced-photometry service was funded under the Heising-Simons Foundation grant #12540303 (PI: Graham). This work was supported by the GROWTH project funded by the National Science Foundation under Grant No 1545949. AGYs research is supported by the EU via ERC grant No. 725161, the ISF GW excellence center, an IMOS space infrastructure grant and the BSF Transformative program as well as The Benoziyo Endowment Fund for the Advancement of Science, the Deloro Institute for Advanced Research in Space and Optics, The Veronika A. Rabl Physics Discretionary Fund, Paul and Tina Gardner and the WIS-CIT joint research grant; AGY is the recipient of the Helen and Martin Kimmel Award for Innovative Investigation. R.L. is supported by a Marie Skłodowska-Curie Individual Fellowship within the Horizon 2020 European Union (EU) Framework Programme for Research and Innovation (H2020-MSCA-IF-2017-794467). Facilities: PO:1.2m, PO:Hale, Liverpool:2m, NOT, Keck:I Software: george (Ambikasaranetal. 2015), heasoft (https://heasarc.nasa.gov/lheasoft/), LAMBDAR(Wright etal.2016),MOSFiT(Guillochonetal. 2018),PhotoFit(Soumagnac etal. 2019)
Group:Infrared Processing and Analysis Center (IPAC), Zwicky Transient Facility
Funders:
Funding AgencyGrant Number
NSFAST-1440341
CaltechUNSPECIFIED
Infrared Processing and Analysis Center (IPAC)UNSPECIFIED
Weizmann Institute of ScienceUNSPECIFIED
Stockholm UniversityUNSPECIFIED
University of MarylandUNSPECIFIED
University of WashingtonUNSPECIFIED
Deutsches Elektronen-SynchrotronUNSPECIFIED
Humboldt UniversityUNSPECIFIED
Los Alamos National LaboratoryUNSPECIFIED
TANGO ConsortiumUNSPECIFIED
University of Wisconsin-MilwaukeeUNSPECIFIED
Lawrence Berkeley National LaboratoryUNSPECIFIED
Science and Technology Facilities Council (STFC)UNSPECIFIED
Heising-Simons Foundation12540303
NSFAST-1545949
European Research Council (ERC)725161
Israel Science FoundationUNSPECIFIED
IMOS Space InfrastructureUNSPECIFIED
Binational Science Foundation (USA-Israel)UNSPECIFIED
Benoziyo Endowment FundUNSPECIFIED
Deloro Institute for Advanced Research in Space and OpticsUNSPECIFIED
Veronika A. Rabl Physics Discretionary FundUNSPECIFIED
Paul and Tina GardnerUNSPECIFIED
WIS-CIT Joint ResearchUNSPECIFIED
Kimmel AwardUNSPECIFIED
Marie Curie FellowshipH2020-MSCA-IF-2017-794467
Subject Keywords:supernovae: general, supernovae: individual (SN2018avk, SN2018don, SN2018bym, SN2018bgv) — surveys
Record Number:CaltechAUTHORS:20191121-151009371
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20191121-151009371
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:100001
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:21 Nov 2019 23:30
Last Modified:27 Nov 2019 17:20

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