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iPTF Survey for Cool Transients

Adams, S. M. and Blagorodnova, N. and Kasliwal, M. M. and Barlow, T. and Cook, D. O. and Ho, A. Y. Q. and Kulkarni, S. R. and Kupfer, T. and Neill, J. D. and Walters, R. and Laher, R. R. and Masci, F. (2018) iPTF Survey for Cool Transients. Publications of the Astronomical Society of the Pacific, 130 (985). Art. No. 034202. ISSN 0004-6280. https://resolver.caltech.edu/CaltechAUTHORS:20180202-104540651

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Abstract

We performed a wide-area (2000 deg^2) g and I band experiment as part of a two month extension to the Intermediate Palomar Transient Factory. We discovered 36 extragalactic transients including iPTF17lf, a highly reddened local SN Ia, iPTF17bkj, a new member of the rare class of transitional Ibn/IIn supernovae, and iPTF17be, a candidate luminous blue variable outburst. We do not detect any luminous red novae and place an upper limit on their rate. We show that adding a slow-cadence I band component to upcoming surveys such as the Zwicky Transient Facility will improve the photometric selection of cool and dusty transients.


Item Type:Article
Related URLs:
URLURL TypeDescription
ttps://doi.org/10.1088/1538-3873/aaa356DOIArticle
http://iopscience.iop.org/article/10.1088/1538-3873/aaa356/metaPublisherArticle
https://arxiv.org/abs/1711.10501arXivDiscussion Paper
ORCID:
AuthorORCID
Adams, S. M.0000-0001-5855-5939
Blagorodnova, N.0000-0003-0901-1606
Kasliwal, M. M.0000-0002-5619-4938
Cook, D. O.0000-0002-6877-7655
Ho, A. Y. Q.0000-0002-9017-3567
Kulkarni, S. R.0000-0001-5390-8563
Kupfer, T.0000-0002-6540-1484
Neill, J. D.0000-0002-0466-1119
Laher, R. R.0000-0003-2451-5482
Masci, F.0000-0002-8532-9395
Additional Information:© 2018 Astronomical Society of the Pacific. Received 2017 July 18. Accepted 2017 December 20. Published 2018 February 1. We thank Mislav Balokovic, Kevin Burdge, Kishalay De, George Djorgovski, Andrew Drake, Marianne Heida, Nikita Kamraj, and Harish Vedantham for taking observations used in this paper. We thank the anonymous referee and Chris Kochanek for helpful comments. A.A.M. is supported by a grant from the Large Synoptic Survey Telescope Corporation, which funds the Data Science Fellowship Program. J.S and F.T. gratefully acknowledge the support from the Knut and Alice Wallenberg Foundation. R.A., M.B., A.G., and R.F. acknowledge support from the Swedish Research Council and the Swedish Space Board. The Intermediate Palomar Transient Factory project is a scientific collaboration among the California Institute of Technology, Los Alamos National Laboratory, the University of Wisconsin, Milwaukee, the Oskar Klein Center, the Weizmann Institute of Science, the TANGO Program of the University System of Taiwan, and the Kavli Institute for the Physics and Mathematics of the Universe. Part of this research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. Some of the data presented herein were obtained at the W.M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W.M. Keck Foundation. These results made use of the Discovery Channel Telescope at Lowell Observatory. Lowell is a private, non-profit institution dedicated to astrophysical research and public appreciation of astronomy and operates the DCT in partnership with Boston University, the University of Maryland, the University of Toledo, Northern Arizona University and Yale University. The upgrade of the DeVeny optical spectrograph has been funded by a generous grant from John and Ginger Giovale. This work is partly based on observations made with the Nordic Optical Telescope, operated by the Nordic Optical Telescope Scientific Association at the Observatorio del Roque de los Muchachos, La Palma, Spain, of the Instituto de Astrofisica de Canarias. This work is partly based on observations made with DOLoRes@TNG.
Group:Infrared Processing and Analysis Center (IPAC), Palomar Transient Factory
Funders:
Funding AgencyGrant Number
Large Synoptic Survey Telescope CorporationUNSPECIFIED
Knut and Alice Wallenberg FoundationUNSPECIFIED
Swedish Research CouncilUNSPECIFIED
Swedish National Space Board (SNSB)UNSPECIFIED
NASA/JPL/CaltechUNSPECIFIED
W. M. Keck FoundationUNSPECIFIED
John and Ginger GiovaleUNSPECIFIED
Subject Keywords:supernovae: general supernovae: individual (SN 2017lf, AT 2017bkj, AT 2017be) surveys
Issue or Number:985
Record Number:CaltechAUTHORS:20180202-104540651
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20180202-104540651
Official Citation:S. M. Adams et al 2018 PASP 130 034202
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:84653
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:02 Feb 2018 22:03
Last Modified:03 Oct 2019 19:21

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