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The Zwicky Transient Facility Bright Transient Survey I: Spectroscopic Classification and the Redshift Completeness of Local Galaxy Catalogs

Fremling, U. C. and Miller, A. A. and Sharma, Y. and Dugas, A. and Perley, D. A. and Taggart, K. and Sollerman, J. and Goobar, A. and Graham, M. L. and Neill, J. D. and Nordin, J. and Rigault, M. and Walters, R. and Andreoni, I. and Bagdasaryan, A. and Belicki, J. and Cannella, C. and Bellm, Eric C. and Cenko, S. B. and De, K. and Dekany, R. and Frederick, S. and Golkhou, V. Zach and Graham, M. and Helou, G. and Ho, A. Y. Q. and Kasliwal, M. and Kupfer, T. and Laher, Russ R. and Mahabal, A. and Masci, Frank J. and Riddle, R. and Rusholme, Ben and Schulze, S. and Shupe, David L. and Smith, R. M. and Yan, Lin and Yao, Y. and Zhuang, Z. and Kulkarni, S. R. (2019) The Zwicky Transient Facility Bright Transient Survey I: Spectroscopic Classification and the Redshift Completeness of Local Galaxy Catalogs. . (Unpublished) https://resolver.caltech.edu/CaltechAUTHORS:20191120-152035670

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Abstract

The Zwicky Transient Facility (ZTF) is performing a three-day cadence survey of the visible Northern sky (~3π). The transient candidates found in this survey are announced via public alerts. As a supplementary product ZTF is also conducting a large spectroscopic campaign: the ZTF Bright Transient Survey (BTS). The goal of the BTS is to spectroscopically classify all extragalactic transients brighter than 18.5 mag at peak brightness and immediately announce those classifications to the public. Extragalactic discoveries from ZTF are predominantly Supernovae (SNe). The BTS is the largest flux-limited SN survey to date. Here we present a catalog of the761 SNe that were classified during the first nine months of the survey (2018 Apr. 1 to 2018 Dec. 31). The BTS SN catalog contains redshifts based on SN template matching and spectroscopic host galaxy redshifts when available. Based on this data we perform an analysis of the redshift completeness of local galaxy catalogs, dubbed as the Redshift Completeness Fraction (RCF; the number of SN host galaxies with known spectroscopic redshift prior to SN discovery divided by the total number of SN hosts). In total, we identify the host galaxies of 512 Type Ia supernovae, 227 of which have known spectroscopic redshifts, yielding an RCF estimate of 44%±1%. We find a steady decrease in the RCF with increasing distance in the local universe. For z < 0.05, or ~200 Mpc, we find RCF = 0.6, which has important ramifications when searching for multimessenger astronomical events. Prospects for dramatically increasing the RCF are limited to new multi-fiber spectroscopic instruments, or wide-field narrowband surveys. We find that existing galaxy redshift catalogs are only 50% complete at r ≈ 16.9 mag. Pushing this limit several magnitudes deeper will pay huge dividends when searching for electromagnetic counterparts to gravitational wave events.


Item Type:Report or Paper (Discussion Paper)
Related URLs:
URLURL TypeDescription
http://arxiv.org/abs/1910.12973arXivDiscussion Paper
ORCID:
AuthorORCID
Fremling, U. C.0000-0002-4223-103X
Miller, A. A.0000-0001-9515-478X
Sollerman, J.0000-0003-1546-6615
Goobar, A.0000-0002-4163-4996
Neill, J. D.0000-0002-0466-1119
Andreoni, I.0000-0002-8977-1498
Bellm, Eric C.0000-0001-8018-5348
Cenko, S. B.0000-0003-1673-970X
De, K.0000-0002-8989-0542
Graham, M.0000-0002-3168-0139
Helou, G.0000-0003-3367-3415
Ho, A. Y. Q.0000-0002-9017-3567
Kasliwal, M.0000-0002-5619-4938
Kupfer, T.0000-0002-6540-1484
Laher, Russ R.0000-0003-2451-5482
Mahabal, A.0000-0003-2242-0244
Masci, Frank J.0000-0002-8532-9395
Riddle, R.0000-0002-0387-370X
Rusholme, Ben0000-0001-7648-4142
Shupe, David L.0000-0003-4401-0430
Yan, Lin0000-0003-1710-9339
Kulkarni, S. R.0000-0001-5390-8563
Additional Information:Received October 30, 2019. 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. This work was supported by the GROWTH project funded by the National Science Foundation under PIRE Grant No 1545949. The ZTF forced-photometry service was funded under the Heising- Simons Foundation grant #12540303 (PI: Graham). A.A.M. is funded by the Large Synoptic Survey Telescope Corporation, the Brinson Foundation, and the Moore Foundation in support of the LSSTC Data Science Fellowship Program, he also receives support as a CIERA Fellow by the CIERA Postdoctoral Fellowship Program (Center for Interdisciplinary Exploration and Research in Astrophysics, Northwestern University). M.R. has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement No 759194 - USNAC). The Oskar Klein Centre is funded by the Swedish Research Council. A.Y.Q.H. is supported by a National Science Foundation Graduate Research Fellowship under Grant No. DGE1144469. Partially 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. Some of the data presented here were obtained with ALFOSC, which is provided by the Instituto de Astrofisica de Andalucia (IAA) under a joint agreement with the University of Copenhagen and NOTSA. 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 NASA; the observatory was made possible by the generous financial support of the W. M. Keck Foundation. This paper is partly based on observations made with the Italian Telescopio Nazionale Galileo (TNG) operated on the island of La Palma by the Fundación Galileo Galilei of the INAF (Istituto Nazionale di Astrofisica) at the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias. Partially based on observations obtained with the Apache Point Observatory 3.5-meter telescope, which is owned and operated by the Astrophysical Research Consortium. Partially based on observations from the LCOGT network. Partially based on public observations collected at the WHT, operated on the island of La Palma by the Isaac Newton Group. 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. The SED Machine is based upon work supported by the National Science Foundation under Grant No. 1106171. We thank students Shaney Sze and Ho Ko for assisting with the manual candidate vetting during the summer of 2018. Software: SNID (Blondin & Tonry 2007), astropy (Astropy Collaboration et al. 2013), scipy (Jones et al. 2001), matplotlib (Hunter 2007), pandas (McKinney 2010), emcee (Foreman-Mackey et al. 2013), corner (Foreman-Mackey 2016), MultinomCI (Signorell & et al. 2019), PYSEDM (Rigault et al. 2019), IRAF (Tody 1986), PyRAF (Science Software Branch at STScI 2012), pyraf-dbsp (Bellm & Sesar 2016), LPipe (Perley 2019), pyDIS (Davenport et al. 2016).
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 Maryland UNSPECIFIED
University of WashingtonUNSPECIFIED
Deutsches Elektronen-SynchrotronUNSPECIFIED
Humboldt UniversityUNSPECIFIED
Los Alamos National LaboratoryUNSPECIFIED
TANGO ConsortiumUNSPECIFIED
University of Wisconsin-MilwaukeeUNSPECIFIED
Lawrence Berkeley National LaboratoryUNSPECIFIED
NSFAST-1545949
Heising-Simons Foundation12540303
Large Synoptic Survey Telescope CorporationUNSPECIFIED
Brinson FoundationUNSPECIFIED
Gordon and Betty Moore FoundationUNSPECIFIED
Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA)UNSPECIFIED
Northwestern UniversityUNSPECIFIED
European Research Council (ERC)759194
Swedish Research CouncilUNSPECIFIED
NSF Graduate Research FellowshipDGE-1144469
W. M. Keck FoundationUNSPECIFIED
Science and Technology Facilities Council (STFC)UNSPECIFIED
NSFAST-1106171
Subject Keywords:supernovae: general— galaxies: distances and redshifts— catalogs— surveys
Record Number:CaltechAUTHORS:20191120-152035670
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20191120-152035670
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:99964
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:20 Nov 2019 23:39
Last Modified:20 Nov 2019 23:39

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