Authors

Tomás Ahumada, College of Computer, Mathematical, & Natural Sciences
Shreya Anand, California Institute of Technology
Michael W. Coughlin, College of Science and Engineering
Igor Andreoni, College of Computer, Mathematical, & Natural Sciences
Erik C. Kool, Stockholms universitet
Harsh Kumar, Indian Institute of Technology Bombay
Simeon Reusch, Deutsches Elektronen-Synchrotron (DESY)
Ana Sagués-Carracedo, Stockholms universitet
Robert Stein, California Institute of Technology
S. Bradley Cenko, NASA Goddard Space Flight Center
Mansi M. Kasliwal, California Institute of Technology
Leo P. Singer, NASA Goddard Space Flight Center
Rachel Dunwoody, University College Dublin
Joseph Mangan, University College Dublin
Varun Bhalerao, Indian Institute of Technology Bombay
Mattia Bulla, Stockholms universitet
Eric Burns, Louisiana State University
Matthew J. Graham, California Institute of Technology
David L. Kaplan, University of Wisconsin-Milwaukee
Daniel Perley, Liverpool John Moores University
Mouza Almualla, American University of Sharjah
Joshua S. Bloom, University of California, Berkeley
Virginia Cunningham, Space Telescope Science Institute
Kishalay De, MIT Kavli Institute for Astrophysics and Space Research
Pradip Gatkine, California Institute of Technology
Anna Y.Q. Ho, Lawrence Berkeley National Laboratory
Viraj Karambelkar, California Institute of Technology
Albert K.H. Kong, National Tsing Hua University
Yuhan Yao, California Institute of Technology
G. C. Anupama, Indian Institute of Astrophysics
Sudhanshu Barway, Indian Institute of Astrophysics
Shaon Ghosh, Montclair State University
Ryosuke Itoh, Bisei Astronomical Observatory

Document Type

Article

Publication Date

6-1-2022

Abstract

The Fermi Gamma-ray Burst Monitor (GBM) triggers on-board in response to ∼40 short gamma-ray bursts (SGRBs) per year; however, their large localization regions have made the search for optical counterparts a challenging endeavour. We have developed and executed an extensive program with the wide field of view of the Zwicky Transient Facility (ZTF) camera, mounted on the Palomar 48 inch Oschin telescope (P48), to perform target-of-opportunity (ToO) observations on 10 Fermi-GBM SGRBs during 2018 and 2020-2021. Bridging the large sky areas with small field-of-view optical telescopes in order to track the evolution of potential candidates, we look for the elusive SGRB afterglows and kilonovae (KNe) associated with these high-energy events. No counterpart has yet been found, even though more than 10 ground-based telescopes, part of the Global Relay of Observatories Watching Transients Happen (GROWTH) network, have taken part in these efforts. The candidate selection procedure and the follow-up strategy have shown that ZTF is an efficient instrument for searching for poorly localized SGRBs, retrieving a reasonable number of candidates to follow up and showing promising capabilities as the community approaches the multi-messenger era. Based on the median limiting magnitude of ZTF, our searches would have been able to retrieve a GW170817-like event up to ∼200 Mpc and SGRB afterglows to z = 0.16 or 0.4, depending on the assumed underlying energy model. Future ToOs will expand the horizon to z = 0.2 and 0.7, respectively.

Publication Source (Journal or Book title)

Astrophysical Journal

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