CaltechAUTHORS
  A Caltech Library Service

2900 Square Degree Search for the Optical Counterpart of Short Gamma-Ray Burst GRB 180523B with the Zwicky Transient Facility

Coughlin, Michael W. and Ahumada, Tomás and Cenko, S. B. and Cunningham, Virginia and Ghosh, Shaon and Singer, Leo P. and Bellm, Eric C. and Burns, Eric and De, Kishalay and Goldstein, Adam and Golkhou, V. Zach and Kaplan, David L. and Kasliwal, Mansi M. and Perley, Daniel A. and Sollerman, J. and Bagdasaryan, Ashot and Dekany, Richard and Duev, Dmitry A. and Feeney, Michael and Graham, Matthew J. and Hale, David and Kulkarni, S. R. and Kupfer, Thomas and Laher, Russ R. and Mahabal, Ashish and Masci, Frank J. and Miller, Adam A. and Neill, James D. and Patterson, Maria T. and Riddle , Reed and Rusholme, Ben and Smith, Roger and Tachibana, Yutaro and Walters, Richard (2019) 2900 Square Degree Search for the Optical Counterpart of Short Gamma-Ray Burst GRB 180523B with the Zwicky Transient Facility. Publications of the Astronomical Society of the Pacific, 131 (998). Art. No. 048001. ISSN 0004-6280. https://resolver.caltech.edu/CaltechAUTHORS:20190220-090032986

[img] PDF - Submitted Version
See Usage Policy.

838Kb

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20190220-090032986

Abstract

There is significant interest in the models for production of short gamma-ray bursts (GRBs). Until now, the number of known short GRBs with multi-wavelength afterglows has been small. While the Fermi GRB Monitor detects many GRBs relative to the Neil Gehrels Swift Observatory, the large localization regions makes the search for counterparts difficult. With the Zwicky Transient Facility (ZTF) recently achieving first light, it is now fruitful to use its combination of depth (m_(AB) ~ 20.6), field of view (≈47 square degrees), and survey cadence (every ~3 days) to perform Target of Opportunity observations. We demonstrate this capability on GRB 180523B, which was recently announced by the Fermi GRB Monitor as a short GRB. ZTF imaged ≈2900 square degrees of the localization region, resulting in the coverage of 61.6% of the enclosed probability over two nights to a depth of m_(AB) ~ 20.5. We characterized 14 previously unidentified transients, and none were found to be consistent with a short GRB counterpart. This search with the ZTF shows it is an efficient camera for searching for coarsely localized short GRB and gravitational-wave counterparts, allowing for a sensitive search with minimal interruption to its nominal cadence.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1088/1538-3873/aaff99DOIArticle
https://arxiv.org/abs/1901.11385arXivDiscussion Paper
ORCID:
AuthorORCID
Coughlin, Michael W.0000-0002-8262-2924
Ahumada, Tomás0000-0002-2184-6430
Cenko, S. B.0000-0003-1673-970X
Ghosh, Shaon0000-0001-9901-6253
Singer, Leo P.0000-0001-9898-5597
Bellm, Eric C.0000-0001-8018-5348
De, Kishalay0000-0002-8989-0542
Golkhou, V. Zach0000-0001-8205-2506
Kaplan, David L.0000-0001-6295-2881
Kasliwal, Mansi M.0000-0002-5619-4938
Perley, Daniel A.0000-0001-8472-1996
Sollerman, J.0000-0003-1546-6615
Duev, Dmitry A.0000-0001-5060-8733
Graham, Matthew J.0000-0002-3168-0139
Kulkarni, S. R.0000-0001-5390-8563
Kupfer, Thomas0000-0002-6540-1484
Laher, Russ R.0000-0003-2451-5482
Mahabal, Ashish0000-0003-2242-0244
Masci, Frank J.0000-0002-8532-9395
Miller, Adam A.0000-0001-9515-478X
Neill, James D.0000-0002-0466-1119
Patterson, Maria T.0000-0002-4753-3387
Rusholme, Ben0000-0001-7648-4142
Tachibana, Yutaro0000-0001-6584-6945
Additional Information:© 2019 The Astronomical Society of the Pacific. Received 2018 November 19; accepted 2019 January 16; published 2019 February 20. 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. Major funding has been provided by the U.S National Science Foundation under grant No. AST-1440341 and by the ZTF partner institutions: the California Institute of Technology, the Oskar Klein Centre, the Weizmann Institute of Science, the University of Maryland, the University of Washington, Deutsches Elektronen-Synchrotron, the University of Wisconsin-Milwaukee, and the TANGO Program of the University System of Taiwan. M.C. is supported by the David and Ellen Lee Postdoctoral Fellowship at the California Institute of Technology. S.G. is supported by the National Science Foundation with NSF Award PHY-1607585.
Group:Infrared Processing and Analysis Center (IPAC), Zwicky Transient Facility
Funders:
Funding AgencyGrant Number
NSFAST-1440341
CaltechUNSPECIFIED
Oskar Klein CentreUNSPECIFIED
Weizmann Institute of ScienceUNSPECIFIED
University of MarylandUNSPECIFIED
University of WashingtonUNSPECIFIED
Deutsches Elektronen-SynchrotronUNSPECIFIED
University of Wisconsin-MilwaukeeUNSPECIFIED
University System of TaiwanUNSPECIFIED
David and Ellen Lee Postdoctoral ScholarshipUNSPECIFIED
NSFPHY-1607585
Subject Keywords:gamma rays: general
Issue or Number:998
Record Number:CaltechAUTHORS:20190220-090032986
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190220-090032986
Official Citation:Michael W. Coughlin et al 2019 PASP 131 048001
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:92997
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:20 Feb 2019 18:24
Last Modified:06 Dec 2019 18:47

Repository Staff Only: item control page