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GROWTH on GW190425: Searching thousands of square degrees to identify an optical or infrared counterpart to a binary neutron star merger with the Zwicky Transient Facility and Palomar Gattini IR

Coughlin, Michael W. and Ahumada, Tomás and Anand, Shreya and De, Kishalay and Hankins, Matthew J. and Kasliwal, Mansi M. and Singer, Leo P. and Bellm, Eric C. and Andreoni, Igor and Cenko, S. Bradley and Cooke, Jeff and Copperwheat, Christopher M. and Dugas, Alison M. and Jencson, Jacob E. and Perley, Daniel A. and Yu, Po-Chieh and Bhalerao, Varun B. and Kumar, Harsh and Bloom, Joshua S. and Anupama, G. C. and Ashley, Michael C. B. and Bagdasaryan, Ashot and Biswas, Rahul and Buckley, David A. H. and Burdge, Kevin B. and Cook, David O. and Cromer, John and Cunningham, Virginia and D'aí, Antonino and Dekany, Richard G. and Delacroix, Alexandre and Dichiara, Simone and Duev, Dmitry A. and Dutta, Anirban and Feeney, Michael and Frederick, Sara and Gatkine, Pradip and Ghosh, Shaon and Goldstein, Daniel A. and Golkhou, V. Zach and Goobar, Ariel and Graham, Matthew J. and Hanayama, Hidekazu and Horiuchi, Takashi and Hung, Tiara and Jha, Saurabh W. and Kong, Albert K. H. and Giomi, Matteo and Kaplan, David L. and Karambelkar, V. R. and Kowalski, Marek and Kulkarni, Shrinivas R. and Kupfer, Thomas and La Parola, Valentina and Masci, Frank J. and Mazzali, Paolo A. and Moore, Anna M. and Mogotsi, Moses and Neill, James D. and Ngeow, Chow-Choong and Martínez-Palomera, Jorge and Pavana, M. and Ofek, Eran O. and Patil, Atharva Sunil and Riddle, Reed and Rigault, Mickael and Rusholme, Ben and Serabyn, Eugene and Shupe, David L. and Sharma, Yashvi and Sollerman, Jesper and Soon, Jamie and Staats, Kai and Taggart, Kirsty and Tan, Hanjie and Travouillon, Tony and Troja, Eleonora and Waratkar, Gaurav and Yatsu, Yoichi (2019) GROWTH on GW190425: Searching thousands of square degrees to identify an optical or infrared counterpart to a binary neutron star merger with the Zwicky Transient Facility and Palomar Gattini IR. . (Submitted) https://resolver.caltech.edu/CaltechAUTHORS:20190802-094555948

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Abstract

The beginning of the third observing run by the network of gravitational-wave detectors has brought the discovery of many compact binary coalescences. Prompted by the detection of the first binary neutron star merger in this run (GW190425 / LIGO/Virgo S190425z), we performed a dedicated follow-up campaign with the Zwicky Transient Facility (ZTF) and Palomar Gattini-IR telescopes. As it was a single gravitational-wave detector discovery, the initial skymap spanned most of the sky observable from Palomar Observatory, the site of both instruments. Covering 8000 deg$^2$ of the inner 99\% of the initial skymap over the next two nights, corresponding to an integrated probability of 46\%, the ZTF system achieved a depth of $\approx$\,21 $m_\textrm{AB}$ in $g$- and $r$-bands. Palomar Gattini-IR covered a total of 2200 square degrees in $J$-band to a depth of 15.5\,mag, including 32\% of the integrated probability based on the initial sky map. However, the revised skymap issued the following day reduced these numbers to 21\% for the Zwicky Transient Facility and 19\% for Palomar Gattini-IR. Out of the 338,646 ZTF transient "alerts" over the first two nights of observations, we narrowed this list to 15 candidate counterparts. Two candidates, ZTF19aarykkb and ZTF19aarzaod were particularly compelling given that their location, distance, and age were consistent with the gravitational-wave event, and their early optical lightcurves were photometrically consistent with that of kilonovae. These two candidates were spectroscopically classified as young core-collapse supernovae. The remaining candidates were photometrically or spectroscopically ruled-out as supernovae. Palomar Gattini-IR identified one fast evolving infrared transient after the merger, PGIR19bn, which was later spectroscopically classified as an M-dwarf flare. [abridged]


Item Type:Report or Paper (Discussion Paper)
Related URLs:
URLURL TypeDescription
http://arxiv.org/abs/1907.12645arXivDiscussion Paper
ORCID:
AuthorORCID
Coughlin, Michael W.0000-0002-8262-2924
Ahumada, Tomás0000-0002-2184-6430
De, Kishalay0000-0002-8989-0542
Hankins, Matthew J.0000-0001-9315-8437
Kasliwal, Mansi M.0000-0002-5619-4938
Singer, Leo P.0000-0001-9898-5597
Bellm, Eric C.0000-0001-8018-5348
Andreoni, Igor0000-0002-8977-1498
Cenko, S. Bradley0000-0003-1673-970X
Jencson, Jacob E.0000-0001-5754-4007
Perley, Daniel A.0000-0001-8472-1996
Yu, Po-Chieh0000-0001-8894-0854
Bloom, Joshua S.0000-0002-7777-216X
Burdge, Kevin B.0000-0002-7226-836X
Cook, David O.0000-0002-6877-7655
Duev, Dmitry A.0000-0001-5060-8733
Frederick, Sara0000-0001-9676-730X
Gatkine, Pradip0000-0002-1955-2230
Ghosh, Shaon0000-0001-9901-6253
Goldstein, Daniel A.0000-0003-3461-8661
Golkhou, V. Zach0000-0001-8205-2506
Goobar, Ariel0000-0002-4163-4996
Graham, Matthew J.0000-0002-3168-0139
Hung, Tiara0000-0002-9878-7889
Kong, Albert K. H.0000-0002-5105-344X
Kaplan, David L.0000-0001-6295-2881
Kulkarni, Shrinivas R.0000-0001-5390-8563
Kupfer, Thomas0000-0002-6540-1484
Masci, Frank J.0000-0002-8532-9395
Moore, Anna M. 0000-0002-2894-6936
Neill, James D.0000-0002-0466-1119
Ngeow, Chow-Choong0000-0001-8771-7554
Martínez-Palomera, Jorge0000-0002-7395-4935
Ofek, Eran O.0000-0002-6786-8774
Riddle, Reed0000-0002-0387-370X
Rusholme, Ben0000-0001-7648-4142
Shupe, David L.0000-0003-4401-0430
Sollerman, Jesper0000-0003-1546-6615
Taggart, Kirsty0000-0002-5748-4558
Additional Information:We would like to thank Peter Nugent for comments on an early version of this paper. This work was supported by the GROWTH (Global Relay of Observatories Watching Transients Happen) project funded by the National Science Foundation under PIRE Grant No 1545949. GROWTH is a collaborative project among California Institute of Technology (USA), University of Maryland College Park (USA), University of Wisconsin Milwaukee (USA), Texas Tech University (USA), San Diego State University (USA), University of Washington (USA), Los Alamos National Laboratory (USA), Tokyo Institute of Technology (Japan), National Central University (Taiwan), Indian Institute of Astrophysics (India), Indian Institute of Technology Bombay (India), Weizmann Institute of Science (Israel), The Oskar Klein Centre at Stockholm University (Sweden), Humboldt University (Germany), Liverpool John Moores University (UK) and University of Sydney (Australia). Based on observations made with the Liverpool Telescope 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. 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 research used resources of the National Energy Research Scientific Computing Center, a DOE Office of Science User Facility supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. The 0.7m GROWTH-India Telescope (GIT) is set up by the Indian Institute of Astrophysics (IIA) and the Indian Institute of Technology Bombay (IITB) with support from the Indo-US Science and Technology Forum (IUSSTF) and the Science and Engineering Research Board (SERB) of the Department of Science and Technology (DST), Government of India Grant No.IUSSTF/PIRE Program/GROWTH/2015-16. It is located at the Indian Astronomical Observatory, IIA at Hanle, Ladakh (India). This publication has made use of data collected at Lulin Observatory, partly supported by MoST grant 105-2112-M-008-024-MY3. The KPED team thanks the National Science Foundation and the National Optical Astronomical Observatory for making the Kitt Peak 2.1-m telescope available. We thank the observatory staff at Kitt Peak for their efforts to assist Robo-AO KP operations. The KPED team thanks the National Science Foundation, the National Optical Astronomical Observatory, the Caltech Space Innovation Council and the Murty family for support in the building and operation of KPED. SED Machine is based upon work supported by the National Science Foundation under Grant No. 1106171. The Palomar GattiniIR project thanks the Mount Cuba Foundation, Heising Simons Foundation, the ANU Futures Scheme, the Binational Science Foundation and Caltech for generous support. G.C. Anupama and Varun Bhalerao acknowledge partial support from SERB and IUSSTF. J. Sollerman acknowledges support from the Knut and Alice Wallenberg Foundation. E. Ofek is grateful for support by a grant from the Israeli Ministry of Science, ISF, Minerva, BSF, BSF transformative program, and the I-CORE Program of the Planning and Budgeting Committee and The Israel Science Foundation (grant No 1829/12). P. Gatkine is supported by NASA Earth and Space Science Fellowship (ASTRO18F-0085). C.-C. Ngeow, A. Patil and P.- C. Yu thank the funding from Ministry of Science and Technology (Taiwan) under grants 104-2923-M-008-004- MY5, 106-2112-M-008-007, 107-2119-M-008-012, 107-2119-M-008-014-MY2 E. Bellm and V. Z. Golkhou acknowledge support from the University of Washington College of Arts and Sciences, Department of Astronomy, and the DIRAC Institute. University of Washington’s DIRAC Institute is supported through generous gifts from the Charles and Lisa Simonyi Fund for Arts and Sciences, and the Washington Research Foundation. E. Bellm acknowledges support from the Large Synoptic Survey Telescope, which is supported in part by the National Science Foundation through Cooperative Agreement 1258333 managed by the Association of Universities for Research in Astronomy (AURA), and the Department of Energy under Contract No. DEAC02-76SF00515 with the SLAC National Accelerator Laboratory. Additional LSST funding comes from private donations, grants to universities, and in-kind support from LSSTC Institutional Members. E. Bellm is supported in part by the NSF AAG grant 1812779 and grant #2018-0908 from the Heising-Simons Foundation. M. W. Coughlin is supported by the David and Ellen Lee Postdoctoral Fellowship at the California Institute of Technology. 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. D. L. Kaplan was supported by NSF grant AST-1816492. A. K. H. Kong acknowledges support from the Ministry of Science and Technology of the Republic of China (Taiwan) under grants 106- 2628-M-007-005 and 107-2628-M-007-003. J. S. Bloom and J. Martinez-Palomera are partially supported by a Gordon and Betty Moore Foundation Data-Driven Discovery grant. Harsh Kumar thanks the LSSTC Data Science Fellowship Program, which is funded by LSSTC, NSF Cybertraining Grant #1829740, the Brinson Foundation, and the Moore Foundation; his participation in the program has benefited this work. S. Anand acknowledges support from the PMA Division Medberry Fellowship at the California Institute of Technology. Rahul Biswas, Ariel Goobar and Jesper Sollerman acknowledge support from the G.R.E.A.T research environment funded by the Swedish National Science Foundation. J. Soon acknowledges support by an Australian Government Research Training Program (RTP) Scholarship.
Group:Zwicky Transient Facility, Infrared Processing and Analysis Center (IPAC)
Funders:
Funding AgencyGrant Number
NSFAST-1545949
NSFAST-1440341
Department of Energy (DOE)DE-AC02-05CH11231
Indo-US Science and Technology ForumUNSPECIFIED
Science and Engineering Research Board (SERB)GROWTH/2015-16
Ministry of Science and Technology (Taipei)105-2112-M-008-024-MY3
NSFAST-1106171
Mt. Cuba Astronomical FoundationUNSPECIFIED
Caltech Space Innovation CouncilUNSPECIFIED
National Optical Astronomy Observatory (NOAO)UNSPECIFIED
Murty familyUNSPECIFIED
Heising-Simons Foundation2018-0908
Australian National UniversityUNSPECIFIED
Binational Science Foundation (USA-Israel)UNSPECIFIED
Knut and Alice Wallenberg FoundationUNSPECIFIED
Ministry of Science (Israel)UNSPECIFIED
Israel Science Foundation1829/12
MINERVA (Israel)UNSPECIFIED
I-CORE Program of the Planning and Budgeting CommitteeUNSPECIFIED
NASA Earth and Space Science Fellowship ASTRO18F-0085
Ministry of Science and Technology (Taipei)104-2923-M-008-004-MY5
Ministry of Science and Technology (Taipei)106-2112-M-008-007
Ministry of Science and Technology (Taipei)107-2119-M-008-012
Ministry of Science and Technology (Taipei)107-2119-M-008-014-MY2
University of WashingtonUNSPECIFIED
DIRAC InstituteUNSPECIFIED
Charles and Lisa Simonyi Fund for Arts and SciencesUNSPECIFIED
Washington Research FoundationUNSPECIFIED
Large Synoptic Survey Telescope CorporationUNSPECIFIED
Association of Universities for Research in Astronomy (AURA)UNSPECIFIED
Department of Energy (DOE)DE-AC02-76SF00515
NSFAAG-1812779
David and Ellen Lee Postdoctoral ScholarshipUNSPECIFIED
NASA/JPL/CaltechUNSPECIFIED
NSFAST-1816492
Ministry of Science and Technology (Taipei)106-2628-M-007-005
Ministry of Science and Technology (Taipei)107-2628-M-007-003
Gordon and Betty Moore FoundationUNSPECIFIED
NSFOAC-1829740
Brinson FoundationUNSPECIFIED
Chauncey Medberry Endowed Graduate FellowshipUNSPECIFIED
Swedish Research CouncilUNSPECIFIED
Australian Government Research Training ProgramUNSPECIFIED
NSFAST-1258333
Record Number:CaltechAUTHORS:20190802-094555948
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190802-094555948
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:97615
Collection:CaltechAUTHORS
Deposited By: Joy Painter
Deposited On:02 Aug 2019 18:16
Last Modified:19 Nov 2019 22:49

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