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LOFAR 144-MHz follow-up observations of GW170817

Broderick, J. W. and Shimwell, T. W. and Gourdji, K. and Rowlinson, A. and Nissanke, S. and Hotokezaka, K. and Jonker, P. G. and Tasse, C. and Hardcastle, M. J. and Oonk, J. B. R. and Fender, R. P. and Wijers, R. A. M. J. and Shulevski, A. and Stewart, A. J. and ter Veen, S. and Moss, V. A. and van der Wiel, M. H. D. and Nichols, D. A. and Piette, A. and Bell, M. E. and Carbone, D. and Corbel, S. and Eislöffel, J. and Grießmeier, J.-M. and Keane, E. F. and Law, C. J. and Muñoz-Darias, T. and Pietka, M. and Serylak, M. and van der Horst, A. J. and van Leeuwen, J. and Wijnands, R. and Zarka, P. and Anderson, J. M. and Bentum, M. J. and Blaauw, R. and Brouw, W. N. and Brüggen, M. and Ciardi, B. and de Vos, M. and Duscha, S. and Fallows, R. A. and Franzen, T. M. O. and Garrett, M. A. and Gunst, A. W. and Hoeft, M. and Hörandel, J. R. and Iacobelli, M. and Jütte, E. and Koopmans, L. V. E. and Krankowski, A. and Maat, P. and Mann, G. and Mulder, H. and Nelles, A. and Paas, H. and Pandey-Pommier, M. and Pekal, R. and Reich, W. and Röttgering, H. J. A. and Schwarz, D. J. and Smirnov, O. and Soida, M. and Toribio, M. C. and van Haarlem, M. P. and van Weeren, R. J. and Vocks, C. and Wucknitz, O. and Zucca, P. (2020) LOFAR 144-MHz follow-up observations of GW170817. Monthly Notices of the Royal Astronomical Society, 494 (4). pp. 5110-5117. ISSN 0035-8711. https://resolver.caltech.edu/CaltechAUTHORS:20200625-112850820

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Abstract

We present low-radio-frequency follow-up observations of AT 2017gfo, the electromagnetic counterpart of GW170817, which was the first binary neutron star merger to be detected by Advanced LIGO–Virgo. These data, with a central frequency of 144 MHz, were obtained with LOFAR, the Low-Frequency Array. The maximum elevation of the target is just 13∘.7 when observed with LOFAR, making our observations particularly challenging to calibrate and significantly limiting the achievable sensitivity. On time-scales of 130–138 and 371–374 d after the merger event, we obtain 3σ upper limits for the afterglow component of 6.6 and 19.5 mJy beam⁻¹, respectively. Using our best upper limit and previously published, contemporaneous higher frequency radio data, we place a limit on any potential steepening of the radio spectrum between 610 and 144 MHz: the two-point spectral index α^(610)_(144) ≳ −2.5. We also show that LOFAR can detect the afterglows of future binary neutron star merger events occurring at more favourable elevations.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1093/mnras/staa950DOIArticle
https://arxiv.org/abs/2004.01726arXivDiscussion Paper
ORCID:
AuthorORCID
Broderick, J. W.0000-0002-2239-6099
Gourdji, K.0000-0002-0152-1129
Rowlinson, A.0000-0002-1195-7022
Nissanke, S.0000-0001-6573-7773
Hotokezaka, K.0000-0002-2502-3730
Jonker, P. G.0000-0001-5679-0695
Hardcastle, M. J.0000-0003-4223-1117
Wijers, R. A. M. J.0000-0002-3101-1808
Shulevski, A.0000-0002-1827-0469
Stewart, A. J.0000-0001-8026-5903
Moss, V. A.0000-0002-3005-9738
Piette, A.0000-0002-4487-5533
Carbone, D.0000-0002-6575-4642
Keane, E. F.0000-0002-4553-655X
Law, C. J.0000-0002-4119-9963
van der Horst, A. J.0000-0001-9149-6707
Koopmans, L. V. E.0000-0003-1840-0312
Additional Information:© 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. This article is published and distributed under the terms of the Oxford University Press, Standard Journals Publication Model (https://academic.oup.com/journals/pages/open_access/funder_policies/chorus/standard_publication_model) Accepted 2020 March 23. Received 2020 March 10; in original form 2019 October 5. We thank the referee for a number of helpful suggestions that improved the content and presentation of this paper. We also thank the ASTRON Radio Observatory for setting up and scheduling the observations described in this paper, as well as preprocessing the data. Additionally, we are grateful to Ben Stappers for providing very useful feedback on an earlier version of this manuscript. This paper is based on data obtained with the International LOFAR Telescope (ILT) under project codes DDT9_002 and LT10_013. LOFAR (van Haarlem et al. 2013) is the Low Frequency Array designed and constructed by ASTRON. It has observing, data processing, and data storage facilities in several countries, that are owned by various parties (each with their own funding sources), and that are collectively operated by the ILT foundation under a joint scientific policy. The ILT resources have benefitted from the following recent major funding sources: CNRS-INSU, Observatoire de Paris and Université d’Orléans, France; BMBF, MIWF-NRW, MPG, Germany; Science Foundation Ireland (SFI), Department of Business, Enterprise and Innovation (DBEI), Ireland; NWO, The Netherlands; The Science and Technology Facilities Council, UK; Ministry of Science and Higher Education, Poland. The LOFAR direction-independent calibration pipeline (https://github.com/lofar-astron/prefactor) was deployed by the LOFAR e-infragroup on the Dutch National Grid infrastructure with support of the SURF Co-operative through grants e-infra170194, e-infra180087, and e-infra180169 (Mechev et al. 2017). The LOFAR direction-dependent calibration and imaging pipeline (http://github.com/mhardcastle/ddf-pipeline/) was run on computing clusters at Leiden Observatory and the University of Hertfordshire, which are supported by a European Research Council Advanced Grant [NEWCLUSTERS-321271] and the UK Science and Technology Funding Council [ST/P000096/1]. PGJ acknowledges funding from the European Research Council under ERC Consolidator Grant agreement no. 647208. SC acknowledges funding support from the UnivEarthS Labex program of Sorbonne Paris Cité (ANR-10-LABX-0023 and ANR-11-IDEX-0005-02). TMD acknowledges support from grants AYA2017-83216-P and RYC-2015-18148. JvL acknowledges funding from Vici research programme ‘ARGO’ with project number 639.043.815, financed by the Netherlands Organisation for Scientific Research (NWO). MB acknowledges support by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) under Germany’s Excellence Strategy – EXC 2121 ‘Quantum Universe’ – 390833306. This research has made use of the VizieR catalogue access tool, CDS, Strasbourg, France (DOI: 10.26093/cds/vizier). The original description of the VizieR service was published in A&AS 143, 23 (Ochsenbein, Bauer & Marcout 2000). This research has made use of the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. This research has made use of NASA’s Astrophysics Data System Bibliographic Services. This project also made use of KVIS (Gooch 1995), TOPCAT (Taylor 2005), NUMPY (Oliphant 2006), and MATPLOTLIB (Hunter 2007).
Funders:
Funding AgencyGrant Number
Centre National de la Recherche Scientifique (CNRS)UNSPECIFIED
Institut national des sciences de l'Univers (INSU)UNSPECIFIED
Observatoire de ParisUNSPECIFIED
Université d’OrléansUNSPECIFIED
Bundesministerium für Bildung und Forschung (BMBF)UNSPECIFIED
Ministerium für Innovation, Wissenschaft und Forschung des Landes Nordrhein-WestfalenUNSPECIFIED
Max-Planck-GesellschaftUNSPECIFIED
Science Foundation, IrelandUNSPECIFIED
Department of Business, Enterprise and Innovation (Ireland)UNSPECIFIED
Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)UNSPECIFIED
Science and Technology Facilities Council (STFC)ST/P000096/1
Ministry of Science and Higher Education (Poland)UNSPECIFIED
Nordrhein-Westfalen Ministerium für Kultur und WissenschaftUNSPECIFIED
SURF (Netherlands)e-infra170194
SURF (Netherlands)e-infra180087
SURF (Netherlands)e-infra180169
European Research Council (ERC)321271
European Research Council (ERC)647208
Agence Nationale pour la Recherche (ANR)ANR-10-LABX-0023
Agence Nationale pour la Recherche (ANR)ANR-11-IDEX-0005-02
Ministerio de Economía, Industria y Competitividad (MINECO)AYA2017-83216-P
Ramón y Cajal FellowshipRYC-2015-18148
Deutsche Forschungsgemeinschaft (DFG)390833306
NASA/JPL/CaltechUNSPECIFIED
Subject Keywords:gravitational waves, stars: neutron, radio continuum: stars
Issue or Number:4
Record Number:CaltechAUTHORS:20200625-112850820
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20200625-112850820
Official Citation:J W Broderick, T W Shimwell, K Gourdji, A Rowlinson, S Nissanke, K Hotokezaka, P G Jonker, C Tasse, M J Hardcastle, J B R Oonk, R P Fender, R A M J Wijers, A Shulevski, A J Stewart, S ter Veen, V A Moss, M H D van der Wiel, D A Nichols, A Piette, M E Bell, D Carbone, S Corbel, J Eislöffel, J-M Grießmeier, E F Keane, C J Law, T Muñoz-Darias, M Pietka, M Serylak, A J van der Horst, J van Leeuwen, R Wijnands, P Zarka, J M Anderson, M J Bentum, R Blaauw, W N Brouw, M Brüggen, B Ciardi, M de Vos, S Duscha, R A Fallows, T M O Franzen, M A Garrett, A W Gunst, M Hoeft, J R Hörandel, M Iacobelli, E Jütte, L V E Koopmans, A Krankowski, P Maat, G Mann, H Mulder, A Nelles, H Paas, M Pandey-Pommier, R Pekal, W Reich, H J A Röttgering, D J Schwarz, O Smirnov, M Soida, M C Toribio, M P van Haarlem, R J van Weeren, C Vocks, O Wucknitz, P Zucca, LOFAR 144-MHz follow-up observations of GW170817, Monthly Notices of the Royal Astronomical Society, Volume 494, Issue 4, June 2020, Pages 5110–5117, https://doi.org/10.1093/mnras/staa950
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:104056
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:25 Jun 2020 19:17
Last Modified:25 Jun 2020 19:17

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