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The SUrvey for Pulsars and Extragalactic Radio Bursts - II. New FRB discoveries and their follow-up

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The SUrvey for Pulsars and Extragalactic Radio Bursts - II. New FRB discoveries and their follow-up

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dc.contributor.author Bhandari, S. es_ES
dc.contributor.author Keane, E. F. es_ES
dc.contributor.author Barr, E. D. es_ES
dc.contributor.author Jameson, A. es_ES
dc.contributor.author Petroff, E. es_ES
dc.contributor.author Johnston, S. es_ES
dc.contributor.author Bailes, M. es_ES
dc.contributor.author Bhat, N. D. R. es_ES
dc.contributor.author Burgay, M. es_ES
dc.contributor.author Burke-Spolaor, S. es_ES
dc.contributor.author Caleb, M. es_ES
dc.contributor.author Eatough, R. P. es_ES
dc.contributor.author Flynn, C. es_ES
dc.contributor.author Green, J. A. es_ES
dc.contributor.author Jankowski, F. es_ES
dc.contributor.author Ardid Ramírez, Miguel es_ES
dc.contributor.author Felis-Enguix, Iván es_ES
dc.contributor.author Martínez Mora, Juan Antonio es_ES
dc.contributor.author Saldaña-Coscollar, María es_ES
dc.date.accessioned 2020-05-14T03:04:15Z
dc.date.available 2020-05-14T03:04:15Z
dc.date.issued 2018-04 es_ES
dc.identifier.issn 0035-8711 es_ES
dc.identifier.uri http://hdl.handle.net/10251/143124
dc.description.abstract [EN] We report the discovery of four Fast Radio Bursts (FRBs) in the ongoing SUrvey for Pulsars and Extragalactic Radio Bursts at the Parkes Radio Telescope: FRBs 150610, 151206, 151230 and 160102. Our real-time discoveries have enabled us to conduct extensive, rapid multimes-senger follow-up at 12 major facilities sensitive to radio, optical, X-ray, gamma-ray photons and neutrinos on time-scales ranging from an hour to a few months post-burst. No counterparts to the FRBs were found and we provide upper limits on afterglow luminosities. None of the FRBs were seen to repeat. Formal ¿ts to all FRBs show hints of scattering while their intrinsic widths are unresolved in time. FRB 151206 is at low Galactic latitude, FRB 151230 shows a sharp spectral cut-off, and FRB 160102 has the highest dispersion measure (DM = 2596.1 ± 0.3 pc cm¿3) detected to date. Three of the FRBs have high dispersion measures (DM > 1500 pc cm¿3), favouring a scenario where the DM is dominated by contributions from the intergalactic medium. The slope of the Parkes FRB source counts distribution with ¿uences >2Jyms is ¿ =¿2.2+01..62 and still consistent with a Euclidean distribution (¿ =¿3/2). We also ¿nd that the all-sk¿y rate is 1.7+¿10..59 × 103FRBs/(4¿ sr)/day above ~2 Jy ms and there is currently no strong evidence for a latitude-dependent FRB sky rate. es_ES
dc.description.sponsorship The Parkes radio telescope and the Australia Telescope Compact Array are part of the Australia Telescope National Facility which is funded by the Commonwealth of Australia for operation as a National Facility managed by CSIRO. Parts of this research were conducted by the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through project number CE110001020. The GMRT is run by the National Centre for Radio Astrophysics of the Tata Institute of Fundamental Research. VLAis run by the NationalRadio Astronomy Observatory (NRAO). NRAO is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. This work was performed on the gSTAR national facility at Swinburne University of Technology. gSTAR is funded by Swinburne and the Australian Government's Education Investment Fund. This work is also based on data collected at Subaru Telescope, which is operated by the National Astronomical Observatory of Japan. We thank the LSST Project for making their code available as free software at http://dm.lsstcorp.org. Funding from the European Research Council under the European Union's Seventh Framework Programme (FP/2007-2013)/ERC Grant Agreement no. 617199 (EP). Access to the Lovell Telescope is supported through an STFC consolidated grant. The 100-m telescope in Effelsberg is operation by the MaxPlanck-Institut fur Radioastronomie with funds of the Max-Planck Society. The Sardinia Radio Telescope (SRT) is funded by the Department of University and Research (MIUR), the Italian Space Agency (ASI), and the Autonomous Region of Sardinia (RAS) and is operated as National Facility by the National Institute for Astrophysics (INAF). TB and RWW are grateful to the STFC for financial support (grant reference ST/P000541/1). Research support to IA is provided by the Australian Astronomical Observatory. The ANTARES authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commissariat a l' energie atomique et aux energies alternatives (CEA), Commission Europeenne (FEDER fund and Marie Curie Programme), Institut Universitaire de France (IUF), IdEx programme and UnivEarthS Labex programme at Sorbonne Paris Cite (ANR-10-LABX-0023 and ANR-11-IDEX-0005-02), Labex OCEVU (ANR-11-LABX-0060) and the A*MIDEX project (ANR-11-IDEX-0001-02), Region Ile-de-France (DIM-ACAV), Region Alsace (contrat CPER), Region Provence-Alpes-Cote d'Azur, Departement du Var and Ville de La Seyne-sur-Mer, France; Bundesministerium fur Bildung und Forschung (BMBF), Germany; Istituto Nazionale di Fisica Nucleare (INFN), Italy; Stichting voor Fundamenteel Onderzoek der Materie (FOM), Nederlandse organisatie voorWetenschappelijk Onderzoek (NWO), the Netherlands; Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia; National Authority for Scientific Research (ANCS), Romania; Ministerio de Economia y Competitividad (MINECO): Plan Estatal de Investigacion (refs. FPA2015-65150C3-1-P, -2-P and -3-P, (MINECO/FEDER)), Severo Ochoa Centre of Excellence and MultiDark Consolider (MINECO), and Prometeo and Grisolia Programmes (Generalitat Valenciana), Spain; Ministry of Higher Education, Scientific Research and Professional Training, Morocco. We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea operation and the CC-IN2P3 for the computing facilities. This work used data supplied by the UK Swift Science Data Centre at the University of Leicester. es_ES
dc.language Inglés es_ES
dc.publisher Oxford University Press es_ES
dc.relation.ispartof Monthly Notices of the Royal Astronomical Society es_ES
dc.rights Reserva de todos los derechos es_ES
dc.subject Radiation mechanisms: general es_ES
dc.subject Methods: data analysis es_ES
dc.subject Methods: observational es_ES
dc.subject Surveys es_ES
dc.subject Intergalactic medium es_ES
dc.subject Radio continuum: general es_ES
dc.subject.classification FISICA APLICADA es_ES
dc.title The SUrvey for Pulsars and Extragalactic Radio Bursts - II. New FRB discoveries and their follow-up es_ES
dc.type Artículo es_ES
dc.identifier.doi 10.1093/mnras/stx3074 es_ES
dc.relation.projectID info:eu-repo/grantAgreement/EC/FP7/610058/EU/Imaging the Event Horizon of Black Holes/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/MINECO//FPA2015-65150-C3-1-P/ES/PARTICIPACION DEL IFIC EN ANTARES, KM3NET-ARCA%2FORCA Y PDG/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/ERC/FP7/617199/EU/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/CAASTRO//CE110001020/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/UKRI//ST%2FP000541%2F1/GB/Durham Astronomy Consolidated Grant 2017-2020/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/ANR//ANR-11-LABX-0060/FR/Origines, Constituants et EVolution de l'Univers/OCEVU/FR/Origines, Constituants et EVolution de l'Univers/OCEVU/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/ANR//ANR-11-IDEX-0005/FR/Université Sorbonne Paris Cité/USPC/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/ANR//ANR-11-IDEX-0001/FR/INITIATIVE D'EXCELLENCE AIX MARSEILLE UNIVERSITE/Amidex/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/ANR//ANR-10-LABX-0023/FR/Earth - Planets - Universe: observation, modeling, transfer/UnivEarthS/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/MINECO//FPA2015-65150-C3-3-P/ES/PARTICIPACION DE LA UGR EN ANTARES, KM3NET-ARCA%2FORCA Y PDG/ es_ES
dc.rights.accessRights Abierto es_ES
dc.contributor.affiliation Universitat Politècnica de València. Departamento de Física Aplicada - Departament de Física Aplicada es_ES
dc.description.bibliographicCitation Bhandari, S.; Keane, EF.; Barr, ED.; Jameson, A.; Petroff, E.; Johnston, S.; Bailes, M.... (2018). The SUrvey for Pulsars and Extragalactic Radio Bursts - II. New FRB discoveries and their follow-up. Monthly Notices of the Royal Astronomical Society. 475(2):1427-1446. https://doi.org/10.1093/mnras/stx3074 es_ES
dc.description.accrualMethod S es_ES
dc.relation.publisherversion https://doi.org/10.1093/mnras/stx3074 es_ES
dc.description.upvformatpinicio 1427 es_ES
dc.description.upvformatpfin 1446 es_ES
dc.type.version info:eu-repo/semantics/publishedVersion es_ES
dc.description.volume 475 es_ES
dc.description.issue 2 es_ES
dc.relation.pasarela S\367330 es_ES
dc.contributor.funder Agence Nationale de la Recherche, Francia es_ES
dc.contributor.funder UK Research and Innovation es_ES
dc.contributor.funder Max Planck Society es_ES
dc.contributor.funder European Commission es_ES
dc.contributor.funder Conseil Régional, Île-de-France es_ES
dc.contributor.funder Australian Government es_ES
dc.contributor.funder Generalitat Valenciana es_ES
dc.contributor.funder Agenzia Spaziale Italiana es_ES
dc.contributor.funder Conseil Régional d'Alsace es_ES
dc.contributor.funder Australian Research Council es_ES
dc.contributor.funder Regione Autonoma della Sardegna es_ES
dc.contributor.funder Université Sorbonne Paris Cité es_ES
dc.contributor.funder Institut Universitaire de France es_ES
dc.contributor.funder European Regional Development Fund es_ES
dc.contributor.funder Swinburne University of Technology es_ES
dc.contributor.funder Australian Astronomical Observatory es_ES
dc.contributor.funder Instituto Nazionale di Fisica Nucleare es_ES
dc.contributor.funder Ministerio de Economía y Competitividad es_ES
dc.contributor.funder Conseil Régional Provence-Alpes-Côte d'Azur es_ES
dc.contributor.funder Département du Var and Ville de La Seyne-sur-Mer es_ES
dc.contributor.funder Ministero dell'università e della ricerca, Italia es_ES
dc.contributor.funder National Authority for Scientific Research, Rumanía es_ES
dc.contributor.funder Bundesministerium für Bildung und Forschung, Alemania es_ES
dc.contributor.funder Centre National de la Recherche Scientifique, Francia es_ES
dc.contributor.funder Science and Technology Facilities Council, Reino Unido es_ES
dc.contributor.funder Netherlands Organization for Scientific Research es_ES
dc.contributor.funder Foundation for Fundamental Research on Matter, Holanda es_ES
dc.contributor.funder Council on grants of the President of the Russian Federation es_ES
dc.contributor.funder Commissariat à l'Énergie Atomique et aux Énergies Alternatives, Francia es_ES
dc.contributor.funder Laboratoire d'Excellence OCEVU (Origines, Constituants & ÉVolution de l'Univers) es_ES
dc.contributor.funder Ministère de l'Education Nationale, de la Formation professionnelle, de l'Enseignement Supérieur et de la Recherche Scientifique, Marruecos es_ES
dc.contributor.funder ARC Centre of Excellence for All-sky Astrophysics
dc.contributor.funder European Research Council
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