Deposited in DRO : 16 February 2018 Version of attached le : Published Version Peer-review status of attached le :

Shivani Bhandari,E. F. Keane, Elizabeth Barr, Allon Jameson, Elena Petroff, Shayne Johnston,Matthew Bailes,N. D. Ramesh Bhat,Marta Burgay,Sarah Burke-Spolaor,M. Caleb,Ralph P. Eatough, Cormac Flynn,James A. Green,Fabian Jankowski,Michael Kramer,V. Venkatraman Krishnan,V. Morello,Andrea Possenti,Ben W Stappers,Caterina Tiburzi,Willem van Straten,Igor Andreoni,Tim Butterley, Poonam Chandra,Jeffery Cooke,Alessandro Corongiu,D. M. Coward,Vik S. Dhillon,Richard Dodson, Liam K Hardy,Eric J. Howell,Phrudth Jaroenjittichai,Alain Klotz,Stuart P. Littlefair,T. R. Marsh,Mitchell B. Mickaliger, T. Muxlow, Didier Perrodin,T. Pritchard,U. Sawangwit, Tomoyuki Terai,Nozomu Tominaga,Pablo Torné,Tomonori Totani,Alessio Trois,Damien Turpin,Yuu Niino, Robert W. Wilson,A. Albert, Markus André,Marco Anghinolfi,Gisela Anton,Miguel Ardid,J. J. Aubert,T. Avgitas,Bruny Baret,Stéphane Basa,B. Belhorma,Vincent Bertin, Stefano Biagi,R. Bormuth,Simon Bourret,M. C. Bouwhuis,Horea Branzas, Roland de Bruijn, Julian Brunner,J. Busto,Antonio Capone,Laurenctiu I. Caramete,J. Carr,Silvia Celli,R. Cherkaoui El Moursli,Tommaso Chiarusi,Marco Circella,J. A. B. Coelho,Alexis Coleiro,Rosa Coniglione,Heide Costantini,P. Coyle,Alexandre Creusot,Anne Deschamps,Giulia De Bonis,Carla Distefano,I. Di Palma,Alba Domi,Corinne Donzaud,Damien Dornic,Doriane Drouhin,T Eberl,I. El Bojaddaini,N. El Khayati,Dominik Elsaesser,Andreas Enzenhöfer,A. Ettahiri,Farida Fassi,Ivan Felis,L. A. Fusco,Pascal Gay,Valentina Giordano,Hervé Glotin,Timothée Grégoire,R. Gracia-Ruiz,Kaspar Graf, Sandy Hallmann,Hans van Haren,A. J. Heijboer,Y. Hello,Juan José Hernández-Rey,J. Hoessl,Jannik Hofestädt,Christophe Hugon,Giulia Illuminati,Clancy W. James,M. de Jong,M. Jongen,Matthias Kadler,Oleg Kalekin,U. Katz,D. Kiessling,Antoine Kouchner, Maximilian Kreter,Ingo Kreykenbohm,Vladimir Kulikovskiy,Cyril Lachaud,Robert Lahmann,Dominique Lefèvre,Emanuele Leonora,Sotiris Loucatos, Michael Marcelin,A. Margiotta, Agostino Marinelli,R. Mele,K. W. Melis,T. Michael,Pasquale Migliozzi, Aboubacar Moussa,S. Navas,Emmanuel Nezri,Mukharbek Organokov,Gabriela Emilia Pǎvǎlaş,Carmelo Pellegrino, Chiara Perrina,Paolo Piattelli,V. Popa,Thierry Pradier,L. Quinn,C. Racca,Giuseppe Riccobene,Agust'in S'anchez-Losa,Melanie Saldana,Ilenia Salvadori,D. F. E. Samtleben,M Sanguineti,Piera Sapienza,F. Schuessler,C. Sieger,Maurizio Spurio,Th. Stolarczyk, Martina Taiuti,Yahya Tayalati,Agata Trovato,Christoph Tönnis

semanticscholar(2018)

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Abstract
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 multimessenger 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 fits 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 fluences >2 Jy ms is α = −2.2+0.6 −1.2 and still consistent with a Euclidean distribution (α = −3/2). We also find that the all-sky rate is 1.7+1.5 −0.9 × 103FRBs/(4π sr)/day above ∼2 Jy ms and there is currently no strong evidence for a latitude-dependent FRB sky rate.
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