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A polarized fast radio burst at low Galactic latitude

Title: A polarized fast radio burst at low Galactic latitude
Authors: E Petroff; S Burke-Spolaor; EF Keane; MA McLaughlin; R Miller; I Andreoni; M Bailes; ED Barr; SR Bernard; S Bhandari; NDR Bhat; M Burgay; M Caleb; D Champion; P Chandra; J Cooke; VS Dhillon; JS Farnes; LK Hardy; P Jaroenjittichai; S Johnston; M Kasliwal; M Kramer; SP Littlefair; JP Macquart; M Mickaliger; A Possenti; T Pritchard; V Ravi; A Rest; A Rowlinson; U Sawangwit; B Stappers; M Sullivan; C Tiburzi; W van Straten; A Albert; M Andre; M Anghinolfi; G Anton; M Ardid; J-J Aubert; T Avgitas; B Baret; J Barrios-Marti; S Basa; V Bertin; S Biagi; R Borrnuth; S Bourret; MC Bouwhuis; R Bruijn; J Brunner; J Busto; A Capone; L Caramete; J Carr; S Celli; T Chiarusi; M Circella; JAB Coelho; A Coleiro; R Coniglione; H Costantini; P Coyle; A Creusot; A Deschamps; G De Bonis; C Distefano; I Di Palma; C Donzaud; D Dornic; D Drouhin; T Eberl; I El Bojaddaini; D Elsasser; A Enzenhofer; I Felis; LA Fusco; S Galata; P Gay; S Geisselsoder; K Geyer; V Giordano; A Gleixner; H Glotin; T Gregoire; R Gracia-Ruiz; K Graf; S Hallmann; H van Haren; AJ Heijboer; Y Hello; JJ Hernandez-Rey; J Hossl; J Hofestadt; C Hugon; G Illuminati; CWCW James; M de Jong; M Jongen; M Kadler; O Kalekin; U Katz; D Kiessling; A Kouchner; M Kreter; I Kreykenbohm; V Kulikovskiy; C Lachaud; R Lahmann; D Lefevre; E Leonora; M Lotze; S Loucatos; M Marcelin; A Margiotta; A Marinelli; JA Martinez-Mora; A Mathieu; R Mele; K Melis; T Michael; P Migliozzi; A Moussa; C Mueller; E Nezri; GE Pavalas; C Pellegrino; C Perrina; P Piattelli; V Popa; T Pradier; L Quinn; C Racca; G Riccobene; K Roensch; A Sanchez-Losa; M Saldana; I Salvadori; DFE Samtleben; M Sanguineti; P Sapienza; J Schnabel; T Seitz; C Sieger; M Spurio; T Stolarczyk; M Taiuti; Y Tayalati; A Trovato; M Tselengidou; D Turpin; C Tonnis; B Vallage; C Vallee; V Van Elewyck; D Vivolo; A Vizzoca; S Wagner; J Wilms; JD Zornoza; J Zuniga; H Abdalla; A Abramowski; F Aharonian; FA Benkhali; AG Akhperjanian; T Andersson; EO Anguner; M Arrieta; P Aubert; M Backes; A Balzer; M Barnard; Y Becherini; JB Tjus; D Berge; S Bernhard; K Bernlohr; R Blackwell; M Bottcher; C Boisson; J Bolmont; P Bordas; J Bregeon; F Brun; P Brun; M Bryan; T Bulik; M Capasso; S Casanova; M Cerruti; N Chakraborty; R Chalme-Calvet; RCG Chaves; A Chen; J Chevalier; M Chretien; S Colafrancesco; G Cologna; B Condon; J Conrad; Y Cui; ID Davids; J Decock; B Degrange; C Deil; J Devin; P de Wilt; L Dirson; A Djannati-Atai; W Domainko; A Donath; LO Drury; G Dubus; K Dutson; J Dyks; T Edwards; K Egberts; P Eger; J-P Ernenwein; S Eschbach; C Farnier; S Fegan; MV Fernandes; A Fiasson; G Fontaine; A Forster; S Funk; M Fussling; S Gabici; M Gajdus; YA Gallant; T Garrigoux; G Giavitto; B Giebels; JF Glicenstein; D Gottschall; A Goya; M-H Grondin; D Hadasch; J Hahn; M Haupt; J Hawkes; G Heinzelmann; G Henri; G Hermann; O Hervet; JA Hinton; W Hofmann; C Hoischen; M Holler; D Horns; A Ivascenko; A Jacholkowska; M Jamrozy; M Janiak; D Jankowsky; F Jankowsky; M Jingo; T Jogler; L Jouvin; I Jung-Richardt; MA Kastendieck; K Katarzynski; D Kerszberg; B Khelifi; M Kieffer; J King; S Klepser; D Klochkov; W Kluzniak; D Kolitzus; N Komin; K Kosack; S Krakau; M Kraus; F Krayzel; PP Kruger; H Laffon; G Lamanna; J Lau; J-P Lees; J Lefaucheur; V Lefranc; A Lemiere; M Lemoine-Goumard; J-P Lenain; E Leser; T Lohse; M Lorentz; R Liu; R Lopez-Coto; I Lypova; V Marandon; A Marcowith; C Mariaud; R Marx; G Maurin; N Maxted; M Mayer; PJ Meintjes; M Meyer; AMW Mitchell; R Moderski; M Mohamed; L Mohrmann; K Mora; E Moulin; T Murach; M de Naurois; F Niederwanger; J Niemiec; L Oakes; P O'Brien; H Odaka; S Ottl; S Ohm; M Ostrowski; I Oya; M Padovani; M Panter; RD Parsons; NW Pekeur; G Pelletier; C Perennes; P-O Petrucci; B Peyaud; Q Piel; S Pita; H Poon; D Prokhorov; H Prokoph; G Puhlhofer; M Punch; A Quirrenbach; S Raab; A Reimer; O Reimer; M Renaud; R de los Reyes; F Rieger; C Romoli; S Rosier-Lees; G Rowell; B Rudak; CB Rulten; V Sahakian; D Salek; DA Sanchez; A Santangelo; M Sasaki; R Schlickeiser; A Schulz; F Schussler; U Schwanke; S Schwemmer; M Settimo; AS Seyffert; N Shafi; I Shilon; R Simoni; H Sol; F Spanier; G Spengler; F Spies; L Stawarz; R Steenkamp; C Stegmann; F Stinzing; K Stycz; I Sushch; J-P Tavernet; T Tavernier; AM Taylor; R Terrier; L Tibaldo; D Tiziani; M Tluczykont; C Trichard; R Tuffs; Y Uchiyama; DJ van der Walt; C van Eldik; C van Rensburg; B van Soelen; G Vasileiadis; J Veh; C Venter; A Viana; P Vincent; J Vink; F Voisin; HJ Volk; T Vuillaume; Z Wadiasingh; SJ Wagner; P Wagner; RM Wagner; R White; A Wierzcholska; P Willmann; A Wornlein; D Wouters; R Yang; V Zabalza; D Zaborov; M Zacharias; R Zanin; AA Zdziarski; A Zech; F Zefi; A Ziegler; N Zywucka
Publication Year: 2017
Collection: University of Leicester: Figshare
Subject Terms: Science & Technology; Physical Sciences; Astronomy & Astrophysics; polarization; methods: data analysis; surveys; ISM: structure
Description: We report on the discovery of a new fast radio burst (FRB), FRB 150215, with the Parkes radio telescope on 2015 February 15. The burst was detected in real time with a dispersion measure (DM) of 1105.6 ± 0.8 pc cm−3, a pulse duration of 2.8+1.2−0.5 ms, and a measured peak flux density assuming that the burst was at beam centre of 0.7+0.2−0.1 Jy. The FRB originated at a Galactic longitude and latitude of 24.66°, 5.28° and 25° away from the Galactic Center. The burst was found to be 43 ± 5 per cent linearly polarized with a rotation measure (RM) in the range −9 < RM < 12 rad m−2 (95 per cent confidence level), consistent with zero. The burst was followed up with 11 telescopes to search for radio, optical, X-ray, γ-ray and neutrino emission. Neither transient nor variable emission was found to be associated with the burst and no repeat pulses have been observed in 17.25 h of observing. The sightline to the burst is close to the Galactic plane and the observed physical properties of FRB 150215 demonstrate the existence of sight lines of anomalously low RM for a given electron column density. The Galactic RM foreground may approach a null value due to magnetic field reversals along the line of sight, a decreased total electron column density from the Milky Way, or some combination of these effects. A lower Galactic DM contribution might explain why this burst was detectable whereas previous searches at low latitude have had lower detection rates than those out of the plane.
Document Type: article in journal/newspaper
Language: unknown
Relation: 2381/44993; https://figshare.com/articles/journal_contribution/A_polarized_fast_radio_burst_at_low_Galactic_latitude/10213745
Availability: https://figshare.com/articles/journal_contribution/A_polarized_fast_radio_burst_at_low_Galactic_latitude/10213745
Rights: All Rights Reserved
Accession Number: edsbas.4F3644CB
Database: BASE