{"refrec":{"BRefID":291439,"RR":"<b>Petroff, E.; van Haren, H.; The ANTARES Collaboration; The H.E.S.S. Collaboration</b> (2017). A polarized fast radio burst at low Galactic latitude. <i>Monthly Notices of the Royal Astronomical Society 469(4)</i>: 4465–4482. <a href=\"https://doi.org/10.1093/mnras/stx1098\" target=\"_blank\">https://doi.org/10.1093/mnras/stx1098</a>","BEntID":283482,"PublicFlag":1,"CheckedFlag":1,"wosflag":1,"vabbflag":1,"RefStringPartII":". <i>Monthly Notices of the Royal Astronomical Society 469(4)</i>: 4465–4482. <a href=\"https://doi.org/10.1093/mnras/stx1098\" target=\"_blank\">https://doi.org/10.1093/mnras/stx1098</a>","DocTypID":8,"DocType":"Journal article","MarineFlag":0,"FreshFlag":0,"BrackishFlag":0,"TerrestrialFlag":0,"Authorstring":"Petroff, E.; van Haren, H.; The ANTARES Collaboration; The H.E.S.S. Collaboration","OrigTitleTranslFlag":0,"Authorstringtrunc":"Petroff, E. <i>et al.</i>","Englishabstract":"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+0.2−0.1Jy. 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.","AbstractOtherLang":null,"BibLvlCode":"AS","StandardTitle":"A polarized fast radio burst at low Galactic latitude","OrigTitleLangCode":"en","OrigTitleLangCodeExtended":"eng","OrigTitleLangID":15,"DateLastModified":{"date":"2024-12-10 01:32:52.928458","timezone_type":1,"timezone":"+01:00"},"UserAccessRight":null,"UserAccID":null,"AuthorKeywords":"surveys; methods: data analysis; polarization; ISM: structure","OtherDescriptors":null,"Notes":null,"AnaPub":2017,"MonPub":null,"DateUpdate":"2020-10-22","DateCreate":"2017-12-14","SecASFANote":null,"ConfID":null,"PeerRev":1,"VlizCoreFlag":1,"WoScode":"WOS:000406837900051","VABBcode":null,"OpenAcc":1,"DOI":"10.1093/mnras/stx1098"},"refs":null,"anarec":{"AnaID":291439,"PubliDate":2017,"Pagination":"4465–4482","XtraPublOfAnaID":null,"ISBN":null,"Volume":"469","Issue":"4","BRefMon":null,"BRefMonRR":null,"BRefXtra":null,"BRefXtraRR":null,"SerBRefID":274984,"SerRR":"Monthly Notices of the Royal Astronomical Society. 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