{"refrec":{"BRefID":255231,"RR":"<b>Adrian-Martinez, S.; van Haren, H.; Antares Collaboration</b> (2016). Optical and X-ray early follow-up of ANTARES neutrino alerts. <i>Journal of Cosmology and Astroparticle Physics 2</i>: 062. <a href=\"https://dx.doi.org/10.1088/1475-7516/2016/02/062\" target=\"_blank\">https://dx.doi.org/10.1088/1475-7516/2016/02/062</a>","BEntID":247234,"PublicFlag":1,"CheckedFlag":0,"wosflag":1,"vabbflag":0,"RefStringPartII":". <i>Journal of Cosmology and Astroparticle Physics 2</i>: 062. <a href=\"https://dx.doi.org/10.1088/1475-7516/2016/02/062\" target=\"_blank\">https://dx.doi.org/10.1088/1475-7516/2016/02/062</a>","DocTypID":8,"DocType":"Journal article","MarineFlag":0,"FreshFlag":0,"BrackishFlag":0,"TerrestrialFlag":0,"Authorstring":"Adrian-Martinez, S.; van Haren, H.; Antares Collaboration","OrigTitleTranslFlag":0,"Authorstringtrunc":"Adrian-Martinez, S.; van Haren, H.; Antares Collaboration","Englishabstract":"High-energy neutrinos could be produced in the interaction of charged cosmic rays withmatter or radiation surrounding astrophysical sources. Even with the recent detection of extraterrestrialhigh-energy neutrinos by the IceCube experiment, no astrophysical neutrino source has yetbeen discovered. Transient sources, such as gamma-ray bursts, core-collapse supernovae, or activegalactic nuclei are promising candidates. Multi-messenger programs o?er a unique opportunity todetect these transient sources. By combining the information provided by the ANTARES neutrinotelescope with information coming from other observatories, the probability of detecting a source isenhanced, allowing the possibility of identifying a neutrino progenitor from a single detected event.A method based on optical and X-ray follow-ups of high-energy neutrino alerts has been developedwithin the ANTARES collaboration. This program, denoted as TAToO, triggers a network of roboticoptical telescopes (TAROT and ROTSE) and the Swift-XRT with a delay of only a few seconds aftera neutrino detection, and is therefore well-suited to search for fast transient sources. To identify anoptical or X-ray counterpart to a neutrino signal, the images provided by the follow-up observationsare analysed with dedicated pipelines. A total of 42 alerts with optical and 7 alerts with X-ray imagestaken with a maximum delay of 24 hours after the neutrino trigger have been analysed. Nooptical or X-ray counterparts associated to the neutrino triggers have been found, and upper limits ontransient source magnitudes have been derived. The probability to reject the gamma-ray burst originhypothesis has been computed for each alert.","AbstractOtherLang":null,"BibLvlCode":"AS","StandardTitle":"Optical and X-ray early follow-up of ANTARES neutrino alerts","OrigTitleLangCode":"en","OrigTitleLangCodeExtended":"eng","OrigTitleLangID":15,"DateLastModified":{"date":"2024-12-10 01:33:17.368041","timezone_type":1,"timezone":"+01:00"},"UserAccessRight":null,"UserAccID":null,"AuthorKeywords":"ANTARES; Neutrino astronomy; Transient sources; Gamma-ray bursts; Optical/X-ray follow-up  ","OtherDescriptors":null,"Notes":null,"AnaPub":2016,"MonPub":null,"DateUpdate":"2020-10-22","DateCreate":"2016-04-19","SecASFANote":null,"ConfID":null,"PeerRev":1,"VlizCoreFlag":1,"WoScode":"WOS:000372467600063","VABBcode":null,"OpenAcc":1,"DOI":"10.1088/1475-7516/2016/02/062"},"refs":null,"anarec":{"AnaID":255231,"PubliDate":2016,"Pagination":"062","XtraPublOfAnaID":null,"ISBN":null,"Volume":"2","Issue":null,"BRefMon":null,"BRefMonRR":null,"BRefXtra":null,"BRefXtraRR":null,"SerBRefID":240564,"SerRR":"Journal of Cosmology and Astroparticle Physics. 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