Multiwavelength follow-up of a rare IceCube neutrino multiplet

M.G. Aartsen; M. Ackermann; J. Adams; J.A. Aguilar; Markus Ahlers; M. Ahrens; I. Al Samarai; D. Altmann; K. Andeen; T. Anderson; I. Ansseau; G. Anton; M. Archinger; C. Arguelles; D. Jason Koskinen; Morten Ankersen Medici; Michael James Larson; Subir Sarkar; E. Hansen; M Rameez

doi:10.1051/0004-6361/201730620

Multiwavelength follow-up of a rare IceCube neutrino multiplet

M.G. Aartsen, M. Ackermann, J. Adams, J.A. Aguilar, Markus Ahlers, M. Ahrens, I. Al Samarai, D. Altmann, K. Andeen, T. Anderson, I. Ansseau, G. Anton, M. Archinger, C. Arguelles, D. Jason Koskinen, Morten Ankersen Medici, Michael James Larson, Subir Sarkar, E. Hansen, M Rameez

18 Citationer (Scopus)

Abstract

On February 17, 2016, the IceCube real-time neutrino search identified, for the first time, three muon neutrino candidates arriving within 100 s of one another, consistent with coming from the same point in the sky. Such a triplet is expected once every 13.7 years as a random coincidence of background events. However, considering the lifetime of the follow-up program the probability of detecting at least one triplet from atmospheric background is 32%. Follow-up observatories were notified in order to search for an electromagnetic counterpart. Observations were obtained by Swift's X-ray telescope, by ASAS-SN, LCO and MASTER at optical wavelengths, and by VERITAS in the very-high-energy gamma-ray regime. Moreover, the Swift BAT serendipitously observed the location 100 s after the first neutrino was detected, and data from the Fermi LAT and HAWC observatory were analyzed. We present details of the neutrino triplet and the follow-up observations. No likely electromagnetic counterpart was detected, and we discuss the implications of these constraints on candidate neutrino sources such as gamma-ray bursts, core-collapse supernovae and active galactic nucleus flares. This study illustrates the potential of and challenges for future follow-up campaigns.

Originalsprog	Engelsk
Artikelnummer	A115
Tidsskrift	Astronomy & Astrophysics
Vol/bind	607
ISSN	0004-6361
DOI	https://doi.org/10.1051/0004-6361/201730620
Status	Udgivet - 1 nov. 2017

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10.1051/0004-6361/201730620

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Aartsen, M. G., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Ahrens, M., Al Samarai, I., Altmann, D., Andeen, K., Anderson, T., Ansseau, I., Anton, G., Archinger, M., Arguelles, C., Koskinen, D. J., Medici, M. A., Larson, M. J., Sarkar, S., Hansen, E., & Rameez, M. (2017). Multiwavelength follow-up of a rare IceCube neutrino multiplet. Astronomy & Astrophysics, 607, [A115]. https://doi.org/10.1051/0004-6361/201730620

Aartsen, MG, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Ahrens, M, Al Samarai, I, Altmann, D, Andeen, K, Anderson, T, Ansseau, I, Anton, G, Archinger, M, Arguelles, C, Koskinen, DJ, Medici, MA, Larson, MJ, Sarkar, S, Hansen, E & Rameez, M 2017, 'Multiwavelength follow-up of a rare IceCube neutrino multiplet', Astronomy & Astrophysics, bind 607, A115. https://doi.org/10.1051/0004-6361/201730620

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title = "Multiwavelength follow-up of a rare IceCube neutrino multiplet",

abstract = "On February 17, 2016, the IceCube real-time neutrino search identified, for the first time, three muon neutrino candidates arriving within 100 s of one another, consistent with coming from the same point in the sky. Such a triplet is expected once every 13.7 years as a random coincidence of background events. However, considering the lifetime of the follow-up program the probability of detecting at least one triplet from atmospheric background is 32%. Follow-up observatories were notified in order to search for an electromagnetic counterpart. Observations were obtained by Swift's X-ray telescope, by ASAS-SN, LCO and MASTER at optical wavelengths, and by VERITAS in the very-high-energy gamma-ray regime. Moreover, the Swift BAT serendipitously observed the location 100 s after the first neutrino was detected, and data from the Fermi LAT and HAWC observatory were analyzed. We present details of the neutrino triplet and the follow-up observations. No likely electromagnetic counterpart was detected, and we discuss the implications of these constraints on candidate neutrino sources such as gamma-ray bursts, core-collapse supernovae and active galactic nucleus flares. This study illustrates the potential of and challenges for future follow-up campaigns.",

author = "M.G. Aartsen and M. Ackermann and J. Adams and J.A. Aguilar and Markus Ahlers and M. Ahrens and {Al Samarai}, I. and D. Altmann and K. Andeen and T. Anderson and I. Ansseau and G. Anton and M. Archinger and C. Arguelles and Koskinen, {D. Jason} and Medici, {Morten Ankersen} and Larson, {Michael James} and Subir Sarkar and E. Hansen and M Rameez",

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doi = "10.1051/0004-6361/201730620",

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T1 - Multiwavelength follow-up of a rare IceCube neutrino multiplet

AU - Aartsen, M.G.

AU - Ackermann, M.

AU - Adams, J.

AU - Aguilar, J.A.

AU - Ahlers, Markus

AU - Ahrens, M.

AU - Al Samarai, I.

AU - Altmann, D.

AU - Andeen, K.

AU - Anderson, T.

AU - Ansseau, I.

AU - Anton, G.

AU - Archinger, M.

AU - Arguelles, C.

AU - Koskinen, D. Jason

AU - Medici, Morten Ankersen

AU - Larson, Michael James

AU - Sarkar, Subir

AU - Hansen, E.

AU - Rameez, M

PY - 2017/11/1

Y1 - 2017/11/1

N2 - On February 17, 2016, the IceCube real-time neutrino search identified, for the first time, three muon neutrino candidates arriving within 100 s of one another, consistent with coming from the same point in the sky. Such a triplet is expected once every 13.7 years as a random coincidence of background events. However, considering the lifetime of the follow-up program the probability of detecting at least one triplet from atmospheric background is 32%. Follow-up observatories were notified in order to search for an electromagnetic counterpart. Observations were obtained by Swift's X-ray telescope, by ASAS-SN, LCO and MASTER at optical wavelengths, and by VERITAS in the very-high-energy gamma-ray regime. Moreover, the Swift BAT serendipitously observed the location 100 s after the first neutrino was detected, and data from the Fermi LAT and HAWC observatory were analyzed. We present details of the neutrino triplet and the follow-up observations. No likely electromagnetic counterpart was detected, and we discuss the implications of these constraints on candidate neutrino sources such as gamma-ray bursts, core-collapse supernovae and active galactic nucleus flares. This study illustrates the potential of and challenges for future follow-up campaigns.

AB - On February 17, 2016, the IceCube real-time neutrino search identified, for the first time, three muon neutrino candidates arriving within 100 s of one another, consistent with coming from the same point in the sky. Such a triplet is expected once every 13.7 years as a random coincidence of background events. However, considering the lifetime of the follow-up program the probability of detecting at least one triplet from atmospheric background is 32%. Follow-up observatories were notified in order to search for an electromagnetic counterpart. Observations were obtained by Swift's X-ray telescope, by ASAS-SN, LCO and MASTER at optical wavelengths, and by VERITAS in the very-high-energy gamma-ray regime. Moreover, the Swift BAT serendipitously observed the location 100 s after the first neutrino was detected, and data from the Fermi LAT and HAWC observatory were analyzed. We present details of the neutrino triplet and the follow-up observations. No likely electromagnetic counterpart was detected, and we discuss the implications of these constraints on candidate neutrino sources such as gamma-ray bursts, core-collapse supernovae and active galactic nucleus flares. This study illustrates the potential of and challenges for future follow-up campaigns.

U2 - 10.1051/0004-6361/201730620

DO - 10.1051/0004-6361/201730620

M3 - Journal article

SN - 0004-6361

VL - 607

JO - Astronomy and Astrophysics Supplement Series

JF - Astronomy and Astrophysics Supplement Series

M1 - A115

ER -

Multiwavelength follow-up of a rare IceCube neutrino multiplet

Abstract

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