Very High-Energy Gamma-Ray Follow-Up Program Using  Neutrino Triggers from IceCube

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

doi:10.1088/1748-0221/11/11/P11009

Very High-Energy Gamma-Ray Follow-Up Program Using Neutrino Triggers from IceCube

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

20 Citationer (Scopus)

Abstract

We describe and report the status of a neutrino-triggered program in IceCube that generates real-time alerts for gamma-ray follow-up observations by atmospheric-Cherenkov telescopes (MAGIC and VERITAS). While IceCube is capable of monitoring the whole sky continuously, high-energy gamma-ray telescopes have restricted fields of view and in general are unlikely to be observing a potential neutrino-flaring source at the time such neutrinos are recorded. The use of neutrino-triggered alerts thus aims at increasing the availability of simultaneous multi-messenger data during potential neutrino flaring activity, which can increase the discovery potential and constrain the phenomenological interpretation of the high-energy emission of selected source classes (e.g. blazars). The requirements of a fast and stable online analysis of potential neutrino signals and its operation are presented, along with first results of the program operating between 14 March 2012 and 31 December 2015.

Originalsprog	Engelsk
Artikelnummer	P11009
Tidsskrift	Journal of Instrumentation
Vol/bind	11
ISSN	1748-0221
DOI	https://doi.org/10.1088/1748-0221/11/11/P11009
Status	Udgivet - 21 nov. 2016

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10.1088/1748-0221/11/11/P11009

_2016_J._Inst._11_P11009Forlagets udgivne version, 1,66 MB

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Aartsen, M. G., Abraham, K., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M. T., Ahrens, M., Altmann, D., Andeen, K., Anderson, T., Ansseau, I., Anton, G., Auffenberg, J., Arguelles, C., Archinger, M., Medici, M. A., Koskinen, D. J., Larson, M. J., Rameez, M., & Sarkar, S. (2016). Very High-Energy Gamma-Ray Follow-Up Program Using Neutrino Triggers from IceCube. Journal of Instrumentation, 11, Artikel P11009. https://doi.org/10.1088/1748-0221/11/11/P11009

Aartsen, MG, Abraham, K, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, MT, Ahrens, M, Altmann, D, Andeen, K, Anderson, T, Ansseau, I, Anton, G, Auffenberg, J, Arguelles, C, Archinger, M, Medici, MA, Koskinen, DJ, Larson, MJ, Rameez, M & Sarkar, S 2016, 'Very High-Energy Gamma-Ray Follow-Up Program Using Neutrino Triggers from IceCube', Journal of Instrumentation, bind 11, P11009. https://doi.org/10.1088/1748-0221/11/11/P11009

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title = "Very High-Energy Gamma-Ray Follow-Up Program Using Neutrino Triggers from IceCube",

abstract = "We describe and report the status of a neutrino-triggered program in IceCube that generates real-time alerts for gamma-ray follow-up observations by atmospheric-Cherenkov telescopes (MAGIC and VERITAS). While IceCube is capable of monitoring the whole sky continuously, high-energy gamma-ray telescopes have restricted fields of view and in general are unlikely to be observing a potential neutrino-flaring source at the time such neutrinos are recorded. The use of neutrino-triggered alerts thus aims at increasing the availability of simultaneous multi-messenger data during potential neutrino flaring activity, which can increase the discovery potential and constrain the phenomenological interpretation of the high-energy emission of selected source classes (e.g. blazars). The requirements of a fast and stable online analysis of potential neutrino signals and its operation are presented, along with first results of the program operating between 14 March 2012 and 31 December 2015.",

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

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AU - Aartsen, M.G.

AU - Abraham, K.

AU - Ackermann, M.

AU - Adams, Joe

AU - Aguilar, J.A.

AU - Ahlers, Markus Tobias

AU - Ahrens, M.

AU - Altmann, D.

AU - Andeen, K.

AU - Anderson, T.

AU - Ansseau, I.

AU - Anton, G.

AU - Auffenberg, J.

AU - Arguelles, C.

AU - Archinger, M.

AU - Medici, Morten Ankersen

AU - Koskinen, David Jason

AU - Larson, Michael James

AU - Rameez, M

AU - Sarkar, Subir

PY - 2016/11/21

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N2 - We describe and report the status of a neutrino-triggered program in IceCube that generates real-time alerts for gamma-ray follow-up observations by atmospheric-Cherenkov telescopes (MAGIC and VERITAS). While IceCube is capable of monitoring the whole sky continuously, high-energy gamma-ray telescopes have restricted fields of view and in general are unlikely to be observing a potential neutrino-flaring source at the time such neutrinos are recorded. The use of neutrino-triggered alerts thus aims at increasing the availability of simultaneous multi-messenger data during potential neutrino flaring activity, which can increase the discovery potential and constrain the phenomenological interpretation of the high-energy emission of selected source classes (e.g. blazars). The requirements of a fast and stable online analysis of potential neutrino signals and its operation are presented, along with first results of the program operating between 14 March 2012 and 31 December 2015.

AB - We describe and report the status of a neutrino-triggered program in IceCube that generates real-time alerts for gamma-ray follow-up observations by atmospheric-Cherenkov telescopes (MAGIC and VERITAS). While IceCube is capable of monitoring the whole sky continuously, high-energy gamma-ray telescopes have restricted fields of view and in general are unlikely to be observing a potential neutrino-flaring source at the time such neutrinos are recorded. The use of neutrino-triggered alerts thus aims at increasing the availability of simultaneous multi-messenger data during potential neutrino flaring activity, which can increase the discovery potential and constrain the phenomenological interpretation of the high-energy emission of selected source classes (e.g. blazars). The requirements of a fast and stable online analysis of potential neutrino signals and its operation are presented, along with first results of the program operating between 14 March 2012 and 31 December 2015.

U2 - 10.1088/1748-0221/11/11/P11009

DO - 10.1088/1748-0221/11/11/P11009

M3 - Journal article

SN - 1748-0221

VL - 11

JO - Journal of Instrumentation

JF - Journal of Instrumentation

M1 - P11009

ER -

Very High-Energy Gamma-Ray Follow-Up Program Using Neutrino Triggers from IceCube

Abstract

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