Standard
Follow-up of Astrophysical Transients in Real Time with the IceCube Neutrino Observatory. / Aartsen, M. G.; Abbasi, R.; Ackermann, M.; Adams, J.; Aguilar, J. A.; Ahlers, M.; Ahrens, M.; Alispach, C.; Amin, N. M.; Andeen, K.; Anderson, T.; Ansseau, I.; Anton, G.; Arguelles, C.; Auffenberg, J.; Axani, S.; Bagherpour, H.; Bai, X.; Balagopal, A. V.; Barbano, A.; Barwick, S. W.; Bastian, B.; Basu, V.; Baum, V.; Baur, S.; Bay, R.; Beatty, J. J.; Becker, K. -H.; Tjus, J. Becker; Bellenghi, C.; BenZvi, S.; Berley, D.; Bernardini, E.; Besson, D. Z.; Binder, G.; Bindig, D.; Blaufuss, E.; Blot, S.; Bohm, C.; Boeser, S.; Botner, O.; Boettcher, J.; Bourbeau, E.; Bourbeau, J.; Bradascio, F.; Braun, J.; Koskinen, D. J.; Medici, M.; Rameez, M.; Stuttard, T.; Icecube Collaboration.
In:
Astrophysical Journal, Vol. 910, No. 1, 4, 03.2021.
Research output: Contribution to journal › Journal article › Research › peer-review
Harvard
Aartsen, MG, Abbasi, R, Ackermann, M, Adams, J, Aguilar, JA
, Ahlers, M, Ahrens, M, Alispach, C, Amin, NM, Andeen, K, Anderson, T, Ansseau, I, Anton, G, Arguelles, C, Auffenberg, J, Axani, S, Bagherpour, H, Bai, X, Balagopal, AV, Barbano, A, Barwick, SW, Bastian, B, Basu, V, Baum, V, Baur, S, Bay, R, Beatty, JJ, Becker, K-H, Tjus, JB, Bellenghi, C, BenZvi, S, Berley, D, Bernardini, E, Besson, DZ, Binder, G, Bindig, D, Blaufuss, E, Blot, S, Bohm, C, Boeser, S, Botner, O, Boettcher, J, Bourbeau, E, Bourbeau, J, Bradascio, F, Braun, J, Koskinen, DJ, Medici, M, Rameez, M
, Stuttard, T & Icecube Collaboration 2021, '
Follow-up of Astrophysical Transients in Real Time with the IceCube Neutrino Observatory',
Astrophysical Journal, vol. 910, no. 1, 4.
https://doi.org/10.3847/1538-4357/abe123APA
Aartsen, M. G., Abbasi, R., Ackermann, M., Adams, J., Aguilar, J. A.
, Ahlers, M., Ahrens, M., Alispach, C., Amin, N. M., Andeen, K., Anderson, T., Ansseau, I., Anton, G., Arguelles, C., Auffenberg, J., Axani, S., Bagherpour, H., Bai, X., Balagopal, A. V., ... Icecube Collaboration (2021).
Follow-up of Astrophysical Transients in Real Time with the IceCube Neutrino Observatory.
Astrophysical Journal,
910(1), [4].
https://doi.org/10.3847/1538-4357/abe123Vancouver
Aartsen MG, Abbasi R, Ackermann M, Adams J, Aguilar JA
, Ahlers M et al.
Follow-up of Astrophysical Transients in Real Time with the IceCube Neutrino Observatory.
Astrophysical Journal. 2021 Mar;910(1). 4.
https://doi.org/10.3847/1538-4357/abe123Author
Aartsen, M. G. ; Abbasi, R. ; Ackermann, M. ; Adams, J. ; Aguilar, J. A. ; Ahlers, M. ; Ahrens, M. ; Alispach, C. ; Amin, N. M. ; Andeen, K. ; Anderson, T. ; Ansseau, I. ; Anton, G. ; Arguelles, C. ; Auffenberg, J. ; Axani, S. ; Bagherpour, H. ; Bai, X. ; Balagopal, A. V. ; Barbano, A. ; Barwick, S. W. ; Bastian, B. ; Basu, V. ; Baum, V. ; Baur, S. ; Bay, R. ; Beatty, J. J. ; Becker, K. -H. ; Tjus, J. Becker ; Bellenghi, C. ; BenZvi, S. ; Berley, D. ; Bernardini, E. ; Besson, D. Z. ; Binder, G. ; Bindig, D. ; Blaufuss, E. ; Blot, S. ; Bohm, C. ; Boeser, S. ; Botner, O. ; Boettcher, J. ; Bourbeau, E. ; Bourbeau, J. ; Bradascio, F. ; Braun, J. ; Koskinen, D. J. ; Medici, M. ; Rameez, M. ; Stuttard, T. ; Icecube Collaboration. / Follow-up of Astrophysical Transients in Real Time with the IceCube Neutrino Observatory. In: Astrophysical Journal. 2021 ; Vol. 910, No. 1.
Bibtex
@article{25d322ac147445f29533a8b7360293f3,
title = "Follow-up of Astrophysical Transients in Real Time with the IceCube Neutrino Observatory",
abstract = "In multi-messenger astronomy, rapid investigation of interesting transients is imperative. As an observatory with a 4 pi steradian field of view, and similar to 99% uptime, the IceCube Neutrino Observatory is a unique facility to follow up transients, as well as to provide valuable insights for other observatories and inform their observational decisions. Since 2016, IceCube has been using low-latency data to rapidly respond to interesting astrophysical events reported by the multi-messenger observational community. Here, we describe the pipeline used to perform these followup analyses, and provide a summary of the 58 analyses performed as of July 2020. We find no significant signal in the first 58 analyses performed. The pipeline has helped inform various electromagnetic observation strategies, and has constrained neutrino emission from potential hadronic cosmic accelerators.",
keywords = "Neutrino astronomy, High energy astrophysics",
author = "Aartsen, {M. G.} and R. Abbasi and M. Ackermann and J. Adams and Aguilar, {J. A.} and M. Ahlers and M. Ahrens and C. Alispach and Amin, {N. M.} and K. Andeen and T. Anderson and I. Ansseau and G. Anton and C. Arguelles and J. Auffenberg and S. Axani and H. Bagherpour and X. Bai and Balagopal, {A. V.} and A. Barbano and Barwick, {S. W.} and B. Bastian and V. Basu and V. Baum and S. Baur and R. Bay and Beatty, {J. J.} and Becker, {K. -H.} and Tjus, {J. Becker} and C. Bellenghi and S. BenZvi and D. Berley and E. Bernardini and Besson, {D. Z.} and G. Binder and D. Bindig and E. Blaufuss and S. Blot and C. Bohm and S. Boeser and O. Botner and J. Boettcher and E. Bourbeau and J. Bourbeau and F. Bradascio and J. Braun and Koskinen, {D. J.} and M. Medici and M. Rameez and T. Stuttard and {Icecube Collaboration}",
year = "2021",
month = mar,
doi = "10.3847/1538-4357/abe123",
language = "English",
volume = "910",
journal = "Astrophysical Journal",
issn = "0004-637X",
publisher = "Institute of Physics Publishing, Inc",
number = "1",
}
RIS
TY - JOUR
T1 - Follow-up of Astrophysical Transients in Real Time with the IceCube Neutrino Observatory
AU - Aartsen, M. G.
AU - Abbasi, R.
AU - Ackermann, M.
AU - Adams, J.
AU - Aguilar, J. A.
AU - Ahlers, M.
AU - Ahrens, M.
AU - Alispach, C.
AU - Amin, N. M.
AU - Andeen, K.
AU - Anderson, T.
AU - Ansseau, I.
AU - Anton, G.
AU - Arguelles, C.
AU - Auffenberg, J.
AU - Axani, S.
AU - Bagherpour, H.
AU - Bai, X.
AU - Balagopal, A. V.
AU - Barbano, A.
AU - Barwick, S. W.
AU - Bastian, B.
AU - Basu, V.
AU - Baum, V.
AU - Baur, S.
AU - Bay, R.
AU - Beatty, J. J.
AU - Becker, K. -H.
AU - Tjus, J. Becker
AU - Bellenghi, C.
AU - BenZvi, S.
AU - Berley, D.
AU - Bernardini, E.
AU - Besson, D. Z.
AU - Binder, G.
AU - Bindig, D.
AU - Blaufuss, E.
AU - Blot, S.
AU - Bohm, C.
AU - Boeser, S.
AU - Botner, O.
AU - Boettcher, J.
AU - Bourbeau, E.
AU - Bourbeau, J.
AU - Bradascio, F.
AU - Braun, J.
AU - Koskinen, D. J.
AU - Medici, M.
AU - Rameez, M.
AU - Stuttard, T.
AU - Icecube Collaboration
PY - 2021/3
Y1 - 2021/3
N2 - In multi-messenger astronomy, rapid investigation of interesting transients is imperative. As an observatory with a 4 pi steradian field of view, and similar to 99% uptime, the IceCube Neutrino Observatory is a unique facility to follow up transients, as well as to provide valuable insights for other observatories and inform their observational decisions. Since 2016, IceCube has been using low-latency data to rapidly respond to interesting astrophysical events reported by the multi-messenger observational community. Here, we describe the pipeline used to perform these followup analyses, and provide a summary of the 58 analyses performed as of July 2020. We find no significant signal in the first 58 analyses performed. The pipeline has helped inform various electromagnetic observation strategies, and has constrained neutrino emission from potential hadronic cosmic accelerators.
AB - In multi-messenger astronomy, rapid investigation of interesting transients is imperative. As an observatory with a 4 pi steradian field of view, and similar to 99% uptime, the IceCube Neutrino Observatory is a unique facility to follow up transients, as well as to provide valuable insights for other observatories and inform their observational decisions. Since 2016, IceCube has been using low-latency data to rapidly respond to interesting astrophysical events reported by the multi-messenger observational community. Here, we describe the pipeline used to perform these followup analyses, and provide a summary of the 58 analyses performed as of July 2020. We find no significant signal in the first 58 analyses performed. The pipeline has helped inform various electromagnetic observation strategies, and has constrained neutrino emission from potential hadronic cosmic accelerators.
KW - Neutrino astronomy
KW - High energy astrophysics
U2 - 10.3847/1538-4357/abe123
DO - 10.3847/1538-4357/abe123
M3 - Journal article
VL - 910
JO - Astrophysical Journal
JF - Astrophysical Journal
SN - 0004-637X
IS - 1
M1 - 4
ER -
