SNEWS 2.0: A next-generation supernova early warning system for multi-messenger astronomy

S. Al Kharusi; S. Y. BenZvi; J. S. Bobowski; W. Bonivento; V. Brdar; T. Brunner; E. Caden; M. Clark; A. Coleiro; M. Colomer-Molla; J. I. Crespo-Anadón; A. Depoian; D. Dornic; V. Fischer; D. Franco; W. Fulgione; A. Gallo Rosso; M. Geske; S. Griswold; M. Gromov; D. Haggard; A. Habig; O. Halim; A. Higuera; R. Hill; S. Horiuchi; K. Ishidoshiro; C. Kato; E. Katsavounidis; D. Khaitan; J. P. Kneller; A. Kopec; V. Kulikovskiy; M. Lai; M. Lamoureux; R. F. Lang; H. L. Li; M. Lincetto; C. Lunardini; J. Migenda; D. Milisavljevic; M. E. McCarthy; E. O. Connor; E. O. Sullivan; G. Pagliaroli; D. Patel; R. Peres; B. W. Pointon; J. Qin; N. Raj; A. Renshaw; A. Roeth; J. Rumleskie; K. Scholberg; A. Sheshukov; T. Sonley; M. Strait; V. Takhistov; I. Tamborra; J. Tseng; C. D. Tunnell; J. Vasel; C. F. Vigorito; B. Viren; C. J. Virtue; J. S. Wang; L. J. Wen; L. Winslow; F. L.H. Wolfs; X. J. Xu; Y. Xu

doi:10.1088/1367-2630/abde33

SNEWS 2.0: A next-generation supernova early warning system for multi-messenger astronomy

S. Al Kharusi, S. Y. BenZvi, J. S. Bobowski, W. Bonivento, V. Brdar, T. Brunner, E. Caden, M. Clark, A. Coleiro, M. Colomer-Molla, J. I. Crespo-Anadón, A. Depoian, D. Dornic, V. Fischer, D. Franco, W. Fulgione, A. Gallo Rosso, M. Geske, S. Griswold, M. GromovD. Haggard, A. Habig, O. Halim, A. Higuera, R. Hill, S. Horiuchi, K. Ishidoshiro, C. Kato, E. Katsavounidis, D. Khaitan, J. P. Kneller, A. Kopec, V. Kulikovskiy, M. Lai, M. Lamoureux, R. F. Lang, H. L. Li, M. Lincetto, C. Lunardini, J. Migenda, D. Milisavljevic, M. E. McCarthy, E. O. Connor, E. O. Sullivan, G. Pagliaroli, D. Patel, R. Peres, B. W. Pointon, J. Qin, N. Raj, A. Renshaw, A. Roeth, J. Rumleskie, K. Scholberg, A. Sheshukov, T. Sonley, M. Strait, V. Takhistov, I. Tamborra, J. Tseng, C. D. Tunnell, J. Vasel, C. F. Vigorito, B. Viren, C. J. Virtue, J. S. Wang, L. J. Wen, L. Winslow, F. L.H. Wolfs, X. J. Xu, Y. Xu

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Abstract

The next core-collapse supernova in the Milky Way or its satellites will represent a once-in-a-generation opportunity to obtain detailed information about the explosion of a star and provide significant scientific insight for a variety of fields because of the extreme conditions found within. Supernovae in our galaxy are not only rare on a human timescale but also happen at unscheduled times, so it is crucial to be ready and use all available instruments to capture all possible information from the event. The first indication of a potential stellar explosion will be the arrival of a bright burst of neutrinos. Its observation by multiple detectors worldwide can provide an early warning for the subsequent electromagnetic fireworks, as well as signal to other detectors with significant backgrounds so they can store their recent data. The supernova early warning system (SNEWS) has been operating as a simple coincidence between neutrino experiments in automated mode since 2005. In the current era of multi-messenger astronomy there are new opportunities for SNEWS to optimize sensitivity to science from the next galactic supernova beyond the simple early alert. This document is the product of a workshop in June 2019 towards design of SNEWS 2.0, an upgraded SNEWS with enhanced capabilities exploiting the unique advantages of prompt neutrino detection to maximize the science gained from such a valuable event.

Original language	English (US)
Article number	031201
Journal	New Journal of Physics
Volume	23
Issue number	3
DOIs	https://doi.org/10.1088/1367-2630/abde33
State	Published - Mar 2021

Bibliographical note

Publisher Copyright:
© 2021 The Author(s). Published by IOP Publishing Ltd on behalf of the Institute of Physics and Deutsche Physikalische Gesellschaft

Keywords

Multi-messenger astronomy
Particle astrophysics
Supernova neutrinos

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10.1088/1367-2630/abde33

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Al Kharusi, S., BenZvi, S. Y., Bobowski, J. S., Bonivento, W., Brdar, V., Brunner, T., Caden, E., Clark, M., Coleiro, A., Colomer-Molla, M., Crespo-Anadón, J. I., Depoian, A., Dornic, D., Fischer, V., Franco, D., Fulgione, W., Gallo Rosso, A., Geske, M., Griswold, S., ... Xu, Y. (2021). SNEWS 2.0: A next-generation supernova early warning system for multi-messenger astronomy. New Journal of Physics, 23(3), Article 031201. https://doi.org/10.1088/1367-2630/abde33

Al Kharusi, S, BenZvi, SY, Bobowski, JS, Bonivento, W, Brdar, V, Brunner, T, Caden, E, Clark, M, Coleiro, A, Colomer-Molla, M, Crespo-Anadón, JI, Depoian, A, Dornic, D, Fischer, V, Franco, D, Fulgione, W, Gallo Rosso, A, Geske, M, Griswold, S, Gromov, M, Haggard, D, Habig, A, Halim, O, Higuera, A, Hill, R, Horiuchi, S, Ishidoshiro, K, Kato, C, Katsavounidis, E, Khaitan, D, Kneller, JP, Kopec, A, Kulikovskiy, V, Lai, M, Lamoureux, M, Lang, RF, Li, HL, Lincetto, M, Lunardini, C, Migenda, J, Milisavljevic, D, McCarthy, ME, Connor, EO, Sullivan, EO, Pagliaroli, G, Patel, D, Peres, R, Pointon, BW, Qin, J, Raj, N, Renshaw, A, Roeth, A, Rumleskie, J, Scholberg, K, Sheshukov, A, Sonley, T, Strait, M, Takhistov, V, Tamborra, I, Tseng, J, Tunnell, CD, Vasel, J, Vigorito, CF, Viren, B, Virtue, CJ, Wang, JS, Wen, LJ, Winslow, L, Wolfs, FLH, Xu, XJ & Xu, Y 2021, 'SNEWS 2.0: A next-generation supernova early warning system for multi-messenger astronomy', New Journal of Physics, vol. 23, no. 3, 031201. https://doi.org/10.1088/1367-2630/abde33

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abstract = "The next core-collapse supernova in the Milky Way or its satellites will represent a once-in-a-generation opportunity to obtain detailed information about the explosion of a star and provide significant scientific insight for a variety of fields because of the extreme conditions found within. Supernovae in our galaxy are not only rare on a human timescale but also happen at unscheduled times, so it is crucial to be ready and use all available instruments to capture all possible information from the event. The first indication of a potential stellar explosion will be the arrival of a bright burst of neutrinos. Its observation by multiple detectors worldwide can provide an early warning for the subsequent electromagnetic fireworks, as well as signal to other detectors with significant backgrounds so they can store their recent data. The supernova early warning system (SNEWS) has been operating as a simple coincidence between neutrino experiments in automated mode since 2005. In the current era of multi-messenger astronomy there are new opportunities for SNEWS to optimize sensitivity to science from the next galactic supernova beyond the simple early alert. This document is the product of a workshop in June 2019 towards design of SNEWS 2.0, an upgraded SNEWS with enhanced capabilities exploiting the unique advantages of prompt neutrino detection to maximize the science gained from such a valuable event.",

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author = "{Al Kharusi}, S. and BenZvi, {S. Y.} and Bobowski, {J. S.} and W. Bonivento and V. Brdar and T. Brunner and E. Caden and M. Clark and A. Coleiro and M. Colomer-Molla and Crespo-Anad{\'o}n, {J. I.} and A. Depoian and D. Dornic and V. Fischer and D. Franco and W. Fulgione and {Gallo Rosso}, A. and M. Geske and S. Griswold and M. Gromov and D. Haggard and A. Habig and O. Halim and A. Higuera and R. Hill and S. Horiuchi and K. Ishidoshiro and C. Kato and E. Katsavounidis and D. Khaitan and Kneller, {J. P.} and A. Kopec and V. Kulikovskiy and M. Lai and M. Lamoureux and Lang, {R. F.} and Li, {H. L.} and M. Lincetto and C. Lunardini and J. Migenda and D. Milisavljevic and McCarthy, {M. E.} and Connor, {E. O.} and Sullivan, {E. O.} and G. Pagliaroli and D. Patel and R. Peres and Pointon, {B. W.} and J. Qin and N. Raj and A. Renshaw and A. Roeth and J. Rumleskie and K. Scholberg and A. Sheshukov and T. Sonley and M. Strait and V. Takhistov and I. Tamborra and J. Tseng and Tunnell, {C. D.} and J. Vasel and Vigorito, {C. F.} and B. Viren and Virtue, {C. J.} and Wang, {J. S.} and Wen, {L. J.} and L. Winslow and Wolfs, {F. L.H.} and Xu, {X. J.} and Y. Xu",

note = "Publisher Copyright: {\textcopyright} 2021 The Author(s). Published by IOP Publishing Ltd on behalf of the Institute of Physics and Deutsche Physikalische Gesellschaft",

year = "2021",

month = mar,

doi = "10.1088/1367-2630/abde33",

language = "English (US)",

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T2 - A next-generation supernova early warning system for multi-messenger astronomy

AU - Al Kharusi, S.

AU - BenZvi, S. Y.

AU - Bobowski, J. S.

AU - Bonivento, W.

AU - Brdar, V.

AU - Brunner, T.

AU - Caden, E.

AU - Clark, M.

AU - Coleiro, A.

AU - Colomer-Molla, M.

AU - Crespo-Anadón, J. I.

AU - Depoian, A.

AU - Dornic, D.

AU - Fischer, V.

AU - Franco, D.

AU - Fulgione, W.

AU - Gallo Rosso, A.

AU - Geske, M.

AU - Griswold, S.

AU - Gromov, M.

AU - Haggard, D.

AU - Habig, A.

AU - Halim, O.

AU - Higuera, A.

AU - Hill, R.

AU - Horiuchi, S.

AU - Ishidoshiro, K.

AU - Kato, C.

AU - Katsavounidis, E.

AU - Khaitan, D.

AU - Kneller, J. P.

AU - Kopec, A.

AU - Kulikovskiy, V.

AU - Lai, M.

AU - Lamoureux, M.

AU - Lang, R. F.

AU - Li, H. L.

AU - Lincetto, M.

AU - Lunardini, C.

AU - Migenda, J.

AU - Milisavljevic, D.

AU - McCarthy, M. E.

AU - Connor, E. O.

AU - Sullivan, E. O.

AU - Pagliaroli, G.

AU - Patel, D.

AU - Peres, R.

AU - Pointon, B. W.

AU - Qin, J.

AU - Raj, N.

AU - Renshaw, A.

AU - Roeth, A.

AU - Rumleskie, J.

AU - Scholberg, K.

AU - Sheshukov, A.

AU - Sonley, T.

AU - Strait, M.

AU - Takhistov, V.

AU - Tamborra, I.

AU - Tseng, J.

AU - Tunnell, C. D.

AU - Vasel, J.

AU - Vigorito, C. F.

AU - Viren, B.

AU - Virtue, C. J.

AU - Wang, J. S.

AU - Wen, L. J.

AU - Winslow, L.

AU - Wolfs, F. L.H.

AU - Xu, X. J.

AU - Xu, Y.

PY - 2021/3

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N2 - The next core-collapse supernova in the Milky Way or its satellites will represent a once-in-a-generation opportunity to obtain detailed information about the explosion of a star and provide significant scientific insight for a variety of fields because of the extreme conditions found within. Supernovae in our galaxy are not only rare on a human timescale but also happen at unscheduled times, so it is crucial to be ready and use all available instruments to capture all possible information from the event. The first indication of a potential stellar explosion will be the arrival of a bright burst of neutrinos. Its observation by multiple detectors worldwide can provide an early warning for the subsequent electromagnetic fireworks, as well as signal to other detectors with significant backgrounds so they can store their recent data. The supernova early warning system (SNEWS) has been operating as a simple coincidence between neutrino experiments in automated mode since 2005. In the current era of multi-messenger astronomy there are new opportunities for SNEWS to optimize sensitivity to science from the next galactic supernova beyond the simple early alert. This document is the product of a workshop in June 2019 towards design of SNEWS 2.0, an upgraded SNEWS with enhanced capabilities exploiting the unique advantages of prompt neutrino detection to maximize the science gained from such a valuable event.

AB - The next core-collapse supernova in the Milky Way or its satellites will represent a once-in-a-generation opportunity to obtain detailed information about the explosion of a star and provide significant scientific insight for a variety of fields because of the extreme conditions found within. Supernovae in our galaxy are not only rare on a human timescale but also happen at unscheduled times, so it is crucial to be ready and use all available instruments to capture all possible information from the event. The first indication of a potential stellar explosion will be the arrival of a bright burst of neutrinos. Its observation by multiple detectors worldwide can provide an early warning for the subsequent electromagnetic fireworks, as well as signal to other detectors with significant backgrounds so they can store their recent data. The supernova early warning system (SNEWS) has been operating as a simple coincidence between neutrino experiments in automated mode since 2005. In the current era of multi-messenger astronomy there are new opportunities for SNEWS to optimize sensitivity to science from the next galactic supernova beyond the simple early alert. This document is the product of a workshop in June 2019 towards design of SNEWS 2.0, an upgraded SNEWS with enhanced capabilities exploiting the unique advantages of prompt neutrino detection to maximize the science gained from such a valuable event.

KW - Multi-messenger astronomy

KW - Particle astrophysics

KW - Supernova neutrinos

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DO - 10.1088/1367-2630/abde33

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SN - 1367-2630

VL - 23

JO - New Journal of Physics

JF - New Journal of Physics

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M1 - 031201

ER -

SNEWS 2.0: A next-generation supernova early warning system for multi-messenger astronomy

Abstract

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