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

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SNEWS 2.0 : a next-generation supernova early warning system for multi-messenger astronomy. / Al Kharusi, S.; BenZvi, S. Y.; Bobowski, J. S.; Bonivento, W.; Brdar; Brunner, T.; Caden, E.; Clark, M.; Coleiro, A.; Colomer-Molla, M.; Crespo-Anadon, J.; Depoian, A.; Dornic, D.; Fischer, Paul; 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, J. P.; Kopec, A.; Kulikovskiy; Lai, M.; Lamoureux, M.; Lang, R. F.; Li, H. L.; Lincetto, M.; Lunardini, C.; Migenda, J.; Milisavljevic, D.; McCarthy, M. E.; Connor, E.; Sullivan, E.; Pagliaroli, G.; Patel, D.; Peres, R.; Pointon, B. W.; Qin, J.; Raj, N.; Renshaw, A.; Roeth, A.; Rumleskie, J.; Scholberg, K.; Sheshukov, A.; Sonley, T.; Strait, M.; Takhistov, ; Tamborra; Tseng, J.; Tunnell, C. D.; Vasel, J.; Vigorito, C. F.; Viren, B.; Virtue, C. J.; Wang, J. S.; Wen, L. J.; Winslow, L.; Wolfs, F. L. H.; Xu, X. J.; Xu, Y.

In: New Journal of Physics, Vol. 23, No. 3, 031201, 15.03.2021.

Research output: Contribution to journal › Review › Research › peer-review

Harvard

Al Kharusi, S, BenZvi, SY, Bobowski, JS, Bonivento, W, Brdar, Brunner, T, Caden, E, Clark, M, Coleiro, A, Colomer-Molla, M, Crespo-Anadon, J, Depoian, A, Dornic, D, Fischer, P, 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, Lai, M, Lamoureux, M, Lang, RF, Li, HL, Lincetto, M, Lunardini, C, Migenda, J, Milisavljevic, D, McCarthy, ME, Connor, E, Sullivan, E, 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, , Tamborra, 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

APA

Al Kharusi, S., BenZvi, S. Y., Bobowski, J. S., Bonivento, W., Brdar, Brunner, T., Caden, E., Clark, M., Coleiro, A., Colomer-Molla, M., Crespo-Anadon, J., Depoian, A., Dornic, D., Fischer, P., 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), [031201]. https://doi.org/10.1088/1367-2630/abde33

Vancouver

Al Kharusi S, BenZvi SY, Bobowski JS, Bonivento W, Brdar, Brunner T et al. SNEWS 2.0: a next-generation supernova early warning system for multi-messenger astronomy. New Journal of Physics. 2021 Mar 15;23(3). 031201. https://doi.org/10.1088/1367-2630/abde33

Author

Al Kharusi, S. ; BenZvi, S. Y. ; Bobowski, J. S. ; Bonivento, W. ; Brdar ; Brunner, T. ; Caden, E. ; Clark, M. ; Coleiro, A. ; Colomer-Molla, M. ; Crespo-Anadon, J. ; Depoian, A. ; Dornic, D. ; Fischer, Paul ; 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, J. P. ; Kopec, A. ; Kulikovskiy ; Lai, M. ; Lamoureux, M. ; Lang, R. F. ; Li, H. L. ; Lincetto, M. ; Lunardini, C. ; Migenda, J. ; Milisavljevic, D. ; McCarthy, M. E. ; Connor, E. ; Sullivan, E. ; Pagliaroli, G. ; Patel, D. ; Peres, R. ; Pointon, B. W. ; Qin, J. ; Raj, N. ; Renshaw, A. ; Roeth, A. ; Rumleskie, J. ; Scholberg, K. ; Sheshukov, A. ; Sonley, T. ; Strait, M. ; Takhistov, ; Tamborra ; Tseng, J. ; Tunnell, C. D. ; Vasel, J. ; Vigorito, C. F. ; Viren, B. ; Virtue, C. J. ; Wang, J. S. ; Wen, L. J. ; Winslow, L. ; Wolfs, F. L. H. ; Xu, X. J. ; Xu, Y. / SNEWS 2.0 : a next-generation supernova early warning system for multi-messenger astronomy. In: New Journal of Physics. 2021 ; Vol. 23, No. 3.

Bibtex

@article{66e0080451264eb3ac5dcce0595d7ea7,
title = "SNEWS 2.0: a next-generation supernova early warning system for multi-messenger astronomy",
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.",
keywords = "supernova neutrinos, multi-messenger astronomy, particle astrophysics",
author = "{Al Kharusi}, S. and BenZvi, {S. Y.} and Bobowski, {J. S.} and W. Bonivento and Brdar and T. Brunner and E. Caden and M. Clark and A. Coleiro and M. Colomer-Molla and J. Crespo-Anadon and A. Depoian and D. Dornic and Paul 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 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 E. Connor and E. Sullivan 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 Takhistov and 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",
year = "2021",
month = mar,
day = "15",
doi = "10.1088/1367-2630/abde33",
language = "English",
volume = "23",
journal = "New Journal of Physics",
issn = "1367-2630",
publisher = "IOP Publishing",
number = "3",

}

RIS

TY - JOUR

T1 - SNEWS 2.0

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, null

AU - Brunner, T.

AU - Caden, E.

AU - Clark, M.

AU - Coleiro, A.

AU - Colomer-Molla, M.

AU - Crespo-Anadon, J.

AU - Depoian, A.

AU - Dornic, D.

AU - Fischer, Paul

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, null

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.

AU - Sullivan, E.

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, null

AU - Tamborra, null

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 - 2021/3/15

Y1 - 2021/3/15

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 - supernova neutrinos

KW - multi-messenger astronomy

KW - particle astrophysics

U2 - 10.1088/1367-2630/abde33

DO - 10.1088/1367-2630/abde33

M3 - Review

VL - 23

JO - New Journal of Physics

JF - New Journal of Physics

SN - 1367-2630

IS - 3

M1 - 031201

ER -

ID: 259826313