Constraints on high-energy neutrino emission from SN 2008D

R. Abbasi, Y. Abdou, T. Abu-Zayyad, J. Adams, J. A. Aguilar, M. Ahlers, K. Andeen, J. Auffenberg, X. Bai, M. Baker, S. W. Barwick, R. Bay, J. L.Bazo Alba, K. Beattie, J. J. Beatty, S. Bechet, J. K. Becker, K. H. Becker, Mohamed Lotfi Benabderrhmane, S. BenZvi & 241 others J. Berdermann, P. Berghaus, D. Berley, E. Bernardini, D. Bertrand, D. Z. Besson, M. Bissok, E. Blaufuss, J. Blumenthal, D. J. Boersma, C. Bohm, D. Bose, S. Boser, O. Botner, J. Braun, S. Buitink, M. Carson, D. Chirkin, B. Christy, J. Clem, F. Clevermann, S. Cohen, C. Colnard, D. F. Cowen, M. V. D'Gostino, M. Danninger, J. C. Davis, C. De Clercq, L. Demirors, O. Depaepe, F. Descamps, P. Desiati, G. De Vries-Uiterweerd, T. DeYoung, J. C. Diaz-Velez, M. Dierckxsens, J. Dreyer, J. P. Dumm, M. R. Duvoort, R. Ehrlich, J. Eisch, R. W. Ellsworth, O. Engdegard, S. Euler, P. A. Evenson, O. Fadiran, A. R. Fazely, A. Fedynitch, T. Feusels, K. Filimonov, C. Finley, M. M. Foerster, B. D. Fox, A. Franckowiak, R. Franke, T. K. Gaisser, J. Gallagher, M. Geisler, L. Gerhardt, L. Gladstone, T. Glusenkamp, A. Goldschmidt, J. A. Goodman, D. Grant, T. Griesel, A. Gro, S. Grullon, M. Gurtner, C. Ha, A. Hallgren, F. Halzen, K. Han, K. Hanson, K. Helbing, P. Herquet, S. Hickford, G. C. Hill, K. D. Hoffman, A. Homeier, K. Hoshina, D. Hubert, W. Huelsnitz, J. P. Hul, P. O. Hulth, K. Hultqvist, S. Hussain, A. Ishihara, J. Jacobsen, G. S. Japaridze, H. Johansson, J. M. Joseph, K. H. Kampert, A. Kappes, T. Karg, A. Karle, J. L. Kelley, N. Kemming, P. Kenny, J. Kiryluk, F. Kislat, S. R. Klein, J. H. Kohne, G. Kohnen, H. Kolanoski, L. Kopke, D. J. Koskinen, M. Kowalski, T. Kowarik, M. Krasberg, T. Krings, G. Kroll, K. Kuehn, T. Kuwabara, M. Labare, S. Lafebre, K. Laihem, H. Landsman, M. J. Larson, R. Lauer, R. Lehmann, J. Lunemann, J. Madsen, P. Majumdar, A. Marotta, R. Maruyama, K. Mase, H. S. Matis, M. Matusik, K. Meagher, M. Merck, P. Meszaros, T. Meures, E. Middell, N. Milke, J. Miller, T. Montaruli, R. Morse, S. M. Movit, R. Nahnhauer, J. W. Nam, U. Naumann, P. Nießen, D. R. Nygren, S. Odrowski, A. Olivas, M. Olivo, A. O'Murchadha, M. Ono, S. Panknin, L. Paul, C. Perez De Los Heros, J. Petrovic, A. Piegsa, D. Pieloth, R. Porrata, J. Posselt, P. B. Price, M. Prikockis, G. T. Przybylski, K. Rawlins, P. Redl, E. Resconi, W. Rhode, M. Ribordy, A. Rizzo, J. P. Rodrigues, P. Roth, F. Rothmaier, C. Rott, T. Ruhe, D. Rutledge, B. Ruzybayev, D. Ryckbosch, H. G. Sander, M. Santander, S. Sarkar, K. Schatto, S. Schlenstedt, T. Schmidt, A. Schukraft, A. Schultes, O. Schulz, M. Schunck, D. Seckel, B. Semburg, S. H. Seo, Y. Sestayo, S. Seunarine, A. Silvestri, K. Singh, A. Slipak, G. M. Spiczak, C. Spiering, M. Stamatikos, T. Stanev, G. Stephens, T. Stezelberger, R. G. Stokstad, S. Stoyanov, E. A. Strahler, T. Straszheim, G. W. Sullivan, Q. Swillens, H. Taavola, I. Taboada, A. Tamburro, O. Tarasova, A. Tepe, S. Ter-Antonyan, S. Tilav, P. A. Toale, S. Toscano, D. Tosi, D. Turčan, N. Van Eijndhoven, J. Vandenbroucke, A. Van Overloop, J. Van Santen, M. Voge, B. Voigt, C. Walck, T. Waldenmaier, M. Wallraff, M. Walter, C. H. Weaver, C. Wendt, S. Westerhoff, N. Whitehorn, K. Wiebe, C. H. Wiebusch, G. Wikstrom, D. R. Williams, R. Wischnewski, H. Wissing, M. Wolf, K. Woschnagg, C. Xu, X. W. Xu, G. Yodh, S. Yoshida, P. Zarzhitsky

Research output: Contribution to journalArticle

Abstract

SN 2008D, a core collapse supernova at a distance of 27 Mpc, was serendipitously discovered by the Swift satellite through an associated X-ray flash. Core collapse supernovae have been observed in association with long gamma-ray bursts and X-ray flashes and a physical connection is widely assumed. This connection could imply that some core collapse supernovae possess mildly relativistic jets in which high-energy neutrinos are produced through proton-proton collisions. The predicted neutrino spectra would be detectable by Cherenkov neutrino detectors like IceCube. A search for a neutrino signal in temporal and spatial correlation with the observed X-ray flash of SN 2008D was conducted using data taken in 2007-2008 with 22 strings of the IceCube detector. Events were selected based on a boosted decision tree classifier trained with simulated signal and experimental background data. The classifier was optimized to the position and a "soft jet" neutrino spectrum assumed for SN 2008D. Using three search windows placed around the X-ray peak, emission time scales from 100-10-000 s were probed. No events passing the cuts were observed in agreement with the signal expectation of 0.13 events. Upper limits on the muon neutrino flux from core collapse supernovae were derived for different emission time scales and the principal model parameters were constrained. While no meaningful limits can be given in the case of an isotropic neutrino emission, the parameter space for a jetted emission can be constrained. Future analyses with the full 86 string IceCube detector could detect up to ∼100 events for a core-collapse supernova at 10 Mpc according to the soft jet model.

Original languageEnglish (US)
Article numberA28
JournalAstronomy and Astrophysics
Volume527
Issue number4
DOIs
StatePublished - Mar 1 2011

Fingerprint

neutrinos
supernovae
energy
flash
timescale
classifiers
detectors
x rays
strings
collision
protons
gamma ray bursts
muons
detector
collisions
parameter

Keywords

  • astroparticle physics
  • neutrinos
  • supernovae: individual: SN 2008D

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Abbasi, R., Abdou, Y., Abu-Zayyad, T., Adams, J., Aguilar, J. A., Ahlers, M., ... Zarzhitsky, P. (2011). Constraints on high-energy neutrino emission from SN 2008D. Astronomy and Astrophysics, 527(4), [A28]. https://doi.org/10.1051/0004-6361/201015770

Constraints on high-energy neutrino emission from SN 2008D. / Abbasi, R.; Abdou, Y.; Abu-Zayyad, T.; Adams, J.; Aguilar, J. A.; Ahlers, M.; Andeen, K.; Auffenberg, J.; Bai, X.; Baker, M.; Barwick, S. W.; Bay, R.; Alba, J. L.Bazo; Beattie, K.; Beatty, J. J.; Bechet, S.; Becker, J. K.; Becker, K. H.; Lotfi Benabderrhmane, Mohamed; BenZvi, S.; Berdermann, J.; Berghaus, P.; Berley, D.; Bernardini, E.; Bertrand, D.; Besson, D. Z.; Bissok, M.; Blaufuss, E.; Blumenthal, J.; Boersma, D. J.; Bohm, C.; Bose, D.; Boser, S.; Botner, O.; Braun, J.; Buitink, S.; Carson, M.; Chirkin, D.; Christy, B.; Clem, J.; Clevermann, F.; Cohen, S.; Colnard, C.; Cowen, D. F.; D'Gostino, M. V.; Danninger, M.; Davis, J. C.; De Clercq, C.; Demirors, L.; Depaepe, O.; Descamps, F.; Desiati, P.; De Vries-Uiterweerd, G.; DeYoung, T.; Diaz-Velez, J. C.; Dierckxsens, M.; Dreyer, J.; Dumm, J. P.; Duvoort, M. R.; Ehrlich, R.; Eisch, J.; Ellsworth, R. W.; Engdegard, O.; Euler, S.; Evenson, P. A.; Fadiran, O.; Fazely, A. R.; Fedynitch, A.; Feusels, T.; Filimonov, K.; Finley, C.; Foerster, M. M.; Fox, B. D.; Franckowiak, A.; Franke, R.; Gaisser, T. K.; Gallagher, J.; Geisler, M.; Gerhardt, L.; Gladstone, L.; Glusenkamp, T.; Goldschmidt, A.; Goodman, J. A.; Grant, D.; Griesel, T.; Gro, A.; Grullon, S.; Gurtner, M.; Ha, C.; Hallgren, A.; Halzen, F.; Han, K.; Hanson, K.; Helbing, K.; Herquet, P.; Hickford, S.; Hill, G. C.; Hoffman, K. D.; Homeier, A.; Hoshina, K.; Hubert, D.; Huelsnitz, W.; Hul, J. P.; Hulth, P. O.; Hultqvist, K.; Hussain, S.; Ishihara, A.; Jacobsen, J.; Japaridze, G. S.; Johansson, H.; Joseph, J. M.; Kampert, K. H.; Kappes, A.; Karg, T.; Karle, A.; Kelley, J. L.; Kemming, N.; Kenny, P.; Kiryluk, J.; Kislat, F.; Klein, S. R.; Kohne, J. H.; Kohnen, G.; Kolanoski, H.; Kopke, L.; Koskinen, D. J.; Kowalski, M.; Kowarik, T.; Krasberg, M.; Krings, T.; Kroll, G.; Kuehn, K.; Kuwabara, T.; Labare, M.; Lafebre, S.; Laihem, K.; Landsman, H.; Larson, M. J.; Lauer, R.; Lehmann, R.; Lunemann, J.; Madsen, J.; Majumdar, P.; Marotta, A.; Maruyama, R.; Mase, K.; Matis, H. S.; Matusik, M.; Meagher, K.; Merck, M.; Meszaros, P.; Meures, T.; Middell, E.; Milke, N.; Miller, J.; Montaruli, T.; Morse, R.; Movit, S. M.; Nahnhauer, R.; Nam, J. W.; Naumann, U.; Nießen, P.; Nygren, D. R.; Odrowski, S.; Olivas, A.; Olivo, M.; O'Murchadha, A.; Ono, M.; Panknin, S.; Paul, L.; Perez De Los Heros, C.; Petrovic, J.; Piegsa, A.; Pieloth, D.; Porrata, R.; Posselt, J.; Price, P. B.; Prikockis, M.; Przybylski, G. T.; Rawlins, K.; Redl, P.; Resconi, E.; Rhode, W.; Ribordy, M.; Rizzo, A.; Rodrigues, J. P.; Roth, P.; Rothmaier, F.; Rott, C.; Ruhe, T.; Rutledge, D.; Ruzybayev, B.; Ryckbosch, D.; Sander, H. G.; Santander, M.; Sarkar, S.; Schatto, K.; Schlenstedt, S.; Schmidt, T.; Schukraft, A.; Schultes, A.; Schulz, O.; Schunck, M.; Seckel, D.; Semburg, B.; Seo, S. H.; Sestayo, Y.; Seunarine, S.; Silvestri, A.; Singh, K.; Slipak, A.; Spiczak, G. M.; Spiering, C.; Stamatikos, M.; Stanev, T.; Stephens, G.; Stezelberger, T.; Stokstad, R. G.; Stoyanov, S.; Strahler, E. A.; Straszheim, T.; Sullivan, G. W.; Swillens, Q.; Taavola, H.; Taboada, I.; Tamburro, A.; Tarasova, O.; Tepe, A.; Ter-Antonyan, S.; Tilav, S.; Toale, P. A.; Toscano, S.; Tosi, D.; Turčan, D.; Van Eijndhoven, N.; Vandenbroucke, J.; Van Overloop, A.; Van Santen, J.; Voge, M.; Voigt, B.; Walck, C.; Waldenmaier, T.; Wallraff, M.; Walter, M.; Weaver, C. H.; Wendt, C.; Westerhoff, S.; Whitehorn, N.; Wiebe, K.; Wiebusch, C. H.; Wikstrom, G.; Williams, D. R.; Wischnewski, R.; Wissing, H.; Wolf, M.; Woschnagg, K.; Xu, C.; Xu, X. W.; Yodh, G.; Yoshida, S.; Zarzhitsky, P.

In: Astronomy and Astrophysics, Vol. 527, No. 4, A28, 01.03.2011.

Research output: Contribution to journalArticle

Abbasi, R, Abdou, Y, Abu-Zayyad, T, Adams, J, Aguilar, JA, Ahlers, M, Andeen, K, Auffenberg, J, Bai, X, Baker, M, Barwick, SW, Bay, R, Alba, JLB, Beattie, K, Beatty, JJ, Bechet, S, Becker, JK, Becker, KH, Lotfi Benabderrhmane, M, BenZvi, S, Berdermann, J, Berghaus, P, Berley, D, Bernardini, E, Bertrand, D, Besson, DZ, Bissok, M, Blaufuss, E, Blumenthal, J, Boersma, DJ, Bohm, C, Bose, D, Boser, S, Botner, O, Braun, J, Buitink, S, Carson, M, Chirkin, D, Christy, B, Clem, J, Clevermann, F, Cohen, S, Colnard, C, Cowen, DF, D'Gostino, MV, Danninger, M, Davis, JC, De Clercq, C, Demirors, L, Depaepe, O, Descamps, F, Desiati, P, De Vries-Uiterweerd, G, DeYoung, T, Diaz-Velez, JC, Dierckxsens, M, Dreyer, J, Dumm, JP, Duvoort, MR, Ehrlich, R, Eisch, J, Ellsworth, RW, Engdegard, O, Euler, S, Evenson, PA, Fadiran, O, Fazely, AR, Fedynitch, A, Feusels, T, Filimonov, K, Finley, C, Foerster, MM, Fox, BD, Franckowiak, A, Franke, R, Gaisser, TK, Gallagher, J, Geisler, M, Gerhardt, L, Gladstone, L, Glusenkamp, T, Goldschmidt, A, Goodman, JA, Grant, D, Griesel, T, Gro, A, Grullon, S, Gurtner, M, Ha, C, Hallgren, A, Halzen, F, Han, K, Hanson, K, Helbing, K, Herquet, P, Hickford, S, Hill, GC, Hoffman, KD, Homeier, A, Hoshina, K, Hubert, D, Huelsnitz, W, Hul, JP, Hulth, PO, Hultqvist, K, Hussain, S, Ishihara, A, Jacobsen, J, Japaridze, GS, Johansson, H, Joseph, JM, Kampert, KH, Kappes, A, Karg, T, Karle, A, Kelley, JL, Kemming, N, Kenny, P, Kiryluk, J, Kislat, F, Klein, SR, Kohne, JH, Kohnen, G, Kolanoski, H, Kopke, L, Koskinen, DJ, Kowalski, M, Kowarik, T, Krasberg, M, Krings, T, Kroll, G, Kuehn, K, Kuwabara, T, Labare, M, Lafebre, S, Laihem, K, Landsman, H, Larson, MJ, Lauer, R, Lehmann, R, Lunemann, J, Madsen, J, Majumdar, P, Marotta, A, Maruyama, R, Mase, K, Matis, HS, Matusik, M, Meagher, K, Merck, M, Meszaros, P, Meures, T, Middell, E, Milke, N, Miller, J, Montaruli, T, Morse, R, Movit, SM, Nahnhauer, R, Nam, JW, Naumann, U, Nießen, P, Nygren, DR, Odrowski, S, Olivas, A, Olivo, M, O'Murchadha, A, Ono, M, Panknin, S, Paul, L, Perez De Los Heros, C, Petrovic, J, Piegsa, A, Pieloth, D, Porrata, R, Posselt, J, Price, PB, Prikockis, M, Przybylski, GT, Rawlins, K, Redl, P, Resconi, E, Rhode, W, Ribordy, M, Rizzo, A, Rodrigues, JP, Roth, P, Rothmaier, F, Rott, C, Ruhe, T, Rutledge, D, Ruzybayev, B, Ryckbosch, D, Sander, HG, Santander, M, Sarkar, S, Schatto, K, Schlenstedt, S, Schmidt, T, Schukraft, A, Schultes, A, Schulz, O, Schunck, M, Seckel, D, Semburg, B, Seo, SH, Sestayo, Y, Seunarine, S, Silvestri, A, Singh, K, Slipak, A, Spiczak, GM, Spiering, C, Stamatikos, M, Stanev, T, Stephens, G, Stezelberger, T, Stokstad, RG, Stoyanov, S, Strahler, EA, Straszheim, T, Sullivan, GW, Swillens, Q, Taavola, H, Taboada, I, Tamburro, A, Tarasova, O, Tepe, A, Ter-Antonyan, S, Tilav, S, Toale, PA, Toscano, S, Tosi, D, Turčan, D, Van Eijndhoven, N, Vandenbroucke, J, Van Overloop, A, Van Santen, J, Voge, M, Voigt, B, Walck, C, Waldenmaier, T, Wallraff, M, Walter, M, Weaver, CH, Wendt, C, Westerhoff, S, Whitehorn, N, Wiebe, K, Wiebusch, CH, Wikstrom, G, Williams, DR, Wischnewski, R, Wissing, H, Wolf, M, Woschnagg, K, Xu, C, Xu, XW, Yodh, G, Yoshida, S & Zarzhitsky, P 2011, 'Constraints on high-energy neutrino emission from SN 2008D', Astronomy and Astrophysics, vol. 527, no. 4, A28. https://doi.org/10.1051/0004-6361/201015770
Abbasi R, Abdou Y, Abu-Zayyad T, Adams J, Aguilar JA, Ahlers M et al. Constraints on high-energy neutrino emission from SN 2008D. Astronomy and Astrophysics. 2011 Mar 1;527(4). A28. https://doi.org/10.1051/0004-6361/201015770
Abbasi, R. ; Abdou, Y. ; Abu-Zayyad, T. ; Adams, J. ; Aguilar, J. A. ; Ahlers, M. ; Andeen, K. ; Auffenberg, J. ; Bai, X. ; Baker, M. ; Barwick, S. W. ; Bay, R. ; Alba, J. L.Bazo ; Beattie, K. ; Beatty, J. J. ; Bechet, S. ; Becker, J. K. ; Becker, K. H. ; Lotfi Benabderrhmane, Mohamed ; BenZvi, S. ; Berdermann, J. ; Berghaus, P. ; Berley, D. ; Bernardini, E. ; Bertrand, D. ; Besson, D. Z. ; Bissok, M. ; Blaufuss, E. ; Blumenthal, J. ; Boersma, D. J. ; Bohm, C. ; Bose, D. ; Boser, S. ; Botner, O. ; Braun, J. ; Buitink, S. ; Carson, M. ; Chirkin, D. ; Christy, B. ; Clem, J. ; Clevermann, F. ; Cohen, S. ; Colnard, C. ; Cowen, D. F. ; D'Gostino, M. V. ; Danninger, M. ; Davis, J. C. ; De Clercq, C. ; Demirors, L. ; Depaepe, O. ; Descamps, F. ; Desiati, P. ; De Vries-Uiterweerd, G. ; DeYoung, T. ; Diaz-Velez, J. C. ; Dierckxsens, M. ; Dreyer, J. ; Dumm, J. P. ; Duvoort, M. R. ; Ehrlich, R. ; Eisch, J. ; Ellsworth, R. W. ; Engdegard, O. ; Euler, S. ; Evenson, P. A. ; Fadiran, O. ; Fazely, A. R. ; Fedynitch, A. ; Feusels, T. ; Filimonov, K. ; Finley, C. ; Foerster, M. M. ; Fox, B. D. ; Franckowiak, A. ; Franke, R. ; Gaisser, T. K. ; Gallagher, J. ; Geisler, M. ; Gerhardt, L. ; Gladstone, L. ; Glusenkamp, T. ; Goldschmidt, A. ; Goodman, J. A. ; Grant, D. ; Griesel, T. ; Gro, A. ; Grullon, S. ; Gurtner, M. ; Ha, C. ; Hallgren, A. ; Halzen, F. ; Han, K. ; Hanson, K. ; Helbing, K. ; Herquet, P. ; Hickford, S. ; Hill, G. C. ; Hoffman, K. D. ; Homeier, A. ; Hoshina, K. ; Hubert, D. ; Huelsnitz, W. ; Hul, J. P. ; Hulth, P. O. ; Hultqvist, K. ; Hussain, S. ; Ishihara, A. ; Jacobsen, J. ; Japaridze, G. S. ; Johansson, H. ; Joseph, J. M. ; Kampert, K. H. ; Kappes, A. ; Karg, T. ; Karle, A. ; Kelley, J. L. ; Kemming, N. ; Kenny, P. ; Kiryluk, J. ; Kislat, F. ; Klein, S. R. ; Kohne, J. H. ; Kohnen, G. ; Kolanoski, H. ; Kopke, L. ; Koskinen, D. J. ; Kowalski, M. ; Kowarik, T. ; Krasberg, M. ; Krings, T. ; Kroll, G. ; Kuehn, K. ; Kuwabara, T. ; Labare, M. ; Lafebre, S. ; Laihem, K. ; Landsman, H. ; Larson, M. J. ; Lauer, R. ; Lehmann, R. ; Lunemann, J. ; Madsen, J. ; Majumdar, P. ; Marotta, A. ; Maruyama, R. ; Mase, K. ; Matis, H. S. ; Matusik, M. ; Meagher, K. ; Merck, M. ; Meszaros, P. ; Meures, T. ; Middell, E. ; Milke, N. ; Miller, J. ; Montaruli, T. ; Morse, R. ; Movit, S. M. ; Nahnhauer, R. ; Nam, J. W. ; Naumann, U. ; Nießen, P. ; Nygren, D. R. ; Odrowski, S. ; Olivas, A. ; Olivo, M. ; O'Murchadha, A. ; Ono, M. ; Panknin, S. ; Paul, L. ; Perez De Los Heros, C. ; Petrovic, J. ; Piegsa, A. ; Pieloth, D. ; Porrata, R. ; Posselt, J. ; Price, P. B. ; Prikockis, M. ; Przybylski, G. T. ; Rawlins, K. ; Redl, P. ; Resconi, E. ; Rhode, W. ; Ribordy, M. ; Rizzo, A. ; Rodrigues, J. P. ; Roth, P. ; Rothmaier, F. ; Rott, C. ; Ruhe, T. ; Rutledge, D. ; Ruzybayev, B. ; Ryckbosch, D. ; Sander, H. G. ; Santander, M. ; Sarkar, S. ; Schatto, K. ; Schlenstedt, S. ; Schmidt, T. ; Schukraft, A. ; Schultes, A. ; Schulz, O. ; Schunck, M. ; Seckel, D. ; Semburg, B. ; Seo, S. H. ; Sestayo, Y. ; Seunarine, S. ; Silvestri, A. ; Singh, K. ; Slipak, A. ; Spiczak, G. M. ; Spiering, C. ; Stamatikos, M. ; Stanev, T. ; Stephens, G. ; Stezelberger, T. ; Stokstad, R. G. ; Stoyanov, S. ; Strahler, E. A. ; Straszheim, T. ; Sullivan, G. W. ; Swillens, Q. ; Taavola, H. ; Taboada, I. ; Tamburro, A. ; Tarasova, O. ; Tepe, A. ; Ter-Antonyan, S. ; Tilav, S. ; Toale, P. A. ; Toscano, S. ; Tosi, D. ; Turčan, D. ; Van Eijndhoven, N. ; Vandenbroucke, J. ; Van Overloop, A. ; Van Santen, J. ; Voge, M. ; Voigt, B. ; Walck, C. ; Waldenmaier, T. ; Wallraff, M. ; Walter, M. ; Weaver, C. H. ; Wendt, C. ; Westerhoff, S. ; Whitehorn, N. ; Wiebe, K. ; Wiebusch, C. H. ; Wikstrom, G. ; Williams, D. R. ; Wischnewski, R. ; Wissing, H. ; Wolf, M. ; Woschnagg, K. ; Xu, C. ; Xu, X. W. ; Yodh, G. ; Yoshida, S. ; Zarzhitsky, P. / Constraints on high-energy neutrino emission from SN 2008D. In: Astronomy and Astrophysics. 2011 ; Vol. 527, No. 4.
@article{63029b86ef1e418ab8cb96feb7bf0b2d,
title = "Constraints on high-energy neutrino emission from SN 2008D",
abstract = "SN 2008D, a core collapse supernova at a distance of 27 Mpc, was serendipitously discovered by the Swift satellite through an associated X-ray flash. Core collapse supernovae have been observed in association with long gamma-ray bursts and X-ray flashes and a physical connection is widely assumed. This connection could imply that some core collapse supernovae possess mildly relativistic jets in which high-energy neutrinos are produced through proton-proton collisions. The predicted neutrino spectra would be detectable by Cherenkov neutrino detectors like IceCube. A search for a neutrino signal in temporal and spatial correlation with the observed X-ray flash of SN 2008D was conducted using data taken in 2007-2008 with 22 strings of the IceCube detector. Events were selected based on a boosted decision tree classifier trained with simulated signal and experimental background data. The classifier was optimized to the position and a {"}soft jet{"} neutrino spectrum assumed for SN 2008D. Using three search windows placed around the X-ray peak, emission time scales from 100-10-000 s were probed. No events passing the cuts were observed in agreement with the signal expectation of 0.13 events. Upper limits on the muon neutrino flux from core collapse supernovae were derived for different emission time scales and the principal model parameters were constrained. While no meaningful limits can be given in the case of an isotropic neutrino emission, the parameter space for a jetted emission can be constrained. Future analyses with the full 86 string IceCube detector could detect up to ∼100 events for a core-collapse supernova at 10 Mpc according to the soft jet model.",
keywords = "astroparticle physics, neutrinos, supernovae: individual: SN 2008D",
author = "R. Abbasi and Y. Abdou and T. Abu-Zayyad and J. Adams and Aguilar, {J. A.} and M. Ahlers and K. Andeen and J. Auffenberg and X. Bai and M. Baker and Barwick, {S. W.} and R. Bay and Alba, {J. L.Bazo} and K. Beattie and Beatty, {J. J.} and S. Bechet and Becker, {J. K.} and Becker, {K. H.} and {Lotfi Benabderrhmane}, Mohamed and S. BenZvi and J. Berdermann and P. Berghaus and D. Berley and E. Bernardini and D. Bertrand and Besson, {D. Z.} and M. Bissok and E. Blaufuss and J. Blumenthal and Boersma, {D. J.} and C. Bohm and D. Bose and S. Boser and O. Botner and J. Braun and S. Buitink and M. Carson and D. Chirkin and B. Christy and J. Clem and F. Clevermann and S. Cohen and C. Colnard and Cowen, {D. F.} and D'Gostino, {M. V.} and M. Danninger and Davis, {J. C.} and {De Clercq}, C. and L. Demirors and O. Depaepe and F. Descamps and P. Desiati and {De Vries-Uiterweerd}, G. and T. DeYoung and Diaz-Velez, {J. C.} and M. Dierckxsens and J. Dreyer and Dumm, {J. P.} and Duvoort, {M. R.} and R. Ehrlich and J. Eisch and Ellsworth, {R. W.} and O. Engdegard and S. Euler and Evenson, {P. A.} and O. Fadiran and Fazely, {A. R.} and A. Fedynitch and T. Feusels and K. Filimonov and C. Finley and Foerster, {M. M.} and Fox, {B. D.} and A. Franckowiak and R. Franke and Gaisser, {T. K.} and J. Gallagher and M. Geisler and L. Gerhardt and L. Gladstone and T. Glusenkamp and A. Goldschmidt and Goodman, {J. A.} and D. Grant and T. Griesel and A. Gro and S. Grullon and M. Gurtner and C. Ha and A. Hallgren and F. Halzen and K. Han and K. Hanson and K. Helbing and P. Herquet and S. Hickford and Hill, {G. C.} and Hoffman, {K. D.} and A. Homeier and K. Hoshina and D. Hubert and W. Huelsnitz and Hul, {J. P.} and Hulth, {P. O.} and K. Hultqvist and S. Hussain and A. Ishihara and J. Jacobsen and Japaridze, {G. S.} and H. Johansson and Joseph, {J. M.} and Kampert, {K. H.} and A. Kappes and T. Karg and A. Karle and Kelley, {J. L.} and N. Kemming and P. Kenny and J. Kiryluk and F. Kislat and Klein, {S. R.} and Kohne, {J. H.} and G. Kohnen and H. Kolanoski and L. Kopke and Koskinen, {D. J.} and M. Kowalski and T. Kowarik and M. Krasberg and T. Krings and G. Kroll and K. Kuehn and T. Kuwabara and M. Labare and S. Lafebre and K. Laihem and H. Landsman and Larson, {M. J.} and R. Lauer and R. Lehmann and J. Lunemann and J. Madsen and P. Majumdar and A. Marotta and R. Maruyama and K. Mase and Matis, {H. S.} and M. Matusik and K. Meagher and M. Merck and P. Meszaros and T. Meures and E. Middell and N. Milke and J. Miller and T. Montaruli and R. Morse and Movit, {S. M.} and R. Nahnhauer and Nam, {J. W.} and U. Naumann and P. Nie{\ss}en and Nygren, {D. R.} and S. Odrowski and A. Olivas and M. Olivo and A. O'Murchadha and M. Ono and S. Panknin and L. Paul and {Perez De Los Heros}, C. and J. Petrovic and A. Piegsa and D. Pieloth and R. Porrata and J. Posselt and Price, {P. B.} and M. Prikockis and Przybylski, {G. T.} and K. Rawlins and P. Redl and E. Resconi and W. Rhode and M. Ribordy and A. Rizzo and Rodrigues, {J. P.} and P. Roth and F. Rothmaier and C. Rott and T. Ruhe and D. Rutledge and B. Ruzybayev and D. Ryckbosch and Sander, {H. G.} and M. Santander and S. Sarkar and K. Schatto and S. Schlenstedt and T. Schmidt and A. Schukraft and A. Schultes and O. Schulz and M. Schunck and D. Seckel and B. Semburg and Seo, {S. H.} and Y. Sestayo and S. Seunarine and A. Silvestri and K. Singh and A. Slipak and Spiczak, {G. M.} and C. Spiering and M. Stamatikos and T. Stanev and G. Stephens and T. Stezelberger and Stokstad, {R. G.} and S. Stoyanov and Strahler, {E. A.} and T. Straszheim and Sullivan, {G. W.} and Q. Swillens and H. Taavola and I. Taboada and A. Tamburro and O. Tarasova and A. Tepe and S. Ter-Antonyan and S. Tilav and Toale, {P. A.} and S. Toscano and D. Tosi and D. Turčan and {Van Eijndhoven}, N. and J. Vandenbroucke and {Van Overloop}, A. and {Van Santen}, J. and M. Voge and B. Voigt and C. Walck and T. Waldenmaier and M. Wallraff and M. Walter and Weaver, {C. H.} and C. Wendt and S. Westerhoff and N. Whitehorn and K. Wiebe and Wiebusch, {C. H.} and G. Wikstrom and Williams, {D. R.} and R. Wischnewski and H. Wissing and M. Wolf and K. Woschnagg and C. Xu and Xu, {X. W.} and G. Yodh and S. Yoshida and P. Zarzhitsky",
year = "2011",
month = "3",
day = "1",
doi = "10.1051/0004-6361/201015770",
language = "English (US)",
volume = "527",
journal = "Astronomy and Astrophysics",
issn = "0004-6361",
publisher = "EDP Sciences",
number = "4",

}

TY - JOUR

T1 - Constraints on high-energy neutrino emission from SN 2008D

AU - Abbasi, R.

AU - Abdou, Y.

AU - Abu-Zayyad, T.

AU - Adams, J.

AU - Aguilar, J. A.

AU - Ahlers, M.

AU - Andeen, K.

AU - Auffenberg, J.

AU - Bai, X.

AU - Baker, M.

AU - Barwick, S. W.

AU - Bay, R.

AU - Alba, J. L.Bazo

AU - Beattie, K.

AU - Beatty, J. J.

AU - Bechet, S.

AU - Becker, J. K.

AU - Becker, K. H.

AU - Lotfi Benabderrhmane, Mohamed

AU - BenZvi, S.

AU - Berdermann, J.

AU - Berghaus, P.

AU - Berley, D.

AU - Bernardini, E.

AU - Bertrand, D.

AU - Besson, D. Z.

AU - Bissok, M.

AU - Blaufuss, E.

AU - Blumenthal, J.

AU - Boersma, D. J.

AU - Bohm, C.

AU - Bose, D.

AU - Boser, S.

AU - Botner, O.

AU - Braun, J.

AU - Buitink, S.

AU - Carson, M.

AU - Chirkin, D.

AU - Christy, B.

AU - Clem, J.

AU - Clevermann, F.

AU - Cohen, S.

AU - Colnard, C.

AU - Cowen, D. F.

AU - D'Gostino, M. V.

AU - Danninger, M.

AU - Davis, J. C.

AU - De Clercq, C.

AU - Demirors, L.

AU - Depaepe, O.

AU - Descamps, F.

AU - Desiati, P.

AU - De Vries-Uiterweerd, G.

AU - DeYoung, T.

AU - Diaz-Velez, J. C.

AU - Dierckxsens, M.

AU - Dreyer, J.

AU - Dumm, J. P.

AU - Duvoort, M. R.

AU - Ehrlich, R.

AU - Eisch, J.

AU - Ellsworth, R. W.

AU - Engdegard, O.

AU - Euler, S.

AU - Evenson, P. A.

AU - Fadiran, O.

AU - Fazely, A. R.

AU - Fedynitch, A.

AU - Feusels, T.

AU - Filimonov, K.

AU - Finley, C.

AU - Foerster, M. M.

AU - Fox, B. D.

AU - Franckowiak, A.

AU - Franke, R.

AU - Gaisser, T. K.

AU - Gallagher, J.

AU - Geisler, M.

AU - Gerhardt, L.

AU - Gladstone, L.

AU - Glusenkamp, T.

AU - Goldschmidt, A.

AU - Goodman, J. A.

AU - Grant, D.

AU - Griesel, T.

AU - Gro, A.

AU - Grullon, S.

AU - Gurtner, M.

AU - Ha, C.

AU - Hallgren, A.

AU - Halzen, F.

AU - Han, K.

AU - Hanson, K.

AU - Helbing, K.

AU - Herquet, P.

AU - Hickford, S.

AU - Hill, G. C.

AU - Hoffman, K. D.

AU - Homeier, A.

AU - Hoshina, K.

AU - Hubert, D.

AU - Huelsnitz, W.

AU - Hul, J. P.

AU - Hulth, P. O.

AU - Hultqvist, K.

AU - Hussain, S.

AU - Ishihara, A.

AU - Jacobsen, J.

AU - Japaridze, G. S.

AU - Johansson, H.

AU - Joseph, J. M.

AU - Kampert, K. H.

AU - Kappes, A.

AU - Karg, T.

AU - Karle, A.

AU - Kelley, J. L.

AU - Kemming, N.

AU - Kenny, P.

AU - Kiryluk, J.

AU - Kislat, F.

AU - Klein, S. R.

AU - Kohne, J. H.

AU - Kohnen, G.

AU - Kolanoski, H.

AU - Kopke, L.

AU - Koskinen, D. J.

AU - Kowalski, M.

AU - Kowarik, T.

AU - Krasberg, M.

AU - Krings, T.

AU - Kroll, G.

AU - Kuehn, K.

AU - Kuwabara, T.

AU - Labare, M.

AU - Lafebre, S.

AU - Laihem, K.

AU - Landsman, H.

AU - Larson, M. J.

AU - Lauer, R.

AU - Lehmann, R.

AU - Lunemann, J.

AU - Madsen, J.

AU - Majumdar, P.

AU - Marotta, A.

AU - Maruyama, R.

AU - Mase, K.

AU - Matis, H. S.

AU - Matusik, M.

AU - Meagher, K.

AU - Merck, M.

AU - Meszaros, P.

AU - Meures, T.

AU - Middell, E.

AU - Milke, N.

AU - Miller, J.

AU - Montaruli, T.

AU - Morse, R.

AU - Movit, S. M.

AU - Nahnhauer, R.

AU - Nam, J. W.

AU - Naumann, U.

AU - Nießen, P.

AU - Nygren, D. R.

AU - Odrowski, S.

AU - Olivas, A.

AU - Olivo, M.

AU - O'Murchadha, A.

AU - Ono, M.

AU - Panknin, S.

AU - Paul, L.

AU - Perez De Los Heros, C.

AU - Petrovic, J.

AU - Piegsa, A.

AU - Pieloth, D.

AU - Porrata, R.

AU - Posselt, J.

AU - Price, P. B.

AU - Prikockis, M.

AU - Przybylski, G. T.

AU - Rawlins, K.

AU - Redl, P.

AU - Resconi, E.

AU - Rhode, W.

AU - Ribordy, M.

AU - Rizzo, A.

AU - Rodrigues, J. P.

AU - Roth, P.

AU - Rothmaier, F.

AU - Rott, C.

AU - Ruhe, T.

AU - Rutledge, D.

AU - Ruzybayev, B.

AU - Ryckbosch, D.

AU - Sander, H. G.

AU - Santander, M.

AU - Sarkar, S.

AU - Schatto, K.

AU - Schlenstedt, S.

AU - Schmidt, T.

AU - Schukraft, A.

AU - Schultes, A.

AU - Schulz, O.

AU - Schunck, M.

AU - Seckel, D.

AU - Semburg, B.

AU - Seo, S. H.

AU - Sestayo, Y.

AU - Seunarine, S.

AU - Silvestri, A.

AU - Singh, K.

AU - Slipak, A.

AU - Spiczak, G. M.

AU - Spiering, C.

AU - Stamatikos, M.

AU - Stanev, T.

AU - Stephens, G.

AU - Stezelberger, T.

AU - Stokstad, R. G.

AU - Stoyanov, S.

AU - Strahler, E. A.

AU - Straszheim, T.

AU - Sullivan, G. W.

AU - Swillens, Q.

AU - Taavola, H.

AU - Taboada, I.

AU - Tamburro, A.

AU - Tarasova, O.

AU - Tepe, A.

AU - Ter-Antonyan, S.

AU - Tilav, S.

AU - Toale, P. A.

AU - Toscano, S.

AU - Tosi, D.

AU - Turčan, D.

AU - Van Eijndhoven, N.

AU - Vandenbroucke, J.

AU - Van Overloop, A.

AU - Van Santen, J.

AU - Voge, M.

AU - Voigt, B.

AU - Walck, C.

AU - Waldenmaier, T.

AU - Wallraff, M.

AU - Walter, M.

AU - Weaver, C. H.

AU - Wendt, C.

AU - Westerhoff, S.

AU - Whitehorn, N.

AU - Wiebe, K.

AU - Wiebusch, C. H.

AU - Wikstrom, G.

AU - Williams, D. R.

AU - Wischnewski, R.

AU - Wissing, H.

AU - Wolf, M.

AU - Woschnagg, K.

AU - Xu, C.

AU - Xu, X. W.

AU - Yodh, G.

AU - Yoshida, S.

AU - Zarzhitsky, P.

PY - 2011/3/1

Y1 - 2011/3/1

N2 - SN 2008D, a core collapse supernova at a distance of 27 Mpc, was serendipitously discovered by the Swift satellite through an associated X-ray flash. Core collapse supernovae have been observed in association with long gamma-ray bursts and X-ray flashes and a physical connection is widely assumed. This connection could imply that some core collapse supernovae possess mildly relativistic jets in which high-energy neutrinos are produced through proton-proton collisions. The predicted neutrino spectra would be detectable by Cherenkov neutrino detectors like IceCube. A search for a neutrino signal in temporal and spatial correlation with the observed X-ray flash of SN 2008D was conducted using data taken in 2007-2008 with 22 strings of the IceCube detector. Events were selected based on a boosted decision tree classifier trained with simulated signal and experimental background data. The classifier was optimized to the position and a "soft jet" neutrino spectrum assumed for SN 2008D. Using three search windows placed around the X-ray peak, emission time scales from 100-10-000 s were probed. No events passing the cuts were observed in agreement with the signal expectation of 0.13 events. Upper limits on the muon neutrino flux from core collapse supernovae were derived for different emission time scales and the principal model parameters were constrained. While no meaningful limits can be given in the case of an isotropic neutrino emission, the parameter space for a jetted emission can be constrained. Future analyses with the full 86 string IceCube detector could detect up to ∼100 events for a core-collapse supernova at 10 Mpc according to the soft jet model.

AB - SN 2008D, a core collapse supernova at a distance of 27 Mpc, was serendipitously discovered by the Swift satellite through an associated X-ray flash. Core collapse supernovae have been observed in association with long gamma-ray bursts and X-ray flashes and a physical connection is widely assumed. This connection could imply that some core collapse supernovae possess mildly relativistic jets in which high-energy neutrinos are produced through proton-proton collisions. The predicted neutrino spectra would be detectable by Cherenkov neutrino detectors like IceCube. A search for a neutrino signal in temporal and spatial correlation with the observed X-ray flash of SN 2008D was conducted using data taken in 2007-2008 with 22 strings of the IceCube detector. Events were selected based on a boosted decision tree classifier trained with simulated signal and experimental background data. The classifier was optimized to the position and a "soft jet" neutrino spectrum assumed for SN 2008D. Using three search windows placed around the X-ray peak, emission time scales from 100-10-000 s were probed. No events passing the cuts were observed in agreement with the signal expectation of 0.13 events. Upper limits on the muon neutrino flux from core collapse supernovae were derived for different emission time scales and the principal model parameters were constrained. While no meaningful limits can be given in the case of an isotropic neutrino emission, the parameter space for a jetted emission can be constrained. Future analyses with the full 86 string IceCube detector could detect up to ∼100 events for a core-collapse supernova at 10 Mpc according to the soft jet model.

KW - astroparticle physics

KW - neutrinos

KW - supernovae: individual: SN 2008D

UR - http://www.scopus.com/inward/record.url?scp=78951494727&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=78951494727&partnerID=8YFLogxK

U2 - 10.1051/0004-6361/201015770

DO - 10.1051/0004-6361/201015770

M3 - Article

VL - 527

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

SN - 0004-6361

IS - 4

M1 - A28

ER -