IceCube sensitivity for low-energy neutrinos from nearby supernovae

R. Abbasi, Y. Abdou, T. Abu-Zayyad, M. Ackermann, J. Adams, J. A. Aguilar, M. Ahlers, M. M. Allen, D. Altmann, K. Andeen, J. Auffenberg, X. Bai, M. Baker, S. W. Barwick, V. Baum, R. Bay, J. L. Bazo Alba, K. Beattie, J. J. Beatty, S. Bechet & 244 others J. K. Becker, K. H. Becker, Mohamed Lotfi Benabderrhmane, S. Benzvi, J. Berdermann, P. Berghaus, D. Berley, E. Bernardini, D. Bertrand, D. Z. Besson, D. Bindig, M. Bissok, E. Blaufuss, J. Blumenthal, D. J. Boersma, C. Bohm, D. Bose, S. Böser, O. Botner, A. M. Brown, S. Buitink, K. S. Caballero-Mora, M. Carson, D. Chirkin, B. Christy, F. Clevermann, S. Cohen, C. Colnard, D. F. Cowen, A. H. Cruz Silva, M. V. D'Agostino, M. Danninger, J. Daughhetee, J. C. Davis, C. De Clercq, T. Degner, L. Demirörs, F. Descamps, P. Desiati, G. De Vries-Uiterweerd, T. Deyoung, J. C. Díaz-Vélez, M. Dierckxsens, J. Dreyer, J. P. Dumm, M. Dunkman, J. Eisch, R. W. Ellsworth, O. Engdegård, S. Euler, P. A. Evenson, O. Fadiran, A. R. Fazely, A. Fedynitch, J. Feintzeig, T. Feusels, K. Filimonov, C. Finley, T. Fischer-Wasels, B. D. Fox, A. Franckowiak, R. Franke, T. K. Gaisser, J. Gallagher, L. Gerhardt, L. Gladstone, T. Glüsenkamp, A. Goldschmidt, J. A. Goodman, D. Góra, D. Grant, T. Griesel, A. Groß, S. Grullon, M. Gurtner, C. Ha, A. Hajismail, A. Hallgren, F. Halzen, K. Han, K. Hanson, D. Heinen, K. Helbing, R. Hellauer, S. Hickford, G. C. Hill, K. D. Hoffman, B. Hoffmann, A. Homeier, K. Hoshina, W. Huelsnitz, J. P. Hülß, P. O. Hulth, K. Hultqvist, S. Hussain, A. Ishihara, E. Jakobi, J. Jacobsen, G. S. Japaridze, H. Johansson, K. H. Kampert, A. Kappes, T. Karg, A. Karle, P. Kenny, J. Kiryluk, F. Kislat, S. R. Klein, H. Köhne, G. Kohnen, H. Kolanoski, L. Köpke, S. Kopper, D. J. Koskinen, M. Kowalski, T. Kowarik, M. Krasberg, G. Kroll, N. Kurahashi, T. Kuwabara, M. Labare, K. Laihem, H. Landsman, M. J. Larson, R. Lauer, J. Lünemann, J. Madsen, A. Marotta, R. Maruyama, K. Mase, H. S. Matis, K. Meagher, M. Merck, P. Mészáros, T. Meures, S. Miarecki, E. Middell, N. Milke, J. Miller, T. Montaruli, R. Morse, S. M. Movit, R. Nahnhauer, J. W. Nam, U. Naumann, D. R. Nygren, S. Odrowski, A. Olivas, M. Olivo, A. O'Murchadha, S. Panknin, L. Paul, C. Pérez De Los Heros, J. Petrovic, A. Piegsa, D. Pieloth, R. Porrata, J. Posselt, P. B. Price, G. T. Przybylski, K. Rawlins, P. Redl, E. Resconi, W. Rhode, M. Ribordy, A. S. Richard, M. Richman, J. P. Rodrigues, F. Rothmaier, C. Rott, T. Ruhe, D. Rutledge, B. Ruzybayev, D. Ryckbosch, H. G. Sander, M. Santander, S. Sarkar, K. Schatto, T. Schmidt, A. Schönwald, A. Schukraft, L. Schulte, 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, T. Stezelberger, R. G. Stokstad, A. Stößl, E. A. Strahler, R. Ström, M. Stüer, G. W. Sullivan, Q. Swillens, H. Taavola, I. Taboada, A. Tamburro, A. Tepe, S. Ter-Antonyan, S. Tilav, P. A. Toale, S. Toscano, D. Tosi, N. Van Eijndhoven, J. Vandenbroucke, A. Van Overloop, J. Van Santen, M. Vehring, M. Voge, C. Walck, T. Waldenmaier, M. Wallraff, M. Walter, Ch Weaver, C. Wendt, S. Westerhoff, N. Whitehorn, K. Wiebe, C. H. Wiebusch, D. R. Williams, R. Wischnewski, H. Wissing, M. Wolf, T. R. Wood, K. Woschnagg, C. Xu, D. L. Xu, X. W. Xu, J. P. Yanez, G. Yodh, S. Yoshida, P. Zarzhitsky, M. Zoll

    Research output: Contribution to journalArticle

    Abstract

    This paper describes the response of the IceCube neutrino telescope located at the geographic south pole to outbursts of MeV neutrinos from the core collapse of nearby massive stars. IceCube was completed in December 2010 forming a lattice of 5160 photomultiplier tubes that monitor a volume of ∼1 km 3 in the deep Antarctic ice for particle induced photons. The telescope was designed to detect neutrinos with energies greater than 100 GeV. Owing to subfreezing ice temperatures, the photomultiplier dark noise rates are particularly low. Hence IceCube can also detect large numbers of MeV neutrinos by observing a collective rise in all photomultiplier rates on top of the dark noise. With 2 ms timing resolution, IceCube can detect subtle features in the temporal development of the supernova neutrino burst. For a supernova at the galactic center, its sensitivity matches that of a background-free megaton-scale supernova search experiment. The sensitivity decreases to 20 standard deviations at the galactic edge (30 kpc) and 6 standard deviations at the Large Magellanic Cloud (50 kpc). IceCube is sending triggers from potential supernovae to the Supernova Early Warning System. The sensitivity to neutrino properties such as the neutrino hierarchy is discussed, as well as the possibility to

    Original languageEnglish (US)
    Article numberA109
    JournalAstronomy and Astrophysics
    Volume535
    DOIs
    StatePublished - Nov 25 2011

    Fingerprint

    supernovae
    neutrinos
    ice
    early warning system
    sensitivity
    outburst
    energy
    standard deviation
    early warning systems
    telescopes
    experiment
    temperature
    Magellanic clouds
    photomultiplier tubes
    rate
    massive stars
    hierarchies
    bursts
    poles
    actuators

    ASJC Scopus subject areas

    • Astronomy and Astrophysics
    • Space and Planetary Science

    Cite this

    Abbasi, R., Abdou, Y., Abu-Zayyad, T., Ackermann, M., Adams, J., Aguilar, J. A., ... Zoll, M. (2011). IceCube sensitivity for low-energy neutrinos from nearby supernovae. Astronomy and Astrophysics, 535, [A109]. https://doi.org/10.1051/0004-6361/201117810

    IceCube sensitivity for low-energy neutrinos from nearby supernovae. / Abbasi, R.; Abdou, Y.; Abu-Zayyad, T.; Ackermann, M.; Adams, J.; Aguilar, J. A.; Ahlers, M.; Allen, M. M.; Altmann, D.; Andeen, K.; Auffenberg, J.; Bai, X.; Baker, M.; Barwick, S. W.; Baum, V.; Bay, R.; Bazo Alba, J. L.; 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.; Bindig, D.; Bissok, M.; Blaufuss, E.; Blumenthal, J.; Boersma, D. J.; Bohm, C.; Bose, D.; Böser, S.; Botner, O.; Brown, A. M.; Buitink, S.; Caballero-Mora, K. S.; Carson, M.; Chirkin, D.; Christy, B.; Clevermann, F.; Cohen, S.; Colnard, C.; Cowen, D. F.; Cruz Silva, A. H.; D'Agostino, M. V.; Danninger, M.; Daughhetee, J.; Davis, J. C.; De Clercq, C.; Degner, T.; Demirörs, L.; Descamps, F.; Desiati, P.; De Vries-Uiterweerd, G.; Deyoung, T.; Díaz-Vélez, J. C.; Dierckxsens, M.; Dreyer, J.; Dumm, J. P.; Dunkman, M.; Eisch, J.; Ellsworth, R. W.; Engdegård, O.; Euler, S.; Evenson, P. A.; Fadiran, O.; Fazely, A. R.; Fedynitch, A.; Feintzeig, J.; Feusels, T.; Filimonov, K.; Finley, C.; Fischer-Wasels, T.; Fox, B. D.; Franckowiak, A.; Franke, R.; Gaisser, T. K.; Gallagher, J.; Gerhardt, L.; Gladstone, L.; Glüsenkamp, T.; Goldschmidt, A.; Goodman, J. A.; Góra, D.; Grant, D.; Griesel, T.; Groß, A.; Grullon, S.; Gurtner, M.; Ha, C.; Hajismail, A.; Hallgren, A.; Halzen, F.; Han, K.; Hanson, K.; Heinen, D.; Helbing, K.; Hellauer, R.; Hickford, S.; Hill, G. C.; Hoffman, K. D.; Hoffmann, B.; Homeier, A.; Hoshina, K.; Huelsnitz, W.; Hülß, J. P.; Hulth, P. O.; Hultqvist, K.; Hussain, S.; Ishihara, A.; Jakobi, E.; Jacobsen, J.; Japaridze, G. S.; Johansson, H.; Kampert, K. H.; Kappes, A.; Karg, T.; Karle, A.; Kenny, P.; Kiryluk, J.; Kislat, F.; Klein, S. R.; Köhne, H.; Kohnen, G.; Kolanoski, H.; Köpke, L.; Kopper, S.; Koskinen, D. J.; Kowalski, M.; Kowarik, T.; Krasberg, M.; Kroll, G.; Kurahashi, N.; Kuwabara, T.; Labare, M.; Laihem, K.; Landsman, H.; Larson, M. J.; Lauer, R.; Lünemann, J.; Madsen, J.; Marotta, A.; Maruyama, R.; Mase, K.; Matis, H. S.; Meagher, K.; Merck, M.; Mészáros, P.; Meures, T.; Miarecki, S.; Middell, E.; Milke, N.; Miller, J.; Montaruli, T.; Morse, R.; Movit, S. M.; Nahnhauer, R.; Nam, J. W.; Naumann, U.; Nygren, D. R.; Odrowski, S.; Olivas, A.; Olivo, M.; O'Murchadha, A.; Panknin, S.; Paul, L.; Pérez De Los Heros, C.; Petrovic, J.; Piegsa, A.; Pieloth, D.; Porrata, R.; Posselt, J.; Price, P. B.; Przybylski, G. T.; Rawlins, K.; Redl, P.; Resconi, E.; Rhode, W.; Ribordy, M.; Richard, A. S.; Richman, M.; Rodrigues, J. P.; Rothmaier, F.; Rott, C.; Ruhe, T.; Rutledge, D.; Ruzybayev, B.; Ryckbosch, D.; Sander, H. G.; Santander, M.; Sarkar, S.; Schatto, K.; Schmidt, T.; Schönwald, A.; Schukraft, A.; Schulte, L.; 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.; Stezelberger, T.; Stokstad, R. G.; Stößl, A.; Strahler, E. A.; Ström, R.; Stüer, M.; Sullivan, G. W.; Swillens, Q.; Taavola, H.; Taboada, I.; Tamburro, A.; Tepe, A.; Ter-Antonyan, S.; Tilav, S.; Toale, P. A.; Toscano, S.; Tosi, D.; Van Eijndhoven, N.; Vandenbroucke, J.; Van Overloop, A.; Van Santen, J.; Vehring, M.; Voge, M.; Walck, C.; Waldenmaier, T.; Wallraff, M.; Walter, M.; Weaver, Ch; Wendt, C.; Westerhoff, S.; Whitehorn, N.; Wiebe, K.; Wiebusch, C. H.; Williams, D. R.; Wischnewski, R.; Wissing, H.; Wolf, M.; Wood, T. R.; Woschnagg, K.; Xu, C.; Xu, D. L.; Xu, X. W.; Yanez, J. P.; Yodh, G.; Yoshida, S.; Zarzhitsky, P.; Zoll, M.

    In: Astronomy and Astrophysics, Vol. 535, A109, 25.11.2011.

    Research output: Contribution to journalArticle

    Abbasi, R, Abdou, Y, Abu-Zayyad, T, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Allen, MM, Altmann, D, Andeen, K, Auffenberg, J, Bai, X, Baker, M, Barwick, SW, Baum, V, Bay, R, Bazo Alba, JL, 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, Bindig, D, Bissok, M, Blaufuss, E, Blumenthal, J, Boersma, DJ, Bohm, C, Bose, D, Böser, S, Botner, O, Brown, AM, Buitink, S, Caballero-Mora, KS, Carson, M, Chirkin, D, Christy, B, Clevermann, F, Cohen, S, Colnard, C, Cowen, DF, Cruz Silva, AH, D'Agostino, MV, Danninger, M, Daughhetee, J, Davis, JC, De Clercq, C, Degner, T, Demirörs, L, Descamps, F, Desiati, P, De Vries-Uiterweerd, G, Deyoung, T, Díaz-Vélez, JC, Dierckxsens, M, Dreyer, J, Dumm, JP, Dunkman, M, Eisch, J, Ellsworth, RW, Engdegård, O, Euler, S, Evenson, PA, Fadiran, O, Fazely, AR, Fedynitch, A, Feintzeig, J, Feusels, T, Filimonov, K, Finley, C, Fischer-Wasels, T, Fox, BD, Franckowiak, A, Franke, R, Gaisser, TK, Gallagher, J, Gerhardt, L, Gladstone, L, Glüsenkamp, T, Goldschmidt, A, Goodman, JA, Góra, D, Grant, D, Griesel, T, Groß, A, Grullon, S, Gurtner, M, Ha, C, Hajismail, A, Hallgren, A, Halzen, F, Han, K, Hanson, K, Heinen, D, Helbing, K, Hellauer, R, Hickford, S, Hill, GC, Hoffman, KD, Hoffmann, B, Homeier, A, Hoshina, K, Huelsnitz, W, Hülß, JP, Hulth, PO, Hultqvist, K, Hussain, S, Ishihara, A, Jakobi, E, Jacobsen, J, Japaridze, GS, Johansson, H, Kampert, KH, Kappes, A, Karg, T, Karle, A, Kenny, P, Kiryluk, J, Kislat, F, Klein, SR, Köhne, H, Kohnen, G, Kolanoski, H, Köpke, L, Kopper, S, Koskinen, DJ, Kowalski, M, Kowarik, T, Krasberg, M, Kroll, G, Kurahashi, N, Kuwabara, T, Labare, M, Laihem, K, Landsman, H, Larson, MJ, Lauer, R, Lünemann, J, Madsen, J, Marotta, A, Maruyama, R, Mase, K, Matis, HS, Meagher, K, Merck, M, Mészáros, P, Meures, T, Miarecki, S, Middell, E, Milke, N, Miller, J, Montaruli, T, Morse, R, Movit, SM, Nahnhauer, R, Nam, JW, Naumann, U, Nygren, DR, Odrowski, S, Olivas, A, Olivo, M, O'Murchadha, A, Panknin, S, Paul, L, Pérez De Los Heros, C, Petrovic, J, Piegsa, A, Pieloth, D, Porrata, R, Posselt, J, Price, PB, Przybylski, GT, Rawlins, K, Redl, P, Resconi, E, Rhode, W, Ribordy, M, Richard, AS, Richman, M, Rodrigues, JP, Rothmaier, F, Rott, C, Ruhe, T, Rutledge, D, Ruzybayev, B, Ryckbosch, D, Sander, HG, Santander, M, Sarkar, S, Schatto, K, Schmidt, T, Schönwald, A, Schukraft, A, Schulte, L, 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, Stezelberger, T, Stokstad, RG, Stößl, A, Strahler, EA, Ström, R, Stüer, M, Sullivan, GW, Swillens, Q, Taavola, H, Taboada, I, Tamburro, A, Tepe, A, Ter-Antonyan, S, Tilav, S, Toale, PA, Toscano, S, Tosi, D, Van Eijndhoven, N, Vandenbroucke, J, Van Overloop, A, Van Santen, J, Vehring, M, Voge, M, Walck, C, Waldenmaier, T, Wallraff, M, Walter, M, Weaver, C, Wendt, C, Westerhoff, S, Whitehorn, N, Wiebe, K, Wiebusch, CH, Williams, DR, Wischnewski, R, Wissing, H, Wolf, M, Wood, TR, Woschnagg, K, Xu, C, Xu, DL, Xu, XW, Yanez, JP, Yodh, G, Yoshida, S, Zarzhitsky, P & Zoll, M 2011, 'IceCube sensitivity for low-energy neutrinos from nearby supernovae', Astronomy and Astrophysics, vol. 535, A109. https://doi.org/10.1051/0004-6361/201117810
    Abbasi R, Abdou Y, Abu-Zayyad T, Ackermann M, Adams J, Aguilar JA et al. IceCube sensitivity for low-energy neutrinos from nearby supernovae. Astronomy and Astrophysics. 2011 Nov 25;535. A109. https://doi.org/10.1051/0004-6361/201117810
    Abbasi, R. ; Abdou, Y. ; Abu-Zayyad, T. ; Ackermann, M. ; Adams, J. ; Aguilar, J. A. ; Ahlers, M. ; Allen, M. M. ; Altmann, D. ; Andeen, K. ; Auffenberg, J. ; Bai, X. ; Baker, M. ; Barwick, S. W. ; Baum, V. ; Bay, R. ; Bazo Alba, J. L. ; 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. ; Bindig, D. ; Bissok, M. ; Blaufuss, E. ; Blumenthal, J. ; Boersma, D. J. ; Bohm, C. ; Bose, D. ; Böser, S. ; Botner, O. ; Brown, A. M. ; Buitink, S. ; Caballero-Mora, K. S. ; Carson, M. ; Chirkin, D. ; Christy, B. ; Clevermann, F. ; Cohen, S. ; Colnard, C. ; Cowen, D. F. ; Cruz Silva, A. H. ; D'Agostino, M. V. ; Danninger, M. ; Daughhetee, J. ; Davis, J. C. ; De Clercq, C. ; Degner, T. ; Demirörs, L. ; Descamps, F. ; Desiati, P. ; De Vries-Uiterweerd, G. ; Deyoung, T. ; Díaz-Vélez, J. C. ; Dierckxsens, M. ; Dreyer, J. ; Dumm, J. P. ; Dunkman, M. ; Eisch, J. ; Ellsworth, R. W. ; Engdegård, O. ; Euler, S. ; Evenson, P. A. ; Fadiran, O. ; Fazely, A. R. ; Fedynitch, A. ; Feintzeig, J. ; Feusels, T. ; Filimonov, K. ; Finley, C. ; Fischer-Wasels, T. ; Fox, B. D. ; Franckowiak, A. ; Franke, R. ; Gaisser, T. K. ; Gallagher, J. ; Gerhardt, L. ; Gladstone, L. ; Glüsenkamp, T. ; Goldschmidt, A. ; Goodman, J. A. ; Góra, D. ; Grant, D. ; Griesel, T. ; Groß, A. ; Grullon, S. ; Gurtner, M. ; Ha, C. ; Hajismail, A. ; Hallgren, A. ; Halzen, F. ; Han, K. ; Hanson, K. ; Heinen, D. ; Helbing, K. ; Hellauer, R. ; Hickford, S. ; Hill, G. C. ; Hoffman, K. D. ; Hoffmann, B. ; Homeier, A. ; Hoshina, K. ; Huelsnitz, W. ; Hülß, J. P. ; Hulth, P. O. ; Hultqvist, K. ; Hussain, S. ; Ishihara, A. ; Jakobi, E. ; Jacobsen, J. ; Japaridze, G. S. ; Johansson, H. ; Kampert, K. H. ; Kappes, A. ; Karg, T. ; Karle, A. ; Kenny, P. ; Kiryluk, J. ; Kislat, F. ; Klein, S. R. ; Köhne, H. ; Kohnen, G. ; Kolanoski, H. ; Köpke, L. ; Kopper, S. ; Koskinen, D. J. ; Kowalski, M. ; Kowarik, T. ; Krasberg, M. ; Kroll, G. ; Kurahashi, N. ; Kuwabara, T. ; Labare, M. ; Laihem, K. ; Landsman, H. ; Larson, M. J. ; Lauer, R. ; Lünemann, J. ; Madsen, J. ; Marotta, A. ; Maruyama, R. ; Mase, K. ; Matis, H. S. ; Meagher, K. ; Merck, M. ; Mészáros, P. ; Meures, T. ; Miarecki, S. ; Middell, E. ; Milke, N. ; Miller, J. ; Montaruli, T. ; Morse, R. ; Movit, S. M. ; Nahnhauer, R. ; Nam, J. W. ; Naumann, U. ; Nygren, D. R. ; Odrowski, S. ; Olivas, A. ; Olivo, M. ; O'Murchadha, A. ; Panknin, S. ; Paul, L. ; Pérez De Los Heros, C. ; Petrovic, J. ; Piegsa, A. ; Pieloth, D. ; Porrata, R. ; Posselt, J. ; Price, P. B. ; Przybylski, G. T. ; Rawlins, K. ; Redl, P. ; Resconi, E. ; Rhode, W. ; Ribordy, M. ; Richard, A. S. ; Richman, M. ; Rodrigues, J. P. ; Rothmaier, F. ; Rott, C. ; Ruhe, T. ; Rutledge, D. ; Ruzybayev, B. ; Ryckbosch, D. ; Sander, H. G. ; Santander, M. ; Sarkar, S. ; Schatto, K. ; Schmidt, T. ; Schönwald, A. ; Schukraft, A. ; Schulte, L. ; 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. ; Stezelberger, T. ; Stokstad, R. G. ; Stößl, A. ; Strahler, E. A. ; Ström, R. ; Stüer, M. ; Sullivan, G. W. ; Swillens, Q. ; Taavola, H. ; Taboada, I. ; Tamburro, A. ; Tepe, A. ; Ter-Antonyan, S. ; Tilav, S. ; Toale, P. A. ; Toscano, S. ; Tosi, D. ; Van Eijndhoven, N. ; Vandenbroucke, J. ; Van Overloop, A. ; Van Santen, J. ; Vehring, M. ; Voge, M. ; Walck, C. ; Waldenmaier, T. ; Wallraff, M. ; Walter, M. ; Weaver, Ch ; Wendt, C. ; Westerhoff, S. ; Whitehorn, N. ; Wiebe, K. ; Wiebusch, C. H. ; Williams, D. R. ; Wischnewski, R. ; Wissing, H. ; Wolf, M. ; Wood, T. R. ; Woschnagg, K. ; Xu, C. ; Xu, D. L. ; Xu, X. W. ; Yanez, J. P. ; Yodh, G. ; Yoshida, S. ; Zarzhitsky, P. ; Zoll, M. / IceCube sensitivity for low-energy neutrinos from nearby supernovae. In: Astronomy and Astrophysics. 2011 ; Vol. 535.
    @article{3a2a0e66e022458cab181ec68113aeb8,
    title = "IceCube sensitivity for low-energy neutrinos from nearby supernovae",
    abstract = "This paper describes the response of the IceCube neutrino telescope located at the geographic south pole to outbursts of MeV neutrinos from the core collapse of nearby massive stars. IceCube was completed in December 2010 forming a lattice of 5160 photomultiplier tubes that monitor a volume of ∼1 km 3 in the deep Antarctic ice for particle induced photons. The telescope was designed to detect neutrinos with energies greater than 100 GeV. Owing to subfreezing ice temperatures, the photomultiplier dark noise rates are particularly low. Hence IceCube can also detect large numbers of MeV neutrinos by observing a collective rise in all photomultiplier rates on top of the dark noise. With 2 ms timing resolution, IceCube can detect subtle features in the temporal development of the supernova neutrino burst. For a supernova at the galactic center, its sensitivity matches that of a background-free megaton-scale supernova search experiment. The sensitivity decreases to 20 standard deviations at the galactic edge (30 kpc) and 6 standard deviations at the Large Magellanic Cloud (50 kpc). IceCube is sending triggers from potential supernovae to the Supernova Early Warning System. The sensitivity to neutrino properties such as the neutrino hierarchy is discussed, as well as the possibility to",
    author = "R. Abbasi and Y. Abdou and T. Abu-Zayyad and M. Ackermann and J. Adams and Aguilar, {J. A.} and M. Ahlers and Allen, {M. M.} and D. Altmann and K. Andeen and J. Auffenberg and X. Bai and M. Baker and Barwick, {S. W.} and V. Baum and R. Bay and {Bazo Alba}, {J. L.} 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 D. Bindig and M. Bissok and E. Blaufuss and J. Blumenthal and Boersma, {D. J.} and C. Bohm and D. Bose and S. B{\"o}ser and O. Botner and Brown, {A. M.} and S. Buitink and Caballero-Mora, {K. S.} and M. Carson and D. Chirkin and B. Christy and F. Clevermann and S. Cohen and C. Colnard and Cowen, {D. F.} and {Cruz Silva}, {A. H.} and D'Agostino, {M. V.} and M. Danninger and J. Daughhetee and Davis, {J. C.} and {De Clercq}, C. and T. Degner and L. Demir{\"o}rs and F. Descamps and P. Desiati and {De Vries-Uiterweerd}, G. and T. Deyoung and D{\'i}az-V{\'e}lez, {J. C.} and M. Dierckxsens and J. Dreyer and Dumm, {J. P.} and M. Dunkman and J. Eisch and Ellsworth, {R. W.} and O. Engdeg{\aa}rd and S. Euler and Evenson, {P. A.} and O. Fadiran and Fazely, {A. R.} and A. Fedynitch and J. Feintzeig and T. Feusels and K. Filimonov and C. Finley and T. Fischer-Wasels and Fox, {B. D.} and A. Franckowiak and R. Franke and Gaisser, {T. K.} and J. Gallagher and L. Gerhardt and L. Gladstone and T. Gl{\"u}senkamp and A. Goldschmidt and Goodman, {J. A.} and D. G{\'o}ra and D. Grant and T. Griesel and A. Gro{\ss} and S. Grullon and M. Gurtner and C. Ha and A. Hajismail and A. Hallgren and F. Halzen and K. Han and K. Hanson and D. Heinen and K. Helbing and R. Hellauer and S. Hickford and Hill, {G. C.} and Hoffman, {K. D.} and B. Hoffmann and A. Homeier and K. Hoshina and W. Huelsnitz and H{\"u}l{\ss}, {J. P.} and Hulth, {P. O.} and K. Hultqvist and S. Hussain and A. Ishihara and E. Jakobi and J. Jacobsen and Japaridze, {G. S.} and H. Johansson and Kampert, {K. H.} and A. Kappes and T. Karg and A. Karle and P. Kenny and J. Kiryluk and F. Kislat and Klein, {S. R.} and H. K{\"o}hne and G. Kohnen and H. Kolanoski and L. K{\"o}pke and S. Kopper and Koskinen, {D. J.} and M. Kowalski and T. Kowarik and M. Krasberg and G. Kroll and N. Kurahashi and T. Kuwabara and M. Labare and K. Laihem and H. Landsman and Larson, {M. J.} and R. Lauer and J. L{\"u}nemann and J. Madsen and A. Marotta and R. Maruyama and K. Mase and Matis, {H. S.} and K. Meagher and M. Merck and P. M{\'e}sz{\'a}ros and T. Meures and S. Miarecki 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 Nygren, {D. R.} and S. Odrowski and A. Olivas and M. Olivo and A. O'Murchadha and S. Panknin and L. Paul and {P{\'e}rez De Los Heros}, C. and J. Petrovic and A. Piegsa and D. Pieloth and R. Porrata and J. Posselt and Price, {P. B.} and Przybylski, {G. T.} and K. Rawlins and P. Redl and E. Resconi and W. Rhode and M. Ribordy and Richard, {A. S.} and M. Richman and Rodrigues, {J. P.} 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 T. Schmidt and A. Sch{\"o}nwald and A. Schukraft and L. Schulte 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 T. Stezelberger and Stokstad, {R. G.} and A. St{\"o}{\ss}l and Strahler, {E. A.} and R. Str{\"o}m and M. St{\"u}er and Sullivan, {G. W.} and Q. Swillens and H. Taavola and I. Taboada and A. Tamburro and A. Tepe and S. Ter-Antonyan and S. Tilav and Toale, {P. A.} and S. Toscano and D. Tosi and {Van Eijndhoven}, N. and J. Vandenbroucke and {Van Overloop}, A. and {Van Santen}, J. and M. Vehring and M. Voge and C. Walck and T. Waldenmaier and M. Wallraff and M. Walter and Ch Weaver and C. Wendt and S. Westerhoff and N. Whitehorn and K. Wiebe and Wiebusch, {C. H.} and Williams, {D. R.} and R. Wischnewski and H. Wissing and M. Wolf and Wood, {T. R.} and K. Woschnagg and C. Xu and Xu, {D. L.} and Xu, {X. W.} and Yanez, {J. P.} and G. Yodh and S. Yoshida and P. Zarzhitsky and M. Zoll",
    year = "2011",
    month = "11",
    day = "25",
    doi = "10.1051/0004-6361/201117810",
    language = "English (US)",
    volume = "535",
    journal = "Astronomy and Astrophysics",
    issn = "0004-6361",
    publisher = "EDP Sciences",

    }

    TY - JOUR

    T1 - IceCube sensitivity for low-energy neutrinos from nearby supernovae

    AU - Abbasi, R.

    AU - Abdou, Y.

    AU - Abu-Zayyad, T.

    AU - Ackermann, M.

    AU - Adams, J.

    AU - Aguilar, J. A.

    AU - Ahlers, M.

    AU - Allen, M. M.

    AU - Altmann, D.

    AU - Andeen, K.

    AU - Auffenberg, J.

    AU - Bai, X.

    AU - Baker, M.

    AU - Barwick, S. W.

    AU - Baum, V.

    AU - Bay, R.

    AU - Bazo Alba, J. L.

    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 - Bindig, D.

    AU - Bissok, M.

    AU - Blaufuss, E.

    AU - Blumenthal, J.

    AU - Boersma, D. J.

    AU - Bohm, C.

    AU - Bose, D.

    AU - Böser, S.

    AU - Botner, O.

    AU - Brown, A. M.

    AU - Buitink, S.

    AU - Caballero-Mora, K. S.

    AU - Carson, M.

    AU - Chirkin, D.

    AU - Christy, B.

    AU - Clevermann, F.

    AU - Cohen, S.

    AU - Colnard, C.

    AU - Cowen, D. F.

    AU - Cruz Silva, A. H.

    AU - D'Agostino, M. V.

    AU - Danninger, M.

    AU - Daughhetee, J.

    AU - Davis, J. C.

    AU - De Clercq, C.

    AU - Degner, T.

    AU - Demirörs, L.

    AU - Descamps, F.

    AU - Desiati, P.

    AU - De Vries-Uiterweerd, G.

    AU - Deyoung, T.

    AU - Díaz-Vélez, J. C.

    AU - Dierckxsens, M.

    AU - Dreyer, J.

    AU - Dumm, J. P.

    AU - Dunkman, M.

    AU - Eisch, J.

    AU - Ellsworth, R. W.

    AU - Engdegård, O.

    AU - Euler, S.

    AU - Evenson, P. A.

    AU - Fadiran, O.

    AU - Fazely, A. R.

    AU - Fedynitch, A.

    AU - Feintzeig, J.

    AU - Feusels, T.

    AU - Filimonov, K.

    AU - Finley, C.

    AU - Fischer-Wasels, T.

    AU - Fox, B. D.

    AU - Franckowiak, A.

    AU - Franke, R.

    AU - Gaisser, T. K.

    AU - Gallagher, J.

    AU - Gerhardt, L.

    AU - Gladstone, L.

    AU - Glüsenkamp, T.

    AU - Goldschmidt, A.

    AU - Goodman, J. A.

    AU - Góra, D.

    AU - Grant, D.

    AU - Griesel, T.

    AU - Groß, A.

    AU - Grullon, S.

    AU - Gurtner, M.

    AU - Ha, C.

    AU - Hajismail, A.

    AU - Hallgren, A.

    AU - Halzen, F.

    AU - Han, K.

    AU - Hanson, K.

    AU - Heinen, D.

    AU - Helbing, K.

    AU - Hellauer, R.

    AU - Hickford, S.

    AU - Hill, G. C.

    AU - Hoffman, K. D.

    AU - Hoffmann, B.

    AU - Homeier, A.

    AU - Hoshina, K.

    AU - Huelsnitz, W.

    AU - Hülß, J. P.

    AU - Hulth, P. O.

    AU - Hultqvist, K.

    AU - Hussain, S.

    AU - Ishihara, A.

    AU - Jakobi, E.

    AU - Jacobsen, J.

    AU - Japaridze, G. S.

    AU - Johansson, H.

    AU - Kampert, K. H.

    AU - Kappes, A.

    AU - Karg, T.

    AU - Karle, A.

    AU - Kenny, P.

    AU - Kiryluk, J.

    AU - Kislat, F.

    AU - Klein, S. R.

    AU - Köhne, H.

    AU - Kohnen, G.

    AU - Kolanoski, H.

    AU - Köpke, L.

    AU - Kopper, S.

    AU - Koskinen, D. J.

    AU - Kowalski, M.

    AU - Kowarik, T.

    AU - Krasberg, M.

    AU - Kroll, G.

    AU - Kurahashi, N.

    AU - Kuwabara, T.

    AU - Labare, M.

    AU - Laihem, K.

    AU - Landsman, H.

    AU - Larson, M. J.

    AU - Lauer, R.

    AU - Lünemann, J.

    AU - Madsen, J.

    AU - Marotta, A.

    AU - Maruyama, R.

    AU - Mase, K.

    AU - Matis, H. S.

    AU - Meagher, K.

    AU - Merck, M.

    AU - Mészáros, P.

    AU - Meures, T.

    AU - Miarecki, S.

    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 - Nygren, D. R.

    AU - Odrowski, S.

    AU - Olivas, A.

    AU - Olivo, M.

    AU - O'Murchadha, A.

    AU - Panknin, S.

    AU - Paul, L.

    AU - Pérez De Los Heros, C.

    AU - Petrovic, J.

    AU - Piegsa, A.

    AU - Pieloth, D.

    AU - Porrata, R.

    AU - Posselt, J.

    AU - Price, P. B.

    AU - Przybylski, G. T.

    AU - Rawlins, K.

    AU - Redl, P.

    AU - Resconi, E.

    AU - Rhode, W.

    AU - Ribordy, M.

    AU - Richard, A. S.

    AU - Richman, M.

    AU - Rodrigues, J. 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 - Schmidt, T.

    AU - Schönwald, A.

    AU - Schukraft, A.

    AU - Schulte, L.

    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 - Stezelberger, T.

    AU - Stokstad, R. G.

    AU - Stößl, A.

    AU - Strahler, E. A.

    AU - Ström, R.

    AU - Stüer, M.

    AU - Sullivan, G. W.

    AU - Swillens, Q.

    AU - Taavola, H.

    AU - Taboada, I.

    AU - Tamburro, A.

    AU - Tepe, A.

    AU - Ter-Antonyan, S.

    AU - Tilav, S.

    AU - Toale, P. A.

    AU - Toscano, S.

    AU - Tosi, D.

    AU - Van Eijndhoven, N.

    AU - Vandenbroucke, J.

    AU - Van Overloop, A.

    AU - Van Santen, J.

    AU - Vehring, M.

    AU - Voge, M.

    AU - Walck, C.

    AU - Waldenmaier, T.

    AU - Wallraff, M.

    AU - Walter, M.

    AU - Weaver, Ch

    AU - Wendt, C.

    AU - Westerhoff, S.

    AU - Whitehorn, N.

    AU - Wiebe, K.

    AU - Wiebusch, C. H.

    AU - Williams, D. R.

    AU - Wischnewski, R.

    AU - Wissing, H.

    AU - Wolf, M.

    AU - Wood, T. R.

    AU - Woschnagg, K.

    AU - Xu, C.

    AU - Xu, D. L.

    AU - Xu, X. W.

    AU - Yanez, J. P.

    AU - Yodh, G.

    AU - Yoshida, S.

    AU - Zarzhitsky, P.

    AU - Zoll, M.

    PY - 2011/11/25

    Y1 - 2011/11/25

    N2 - This paper describes the response of the IceCube neutrino telescope located at the geographic south pole to outbursts of MeV neutrinos from the core collapse of nearby massive stars. IceCube was completed in December 2010 forming a lattice of 5160 photomultiplier tubes that monitor a volume of ∼1 km 3 in the deep Antarctic ice for particle induced photons. The telescope was designed to detect neutrinos with energies greater than 100 GeV. Owing to subfreezing ice temperatures, the photomultiplier dark noise rates are particularly low. Hence IceCube can also detect large numbers of MeV neutrinos by observing a collective rise in all photomultiplier rates on top of the dark noise. With 2 ms timing resolution, IceCube can detect subtle features in the temporal development of the supernova neutrino burst. For a supernova at the galactic center, its sensitivity matches that of a background-free megaton-scale supernova search experiment. The sensitivity decreases to 20 standard deviations at the galactic edge (30 kpc) and 6 standard deviations at the Large Magellanic Cloud (50 kpc). IceCube is sending triggers from potential supernovae to the Supernova Early Warning System. The sensitivity to neutrino properties such as the neutrino hierarchy is discussed, as well as the possibility to

    AB - This paper describes the response of the IceCube neutrino telescope located at the geographic south pole to outbursts of MeV neutrinos from the core collapse of nearby massive stars. IceCube was completed in December 2010 forming a lattice of 5160 photomultiplier tubes that monitor a volume of ∼1 km 3 in the deep Antarctic ice for particle induced photons. The telescope was designed to detect neutrinos with energies greater than 100 GeV. Owing to subfreezing ice temperatures, the photomultiplier dark noise rates are particularly low. Hence IceCube can also detect large numbers of MeV neutrinos by observing a collective rise in all photomultiplier rates on top of the dark noise. With 2 ms timing resolution, IceCube can detect subtle features in the temporal development of the supernova neutrino burst. For a supernova at the galactic center, its sensitivity matches that of a background-free megaton-scale supernova search experiment. The sensitivity decreases to 20 standard deviations at the galactic edge (30 kpc) and 6 standard deviations at the Large Magellanic Cloud (50 kpc). IceCube is sending triggers from potential supernovae to the Supernova Early Warning System. The sensitivity to neutrino properties such as the neutrino hierarchy is discussed, as well as the possibility to

    UR - http://www.scopus.com/inward/record.url?scp=81755166566&partnerID=8YFLogxK

    UR - http://www.scopus.com/inward/citedby.url?scp=81755166566&partnerID=8YFLogxK

    U2 - 10.1051/0004-6361/201117810

    DO - 10.1051/0004-6361/201117810

    M3 - Article

    VL - 535

    JO - Astronomy and Astrophysics

    JF - Astronomy and Astrophysics

    SN - 0004-6361

    M1 - A109

    ER -