Search for steady point-like sources in the astrophysical muon neutrino flux with 8 years of IceCube data

Abstract The IceCube Collaboration has observed a high-energy astrophysical neutrino flux and recently found evidence for neutrino emission from the blazar TXS 0506 $$+$$...

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Main Authors:	Aartsen, M. G, Ackermann, M., Adams, J., Aguilar, J. A, Ahlers, M., Ahrens, M., Altmann, D., Andeen, K., Anderson, T., Ansseau, I., Anton, G., Argüelles, C., Auffenberg, J., Axani, S., Backes, P., Bagherpour, H., Bai, X., Barbano, A., Barron, J. P, Barwick, S. W, Baum, V., Bay, R., Beatty, J. J, Becker Tjus, J., Becker, K.-H., BenZvi, S., Berley, D., Bernardini, E., Besson, D. Z, Binder, G., Bindig, D., Blaufuss, E., Blot, S., Bohm, C., Börner, M., Bos, F., Böser, S., Botner, O., Bourbeau, E., Bourbeau, J., Bradascio, F., Braun, J., Bretz, H.-P., Bron, S., Brostean-Kaiser, J., Burgman, A., Busse, R. S, Carver, T., Chen, C., Cheung, E., Chirkin, D., Clark, K., Classen, L., Collin, G. H, Conrad, J. M, Coppin, P., Correa, P., Cowen, D. F, Cross, R., Dave, P., Day, M., de André, J. P A M, De Clercq, C., DeLaunay, J. J, Dembinski, H., Deoskar, K., De Ridder, S., Desiati, P., de Vries, K. D, de Wasseige, G., de With, M., DeYoung, T., Díaz-Vélez, J. C, Dujmovic, H., Dunkman, M., Dvorak, E., Eberhardt, B., Ehrhardt, T., Eichmann, B., Eller, P., Evenson, P. A, Fahey, S., Fazely, A. R, Felde, J., Filimonov, K., Finley, C., Franckowiak, A., Friedman, E., Fritz, A., Gaisser, T. K, Gallagher, J., Ganster, E., Garrappa, S., Gerhardt, L., Ghorbani, K., Giang, W., Glauch, T., Glüsenkamp, T., Goldschmidt, A., Gonzalez, J. G, Grant, D., Griffith, Z., Haack, C., Hallgren, A., Halve, L., Halzen, F., Hanson, K., Hebecker, D., Heereman, D., Helbing, K., Hellauer, R., Hickford, S., Hignight, J., Hill, G. C, Hoffman, K. D, Hoffmann, R., Hoinka, T., Hokanson-Fasig, B., Hoshina, K., Huang, F., Huber, M., Hultqvist, K., Hünnefeld, M., Hussain, R., In, S., Iovine, N., Ishihara, A., Jacobi, E., Japaridze, G. S, Jeong, M., Jero, K., Jones, B. J P, Kalaczynski, P., Kang, W., Kappes, A., Kappesser, D., Karg, T., Karle, A., Katz, U., Kauer, M., Keivani, A., Kelley, J. L, Kheirandish, A., Kim, J., Kintscher, T., Kiryluk, J., Kittler, T., Klein, S. R, Koirala, R., Kolanoski, H., Köpke, L., Kopper, C., Kopper, S., Koskinen, D. J, Kowalski, M., Krings, K., Kroll, M., Krückl, G., Kunwar, S., Kurahashi, N., Kyriacou, A., Labare, M., Lanfranchi, J. L, Larson, M. J, Lauber, F., Leonard, K., Leuermann, M., Liu, Q. R, Lohfink, E., Mariscal, C. J L, Lu, L., Lünemann, J., Luszczak, W., Madsen, J., Maggi, G., Mahn, K. B M, Makino, Y., Mancina, S., Mariş, I. C, Maruyama, R., Mase, K., Maunu, R., Meagher, K., Medici, M., Meier, M., Menne, T., Merino, G., Meures, T., Miarecki, S., Micallef, J., Momenté, G., Montaruli, T., Moore, R. W, Moulai, M., Nagai, R., Nahnhauer, R., Nakarmi, P., Naumann, U., Neer, G., Niederhausen, H., Nowicki, S. C, Nygren, D. R, Obertacke Pollmann, A., Olivas, A., O’Murchadha, A., O’Sullivan, E., Palczewski, T., Pandya, H., Pankova, D. V, Peiffer, P., Pérez de los Heros, C., Pieloth, D., Pinat, E., Pizzuto, A., Plum, M., Price, P. B, Przybylski, G. T, Raab, C., Rameez, M., Rauch, L., Rawlins, K., Rea, I. C, Reimann, R., Relethford, B., Renzi, G., Resconi, E., Rhode, W., Richman, M., Robertson, S., Rongen, M., Rott, C., Ruhe, T., Ryckbosch, D., Rysewyk, D., Safa, I., Sanchez Herrera, S. E, Sandrock, A., Sandroos, J., Santander, M., Sarkar, S., Satalecka, K., Schaufel, M., Schlunder, P., Schmidt, T., Schneider, A., Schneider, J., Schöneberg, S., Schumacher, L., Sclafani, S., Seckel, D., Seunarine, S., Soedingrekso, J., Soldin, D., Song, M., Spiczak, G. M, Spiering, C., Stachurska, J., Stamatikos, M., Stanev, T., Stasik, A., Stein, R., Stettner, J., Steuer, A., Stezelberger, T., Stokstad, R. G, Stößl, A., Strotjohann, N. L, Stuttard, T., Sullivan, G. W, Sutherland, M., Taboada, I., Tenholt, F., Ter-Antonyan, S., Terliuk, A., Tilav, S., Tobin, M. N, Tönnis, C., Toscano, S., Tosi, D., Tselengidou, M., Tung, C. F, Turcati, A., Turcotte, R., Turley, C. F, Ty, B., Unger, E., Unland Elorrieta, M. A, Usner, M., Vandenbroucke, J., Van Driessche, W., van Eijk, D., van Eijndhoven, N., Vanheule, S., van Santen, J., Vraeghe, M., Walck, C., Wallace, A., Wallraff, M., Wandler, F. D, Wandkowsky, N., Watson, T. B, Weaver, C., Weiss, M. J, Wendt, C., Werthebach, J., Westerhoff, S., Whelan, B. J, Whitehorn, N., Wiebe, K., Wiebusch, C. H, Wille, L., Williams, D. R, Wills, L., Wolf, M., Wood, J., Wood, T. R, Woolsey, E., Woschnagg, K., Wrede, G., Xu, D. L, Xu, X. W, Xu, Y., Yanez, J. P, Yodh, G., Yoshida, S., Yuan, T.
Other Authors:	Massachusetts Institute of Technology. Department of Physics
Format:	Article
Language:	English
Published:	Springer Berlin Heidelberg 2021
Online Access:	https://hdl.handle.net/1721.1/131276

_version_	1826197698215149568
author	Aartsen, M. G Ackermann, M. Adams, J. Aguilar, J. A Ahlers, M. Ahrens, M. Altmann, D. Andeen, K. Anderson, T. Ansseau, I. Anton, G. Argüelles, C. Auffenberg, J. Axani, S. Backes, P. Bagherpour, H. Bai, X. Barbano, A. Barron, J. P Barwick, S. W Baum, V. Bay, R. Beatty, J. J Becker Tjus, J. Becker, K.-H. BenZvi, S. Berley, D. Bernardini, E. Besson, D. Z Binder, G. Bindig, D. Blaufuss, E. Blot, S. Bohm, C. Börner, M. Bos, F. Böser, S. Botner, O. Bourbeau, E. Bourbeau, J. Bradascio, F. Braun, J. Bretz, H.-P. Bron, S. Brostean-Kaiser, J. Burgman, A. Busse, R. S Carver, T. Chen, C. Cheung, E. Chirkin, D. Clark, K. Classen, L. Collin, G. H Conrad, J. M Coppin, P. Correa, P. Cowen, D. F Cross, R. Dave, P. Day, M. de André, J. P A M De Clercq, C. DeLaunay, J. J Dembinski, H. Deoskar, K. De Ridder, S. Desiati, P. de Vries, K. D de Wasseige, G. de With, M. DeYoung, T. Díaz-Vélez, J. C Dujmovic, H. Dunkman, M. Dvorak, E. Eberhardt, B. Ehrhardt, T. Eichmann, B. Eller, P. Evenson, P. A Fahey, S. Fazely, A. R Felde, J. Filimonov, K. Finley, C. Franckowiak, A. Friedman, E. Fritz, A. Gaisser, T. K Gallagher, J. Ganster, E. Garrappa, S. Gerhardt, L. Ghorbani, K. Giang, W. Glauch, T. Glüsenkamp, T. Goldschmidt, A. Gonzalez, J. G Grant, D. Griffith, Z. Haack, C. Hallgren, A. Halve, L. Halzen, F. Hanson, K. Hebecker, D. Heereman, D. Helbing, K. Hellauer, R. Hickford, S. Hignight, J. Hill, G. C Hoffman, K. D Hoffmann, R. Hoinka, T. Hokanson-Fasig, B. Hoshina, K. Huang, F. Huber, M. Hultqvist, K. Hünnefeld, M. Hussain, R. In, S. Iovine, N. Ishihara, A. Jacobi, E. Japaridze, G. S Jeong, M. Jero, K. Jones, B. J P Kalaczynski, P. Kang, W. Kappes, A. Kappesser, D. Karg, T. Karle, A. Katz, U. Kauer, M. Keivani, A. Kelley, J. L Kheirandish, A. Kim, J. Kintscher, T. Kiryluk, J. Kittler, T. Klein, S. R Koirala, R. Kolanoski, H. Köpke, L. Kopper, C. Kopper, S. Koskinen, D. J Kowalski, M. Krings, K. Kroll, M. Krückl, G. Kunwar, S. Kurahashi, N. Kyriacou, A. Labare, M. Lanfranchi, J. L Larson, M. J Lauber, F. Leonard, K. Leuermann, M. Liu, Q. R Lohfink, E. Mariscal, C. J L Lu, L. Lünemann, J. Luszczak, W. Madsen, J. Maggi, G. Mahn, K. B M Makino, Y. Mancina, S. Mariş, I. C Maruyama, R. Mase, K. Maunu, R. Meagher, K. Medici, M. Meier, M. Menne, T. Merino, G. Meures, T. Miarecki, S. Micallef, J. Momenté, G. Montaruli, T. Moore, R. W Moulai, M. Nagai, R. Nahnhauer, R. Nakarmi, P. Naumann, U. Neer, G. Niederhausen, H. Nowicki, S. C Nygren, D. R Obertacke Pollmann, A. Olivas, A. O’Murchadha, A. O’Sullivan, E. Palczewski, T. Pandya, H. Pankova, D. V Peiffer, P. Pérez de los Heros, C. Pieloth, D. Pinat, E. Pizzuto, A. Plum, M. Price, P. B Przybylski, G. T Raab, C. Rameez, M. Rauch, L. Rawlins, K. Rea, I. C Reimann, R. Relethford, B. Renzi, G. Resconi, E. Rhode, W. Richman, M. Robertson, S. Rongen, M. Rott, C. Ruhe, T. Ryckbosch, D. Rysewyk, D. Safa, I. Sanchez Herrera, S. E Sandrock, A. Sandroos, J. Santander, M. Sarkar, S. Sarkar, S. Satalecka, K. Schaufel, M. Schlunder, P. Schmidt, T. Schneider, A. Schneider, J. Schöneberg, S. Schumacher, L. Sclafani, S. Seckel, D. Seunarine, S. Soedingrekso, J. Soldin, D. Song, M. Spiczak, G. M Spiering, C. Stachurska, J. Stamatikos, M. Stanev, T. Stasik, A. Stein, R. Stettner, J. Steuer, A. Stezelberger, T. Stokstad, R. G Stößl, A. Strotjohann, N. L Stuttard, T. Sullivan, G. W Sutherland, M. Taboada, I. Tenholt, F. Ter-Antonyan, S. Terliuk, A. Tilav, S. Tobin, M. N Tönnis, C. Toscano, S. Tosi, D. Tselengidou, M. Tung, C. F Turcati, A. Turcotte, R. Turley, C. F Ty, B. Unger, E. Unland Elorrieta, M. A Usner, M. Vandenbroucke, J. Van Driessche, W. van Eijk, D. van Eijndhoven, N. Vanheule, S. van Santen, J. Vraeghe, M. Walck, C. Wallace, A. Wallraff, M. Wandler, F. D Wandkowsky, N. Watson, T. B Weaver, C. Weiss, M. J Wendt, C. Werthebach, J. Westerhoff, S. Whelan, B. J Whitehorn, N. Wiebe, K. Wiebusch, C. H Wille, L. Williams, D. R Wills, L. Wolf, M. Wood, J. Wood, T. R Woolsey, E. Woschnagg, K. Wrede, G. Xu, D. L Xu, X. W Xu, Y. Yanez, J. P Yodh, G. Yoshida, S. Yuan, T.
author2	Massachusetts Institute of Technology. Department of Physics
author_facet	Massachusetts Institute of Technology. Department of Physics Aartsen, M. G Ackermann, M. Adams, J. Aguilar, J. A Ahlers, M. Ahrens, M. Altmann, D. Andeen, K. Anderson, T. Ansseau, I. Anton, G. Argüelles, C. Auffenberg, J. Axani, S. Backes, P. Bagherpour, H. Bai, X. Barbano, A. Barron, J. P Barwick, S. W Baum, V. Bay, R. Beatty, J. J Becker Tjus, J. Becker, K.-H. BenZvi, S. Berley, D. Bernardini, E. Besson, D. Z Binder, G. Bindig, D. Blaufuss, E. Blot, S. Bohm, C. Börner, M. Bos, F. Böser, S. Botner, O. Bourbeau, E. Bourbeau, J. Bradascio, F. Braun, J. Bretz, H.-P. Bron, S. Brostean-Kaiser, J. Burgman, A. Busse, R. S Carver, T. Chen, C. Cheung, E. Chirkin, D. Clark, K. Classen, L. Collin, G. H Conrad, J. M Coppin, P. Correa, P. Cowen, D. F Cross, R. Dave, P. Day, M. de André, J. P A M De Clercq, C. DeLaunay, J. J Dembinski, H. Deoskar, K. De Ridder, S. Desiati, P. de Vries, K. D de Wasseige, G. de With, M. DeYoung, T. Díaz-Vélez, J. C Dujmovic, H. Dunkman, M. Dvorak, E. Eberhardt, B. Ehrhardt, T. Eichmann, B. Eller, P. Evenson, P. A Fahey, S. Fazely, A. R Felde, J. Filimonov, K. Finley, C. Franckowiak, A. Friedman, E. Fritz, A. Gaisser, T. K Gallagher, J. Ganster, E. Garrappa, S. Gerhardt, L. Ghorbani, K. Giang, W. Glauch, T. Glüsenkamp, T. Goldschmidt, A. Gonzalez, J. G Grant, D. Griffith, Z. Haack, C. Hallgren, A. Halve, L. Halzen, F. Hanson, K. Hebecker, D. Heereman, D. Helbing, K. Hellauer, R. Hickford, S. Hignight, J. Hill, G. C Hoffman, K. D Hoffmann, R. Hoinka, T. Hokanson-Fasig, B. Hoshina, K. Huang, F. Huber, M. Hultqvist, K. Hünnefeld, M. Hussain, R. In, S. Iovine, N. Ishihara, A. Jacobi, E. Japaridze, G. S Jeong, M. Jero, K. Jones, B. J P Kalaczynski, P. Kang, W. Kappes, A. Kappesser, D. Karg, T. Karle, A. Katz, U. Kauer, M. Keivani, A. Kelley, J. L Kheirandish, A. Kim, J. Kintscher, T. Kiryluk, J. Kittler, T. Klein, S. R Koirala, R. Kolanoski, H. Köpke, L. Kopper, C. Kopper, S. Koskinen, D. J Kowalski, M. Krings, K. Kroll, M. Krückl, G. Kunwar, S. Kurahashi, N. Kyriacou, A. Labare, M. Lanfranchi, J. L Larson, M. J Lauber, F. Leonard, K. Leuermann, M. Liu, Q. R Lohfink, E. Mariscal, C. J L Lu, L. Lünemann, J. Luszczak, W. Madsen, J. Maggi, G. Mahn, K. B M Makino, Y. Mancina, S. Mariş, I. C Maruyama, R. Mase, K. Maunu, R. Meagher, K. Medici, M. Meier, M. Menne, T. Merino, G. Meures, T. Miarecki, S. Micallef, J. Momenté, G. Montaruli, T. Moore, R. W Moulai, M. Nagai, R. Nahnhauer, R. Nakarmi, P. Naumann, U. Neer, G. Niederhausen, H. Nowicki, S. C Nygren, D. R Obertacke Pollmann, A. Olivas, A. O’Murchadha, A. O’Sullivan, E. Palczewski, T. Pandya, H. Pankova, D. V Peiffer, P. Pérez de los Heros, C. Pieloth, D. Pinat, E. Pizzuto, A. Plum, M. Price, P. B Przybylski, G. T Raab, C. Rameez, M. Rauch, L. Rawlins, K. Rea, I. C Reimann, R. Relethford, B. Renzi, G. Resconi, E. Rhode, W. Richman, M. Robertson, S. Rongen, M. Rott, C. Ruhe, T. Ryckbosch, D. Rysewyk, D. Safa, I. Sanchez Herrera, S. E Sandrock, A. Sandroos, J. Santander, M. Sarkar, S. Sarkar, S. Satalecka, K. Schaufel, M. Schlunder, P. Schmidt, T. Schneider, A. Schneider, J. Schöneberg, S. Schumacher, L. Sclafani, S. Seckel, D. Seunarine, S. Soedingrekso, J. Soldin, D. Song, M. Spiczak, G. M Spiering, C. Stachurska, J. Stamatikos, M. Stanev, T. Stasik, A. Stein, R. Stettner, J. Steuer, A. Stezelberger, T. Stokstad, R. G Stößl, A. Strotjohann, N. L Stuttard, T. Sullivan, G. W Sutherland, M. Taboada, I. Tenholt, F. Ter-Antonyan, S. Terliuk, A. Tilav, S. Tobin, M. N Tönnis, C. Toscano, S. Tosi, D. Tselengidou, M. Tung, C. F Turcati, A. Turcotte, R. Turley, C. F Ty, B. Unger, E. Unland Elorrieta, M. A Usner, M. Vandenbroucke, J. Van Driessche, W. van Eijk, D. van Eijndhoven, N. Vanheule, S. van Santen, J. Vraeghe, M. Walck, C. Wallace, A. Wallraff, M. Wandler, F. D Wandkowsky, N. Watson, T. B Weaver, C. Weiss, M. J Wendt, C. Werthebach, J. Westerhoff, S. Whelan, B. J Whitehorn, N. Wiebe, K. Wiebusch, C. H Wille, L. Williams, D. R Wills, L. Wolf, M. Wood, J. Wood, T. R Woolsey, E. Woschnagg, K. Wrede, G. Xu, D. L Xu, X. W Xu, Y. Yanez, J. P Yodh, G. Yoshida, S. Yuan, T.
author_sort	Aartsen, M. G
collection	MIT
description	Abstract The IceCube Collaboration has observed a high-energy astrophysical neutrino flux and recently found evidence for neutrino emission from the blazar TXS 0506 $$+$$ + 056. These results open a new window into the high-energy universe. However, the source or sources of most of the observed flux of astrophysical neutrinos remains uncertain. Here, a search for steady point-like neutrino sources is performed using an unbinned likelihood analysis. The method searches for a spatial accumulation of muon-neutrino events using the very high-statistics sample of about 497,000 neutrinos recorded by IceCube between 2009 and 2017. The median angular resolution is $$\sim 1^\circ $$ ∼ 1 ∘ at 1 TeV and improves to $$\sim 0.3^\circ $$ ∼ 0 . 3 ∘ for neutrinos with an energy of 1 PeV. Compared to previous analyses, this search is optimized for point-like neutrino emission with the same flux-characteristics as the observed astrophysical muon-neutrino flux and introduces an improved event-reconstruction and parametrization of the background. The result is an improvement in sensitivity to the muon-neutrino flux compared to the previous analysis of $$\sim 35\%$$ ∼ 35 % assuming an $$E^{-2}$$ E - 2 spectrum. The sensitivity on the muon-neutrino flux is at a level of $$E^2 \mathrm {d} N /\mathrm {d} E = 3\cdot 10^{-13}\,\mathrm {TeV}\,\mathrm {cm}^{-2}\,\mathrm {s}^{-1}$$ E 2 d N / d E = 3 · 10 - 13 TeV cm - 2 s - 1 . No new evidence for neutrino sources is found in a full sky scan and in an a priori candidate source list that is motivated by gamma-ray observations. Furthermore, no significant excesses above background are found from populations of sub-threshold sources. The implications of the non-observation for potential source classes are discussed.
first_indexed	2024-09-23T10:51:46Z
format	Article
id	mit-1721.1/131276
institution	Massachusetts Institute of Technology
language	English
last_indexed	2024-09-23T10:51:46Z
publishDate	2021
publisher	Springer Berlin Heidelberg
record_format	dspace
spelling	mit-1721.1/1312762024-01-03T18:38:07Z Search for steady point-like sources in the astrophysical muon neutrino flux with 8 years of IceCube data Aartsen, M. G Ackermann, M. Adams, J. Aguilar, J. A Ahlers, M. Ahrens, M. Altmann, D. Andeen, K. Anderson, T. Ansseau, I. Anton, G. Argüelles, C. Auffenberg, J. Axani, S. Backes, P. Bagherpour, H. Bai, X. Barbano, A. Barron, J. P Barwick, S. W Baum, V. Bay, R. Beatty, J. J Becker Tjus, J. Becker, K.-H. BenZvi, S. Berley, D. Bernardini, E. Besson, D. Z Binder, G. Bindig, D. Blaufuss, E. Blot, S. Bohm, C. Börner, M. Bos, F. Böser, S. Botner, O. Bourbeau, E. Bourbeau, J. Bradascio, F. Braun, J. Bretz, H.-P. Bron, S. Brostean-Kaiser, J. Burgman, A. Busse, R. S Carver, T. Chen, C. Cheung, E. Chirkin, D. Clark, K. Classen, L. Collin, G. H Conrad, J. M Coppin, P. Correa, P. Cowen, D. F Cross, R. Dave, P. Day, M. de André, J. P A M De Clercq, C. DeLaunay, J. J Dembinski, H. Deoskar, K. De Ridder, S. Desiati, P. de Vries, K. D de Wasseige, G. de With, M. DeYoung, T. Díaz-Vélez, J. C Dujmovic, H. Dunkman, M. Dvorak, E. Eberhardt, B. Ehrhardt, T. Eichmann, B. Eller, P. Evenson, P. A Fahey, S. Fazely, A. R Felde, J. Filimonov, K. Finley, C. Franckowiak, A. Friedman, E. Fritz, A. Gaisser, T. K Gallagher, J. Ganster, E. Garrappa, S. Gerhardt, L. Ghorbani, K. Giang, W. Glauch, T. Glüsenkamp, T. Goldschmidt, A. Gonzalez, J. G Grant, D. Griffith, Z. Haack, C. Hallgren, A. Halve, L. Halzen, F. Hanson, K. Hebecker, D. Heereman, D. Helbing, K. Hellauer, R. Hickford, S. Hignight, J. Hill, G. C Hoffman, K. D Hoffmann, R. Hoinka, T. Hokanson-Fasig, B. Hoshina, K. Huang, F. Huber, M. Hultqvist, K. Hünnefeld, M. Hussain, R. In, S. Iovine, N. Ishihara, A. Jacobi, E. Japaridze, G. S Jeong, M. Jero, K. Jones, B. J P Kalaczynski, P. Kang, W. Kappes, A. Kappesser, D. Karg, T. Karle, A. Katz, U. Kauer, M. Keivani, A. Kelley, J. L Kheirandish, A. Kim, J. Kintscher, T. Kiryluk, J. Kittler, T. Klein, S. R Koirala, R. Kolanoski, H. Köpke, L. Kopper, C. Kopper, S. Koskinen, D. J Kowalski, M. Krings, K. Kroll, M. Krückl, G. Kunwar, S. Kurahashi, N. Kyriacou, A. Labare, M. Lanfranchi, J. L Larson, M. J Lauber, F. Leonard, K. Leuermann, M. Liu, Q. R Lohfink, E. Mariscal, C. J L Lu, L. Lünemann, J. Luszczak, W. Madsen, J. Maggi, G. Mahn, K. B M Makino, Y. Mancina, S. Mariş, I. C Maruyama, R. Mase, K. Maunu, R. Meagher, K. Medici, M. Meier, M. Menne, T. Merino, G. Meures, T. Miarecki, S. Micallef, J. Momenté, G. Montaruli, T. Moore, R. W Moulai, M. Nagai, R. Nahnhauer, R. Nakarmi, P. Naumann, U. Neer, G. Niederhausen, H. Nowicki, S. C Nygren, D. R Obertacke Pollmann, A. Olivas, A. O’Murchadha, A. O’Sullivan, E. Palczewski, T. Pandya, H. Pankova, D. V Peiffer, P. Pérez de los Heros, C. Pieloth, D. Pinat, E. Pizzuto, A. Plum, M. Price, P. B Przybylski, G. T Raab, C. Rameez, M. Rauch, L. Rawlins, K. Rea, I. C Reimann, R. Relethford, B. Renzi, G. Resconi, E. Rhode, W. Richman, M. Robertson, S. Rongen, M. Rott, C. Ruhe, T. Ryckbosch, D. Rysewyk, D. Safa, I. Sanchez Herrera, S. E Sandrock, A. Sandroos, J. Santander, M. Sarkar, S. Sarkar, S. Satalecka, K. Schaufel, M. Schlunder, P. Schmidt, T. Schneider, A. Schneider, J. Schöneberg, S. Schumacher, L. Sclafani, S. Seckel, D. Seunarine, S. Soedingrekso, J. Soldin, D. Song, M. Spiczak, G. M Spiering, C. Stachurska, J. Stamatikos, M. Stanev, T. Stasik, A. Stein, R. Stettner, J. Steuer, A. Stezelberger, T. Stokstad, R. G Stößl, A. Strotjohann, N. L Stuttard, T. Sullivan, G. W Sutherland, M. Taboada, I. Tenholt, F. Ter-Antonyan, S. Terliuk, A. Tilav, S. Tobin, M. N Tönnis, C. Toscano, S. Tosi, D. Tselengidou, M. Tung, C. F Turcati, A. Turcotte, R. Turley, C. F Ty, B. Unger, E. Unland Elorrieta, M. A Usner, M. Vandenbroucke, J. Van Driessche, W. van Eijk, D. van Eijndhoven, N. Vanheule, S. van Santen, J. Vraeghe, M. Walck, C. Wallace, A. Wallraff, M. Wandler, F. D Wandkowsky, N. Watson, T. B Weaver, C. Weiss, M. J Wendt, C. Werthebach, J. Westerhoff, S. Whelan, B. J Whitehorn, N. Wiebe, K. Wiebusch, C. H Wille, L. Williams, D. R Wills, L. Wolf, M. Wood, J. Wood, T. R Woolsey, E. Woschnagg, K. Wrede, G. Xu, D. L Xu, X. W Xu, Y. Yanez, J. P Yodh, G. Yoshida, S. Yuan, T. Massachusetts Institute of Technology. Department of Physics Massachusetts Institute of Technology. Department of Physics Abstract The IceCube Collaboration has observed a high-energy astrophysical neutrino flux and recently found evidence for neutrino emission from the blazar TXS 0506 $$+$$ + 056. These results open a new window into the high-energy universe. However, the source or sources of most of the observed flux of astrophysical neutrinos remains uncertain. Here, a search for steady point-like neutrino sources is performed using an unbinned likelihood analysis. The method searches for a spatial accumulation of muon-neutrino events using the very high-statistics sample of about 497,000 neutrinos recorded by IceCube between 2009 and 2017. The median angular resolution is $$\sim 1^\circ $$ ∼ 1 ∘ at 1 TeV and improves to $$\sim 0.3^\circ $$ ∼ 0 . 3 ∘ for neutrinos with an energy of 1 PeV. Compared to previous analyses, this search is optimized for point-like neutrino emission with the same flux-characteristics as the observed astrophysical muon-neutrino flux and introduces an improved event-reconstruction and parametrization of the background. The result is an improvement in sensitivity to the muon-neutrino flux compared to the previous analysis of $$\sim 35\%$$ ∼ 35 % assuming an $$E^{-2}$$ E - 2 spectrum. The sensitivity on the muon-neutrino flux is at a level of $$E^2 \mathrm {d} N /\mathrm {d} E = 3\cdot 10^{-13}\,\mathrm {TeV}\,\mathrm {cm}^{-2}\,\mathrm {s}^{-1}$$ E 2 d N / d E = 3 · 10 - 13 TeV cm - 2 s - 1 . No new evidence for neutrino sources is found in a full sky scan and in an a priori candidate source list that is motivated by gamma-ray observations. Furthermore, no significant excesses above background are found from populations of sub-threshold sources. The implications of the non-observation for potential source classes are discussed. 2021-09-16T15:14:53Z 2021-09-16T15:14:53Z 2019-03 2019-03-14T08:13:59Z Article http://purl.org/eprint/type/JournalArticle 1434-6044 1434-6052 https://hdl.handle.net/1721.1/131276 en https://doi.org/10.1140/epjc/s10052-019-6680-0 The European Physical Journal C Creative Commons Attribution 4.0 International license https://creativecommons.org/licenses/by/4.0/ The Author(s) application/pdf Springer Berlin Heidelberg Springer Berlin Heidelberg
spellingShingle	Aartsen, M. G Ackermann, M. Adams, J. Aguilar, J. A Ahlers, M. Ahrens, M. Altmann, D. Andeen, K. Anderson, T. Ansseau, I. Anton, G. Argüelles, C. Auffenberg, J. Axani, S. Backes, P. Bagherpour, H. Bai, X. Barbano, A. Barron, J. P Barwick, S. W Baum, V. Bay, R. Beatty, J. J Becker Tjus, J. Becker, K.-H. BenZvi, S. Berley, D. Bernardini, E. Besson, D. Z Binder, G. Bindig, D. Blaufuss, E. Blot, S. Bohm, C. Börner, M. Bos, F. Böser, S. Botner, O. Bourbeau, E. Bourbeau, J. Bradascio, F. Braun, J. Bretz, H.-P. Bron, S. Brostean-Kaiser, J. Burgman, A. Busse, R. S Carver, T. Chen, C. Cheung, E. Chirkin, D. Clark, K. Classen, L. Collin, G. H Conrad, J. M Coppin, P. Correa, P. Cowen, D. F Cross, R. Dave, P. Day, M. de André, J. P A M De Clercq, C. DeLaunay, J. J Dembinski, H. Deoskar, K. De Ridder, S. Desiati, P. de Vries, K. D de Wasseige, G. de With, M. DeYoung, T. Díaz-Vélez, J. C Dujmovic, H. Dunkman, M. Dvorak, E. Eberhardt, B. Ehrhardt, T. Eichmann, B. Eller, P. Evenson, P. A Fahey, S. Fazely, A. R Felde, J. Filimonov, K. Finley, C. Franckowiak, A. Friedman, E. Fritz, A. Gaisser, T. K Gallagher, J. Ganster, E. Garrappa, S. Gerhardt, L. Ghorbani, K. Giang, W. Glauch, T. Glüsenkamp, T. Goldschmidt, A. Gonzalez, J. G Grant, D. Griffith, Z. Haack, C. Hallgren, A. Halve, L. Halzen, F. Hanson, K. Hebecker, D. Heereman, D. Helbing, K. Hellauer, R. Hickford, S. Hignight, J. Hill, G. C Hoffman, K. D Hoffmann, R. Hoinka, T. Hokanson-Fasig, B. Hoshina, K. Huang, F. Huber, M. Hultqvist, K. Hünnefeld, M. Hussain, R. In, S. Iovine, N. Ishihara, A. Jacobi, E. Japaridze, G. S Jeong, M. Jero, K. Jones, B. J P Kalaczynski, P. Kang, W. Kappes, A. Kappesser, D. Karg, T. Karle, A. Katz, U. Kauer, M. Keivani, A. Kelley, J. L Kheirandish, A. Kim, J. Kintscher, T. Kiryluk, J. Kittler, T. Klein, S. R Koirala, R. Kolanoski, H. Köpke, L. Kopper, C. Kopper, S. Koskinen, D. J Kowalski, M. Krings, K. Kroll, M. Krückl, G. Kunwar, S. Kurahashi, N. Kyriacou, A. Labare, M. Lanfranchi, J. L Larson, M. J Lauber, F. Leonard, K. Leuermann, M. Liu, Q. R Lohfink, E. Mariscal, C. J L Lu, L. Lünemann, J. Luszczak, W. Madsen, J. Maggi, G. Mahn, K. B M Makino, Y. Mancina, S. Mariş, I. C Maruyama, R. Mase, K. Maunu, R. Meagher, K. Medici, M. Meier, M. Menne, T. Merino, G. Meures, T. Miarecki, S. Micallef, J. Momenté, G. Montaruli, T. Moore, R. W Moulai, M. Nagai, R. Nahnhauer, R. Nakarmi, P. Naumann, U. Neer, G. Niederhausen, H. Nowicki, S. C Nygren, D. R Obertacke Pollmann, A. Olivas, A. O’Murchadha, A. O’Sullivan, E. Palczewski, T. Pandya, H. Pankova, D. V Peiffer, P. Pérez de los Heros, C. Pieloth, D. Pinat, E. Pizzuto, A. Plum, M. Price, P. B Przybylski, G. T Raab, C. Rameez, M. Rauch, L. Rawlins, K. Rea, I. C Reimann, R. Relethford, B. Renzi, G. Resconi, E. Rhode, W. Richman, M. Robertson, S. Rongen, M. Rott, C. Ruhe, T. Ryckbosch, D. Rysewyk, D. Safa, I. Sanchez Herrera, S. E Sandrock, A. Sandroos, J. Santander, M. Sarkar, S. Sarkar, S. Satalecka, K. Schaufel, M. Schlunder, P. Schmidt, T. Schneider, A. Schneider, J. Schöneberg, S. Schumacher, L. Sclafani, S. Seckel, D. Seunarine, S. Soedingrekso, J. Soldin, D. Song, M. Spiczak, G. M Spiering, C. Stachurska, J. Stamatikos, M. Stanev, T. Stasik, A. Stein, R. Stettner, J. Steuer, A. Stezelberger, T. Stokstad, R. G Stößl, A. Strotjohann, N. L Stuttard, T. Sullivan, G. W Sutherland, M. Taboada, I. Tenholt, F. Ter-Antonyan, S. Terliuk, A. Tilav, S. Tobin, M. N Tönnis, C. Toscano, S. Tosi, D. Tselengidou, M. Tung, C. F Turcati, A. Turcotte, R. Turley, C. F Ty, B. Unger, E. Unland Elorrieta, M. A Usner, M. Vandenbroucke, J. Van Driessche, W. van Eijk, D. van Eijndhoven, N. Vanheule, S. van Santen, J. Vraeghe, M. Walck, C. Wallace, A. Wallraff, M. Wandler, F. D Wandkowsky, N. Watson, T. B Weaver, C. Weiss, M. J Wendt, C. Werthebach, J. Westerhoff, S. Whelan, B. J Whitehorn, N. Wiebe, K. Wiebusch, C. H Wille, L. Williams, D. R Wills, L. Wolf, M. Wood, J. Wood, T. R Woolsey, E. Woschnagg, K. Wrede, G. Xu, D. L Xu, X. W Xu, Y. Yanez, J. P Yodh, G. Yoshida, S. Yuan, T. Search for steady point-like sources in the astrophysical muon neutrino flux with 8 years of IceCube data
title	Search for steady point-like sources in the astrophysical muon neutrino flux with 8 years of IceCube data
title_full	Search for steady point-like sources in the astrophysical muon neutrino flux with 8 years of IceCube data
title_fullStr	Search for steady point-like sources in the astrophysical muon neutrino flux with 8 years of IceCube data
title_full_unstemmed	Search for steady point-like sources in the astrophysical muon neutrino flux with 8 years of IceCube data
title_short	Search for steady point-like sources in the astrophysical muon neutrino flux with 8 years of IceCube data
title_sort	search for steady point like sources in the astrophysical muon neutrino flux with 8 years of icecube data
url	https://hdl.handle.net/1721.1/131276
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Search for steady point-like sources in the astrophysical muon neutrino flux with 8 years of IceCube data

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