Constraints on populations of neutrino sources from searches in the directions of IceCube neutrino alerts
- Author
- R. Abbasi, M. Ackermann, J. Adams, N. Aggarwal, J. A. Aguilar, M. Ahlers, J. M. Alameddine, A. A. Alves, N. M. Amin, K. Andeen, T. Anderson, G. Anton, C. Argüelles, Y. Ashida, S. Athanasiadou, S. N. Axani, X. Bai, A. Balagopal V., M. Baricevic, S. W. Barwick, V. Basu, R. Bay, J. J. Beatty, K.-H. Becker, J. Becker Tjus, J. Beise, C. Bellenghi, S. Benda, S. BenZvi, D. Berley, E. Bernardini, D. Z. Besson, G. Binder, D. Bindig, E. Blaufuss, S. Blot, F. Bontempo, J. Y. Book, J. Borowka, C. Boscolo Meneguolo, S. Böser, O. Botner, J. Böttcher, E. Bourbeau, J. Braun, B. Brinson, J. Brostean-Kaiser, R. T. Burley, R. S. Busse, M. A. Campana, E. G. Carnie-Bronca, C. Chen, Z. Chen, D. Chirkin, K. Choi, B. A. Clark, L. Classen, A. Coleman, G. H. Collin, A. Connolly, J. M. Conrad, P. Coppin, P. Correa, S. Countryman, D. F. Cowen, R. Cross, C. Dappen, P. Dave, C. De Clercq, J. J. DeLaunay, D. Delgado López, H. Dembinski, K. Deoskar, A. Desai, P. Desiati, K. D. de Vries, G. de Wasseige, T. DeYoung, A. Diaz, J. C. Díaz-Vélez, M. Dittmer, H. Dujmovic, M. A. DuVernois, T. Ehrhardt, P. Eller, R. Engel, H. Erpenbeck, J. Evans, P. A. Evenson, K. L. Fan, A. R. Fazely, A. Fedynitch, N. Feigl, S. Fiedlschuster, A. T. Fienberg, C. Finley, L. Fischer, D. Fox, A. Franckowiak, E. Friedman, A. Fritz, P. Fürst, T. K. Gaisser, J. Gallagher, E. Ganster, A. Garcia, S. Garrappa, L. Gerhardt, A. Ghadimi, C. Glaser, T. Glauch, T. Glüsenkamp, N. Goehlke, J. G. Gonzalez, S. Goswami, D. Grant, S. J. Gray, T. Grégoire, S. Griswold, C. Günther, P. Gutjahr, C. Haack, A. Hallgren, R. Halliday, L. Halve, F. Halzen, H. Hamdaoui, M. Ha Minh, K. Hanson, J. Hardin, A. A. Harnisch, P. Hatch, A. Haungs, K. Helbing, J. Hellrung, F. Henningsen, L. Heuermann, S. Hickford, A. Hidvegi, C. Hill, G. C. Hill, K. D. Hoffman, K. Hoshina, W. Hou, T. Huber, K. Hultqvist, M. Hünnefeld, R. Hussain, K. Hymon, S. In, N. Iovine, A. Ishihara, M. Jansson, G. S. Japaridze, M. Jeong, M. Jin, B. J. P. Jones, D. Kang, W. Kang, X. Kang, A. Kappes, D. Kappesser, L. Kardum, T. Karg, M. Karl, A. Karle, U. Katz, M. Kauer, J. L. Kelley, A. Kheirandish, K. Kin, J. Kiryluk, S. R. Klein, A. Kochocki, R. Koirala, H. Kolanoski, T. Kontrimas, L. Köpke, C. Kopper, D. J. Koskinen, P. Koundal, M. Kovacevich, M. Kowalski, T. Kozynets, E. Krupczak, E. Kun, N. Kurahashi, N. Lad, C. Lagunas Gualda, M. J. Larson, F. Lauber, J. P. Lazar, J. W. Lee, K. Leonard, A. Leszczyńska, M. Lincetto, Q. R. Liu, M. Liubarska, E. Lohfink, C. Love, C. J. Lozano Mariscal, L. Lu, F. Lucarelli, A. Ludwig, W. Luszczak, Y. Lyu, W. Y. Ma, J. Madsen, K. B. M. Mahn, Y. Makino, S. Mancina, W. Marie Sainte, I. C. Mariş, S. Marka, Z. Marka, M. Marsee, I. Martinez-Soler, R. Maruyama, T. McElroy, F. McNally, J. V. Mead, K. Meagher, S. Mechbal, A. Medina, M. Meier, S. Meighen-Berger, Y. Merckx, J. Micallef, D. Mockler, T. Montaruli, R. W. Moore, R. Morse, M. Moulai, T. Mukherjee, R. Naab, R. Nagai, U. Naumann, A. Nayerhoda, J. Necker, M. Neumann, H. Niederhausen, M. U. Nisa, A. Noell, S. C. Nowicki, A. Obertacke Pollmann, M. Oehler, Bob Oeyen (UGent) , A. Olivas, R. Orsoe, J. Osborn, E. O’Sullivan, H. Pandya, D. V. Pankova, N. Park, G. K. Parker, E. N. Paudel, L. Paul, C. Pérez de los Heros, L. Peters, J. Peterson, S. Philippen, S. Pieper, A. Pizzuto, M. Plum, Y. Popovych, Alessio Porcelli (UGent) , M. Prado Rodriguez, B. Pries, R. Procter-Murphy, G. T. Przybylski, C. Raab, J. Rack-Helleis, M. Rameez, K. Rawlins, Z. Rechav, A. Rehman, P. Reichherzer, G. Renzi, E. Resconi, S. Reusch, W. Rhode, M. Richman, B. Riedel, E. J. Roberts, S. Robertson, S. Rodan, G. Roellinghoff, M. Rongen, C. Rott, T. Ruhe, L. Ruohan, Dirk Ryckbosch (UGent) , D. Rysewyk Cantu, I. Safa, J. Saffer, D. Salazar-Gallegos, P. Sampathkumar, S. E. Sanchez Herrera, A. Sandrock, M. Santander, S. Sarkar, S. Sarkar, J. Savelberg, M. Schaufel, H. Schieler, S. Schindler, B. Schlueter, T. Schmidt, J. Schneider, F. G. Schröder, L. Schumacher, G. Schwefer, S. Sclafani, S. Seunarine, A. Sharma, S. Shefali, N. Shimizu, M. Silva, B. Skrzypek, B. Smithers, R. Snihur, J. Soedingrekso, A. Søgaard, D. Soldin, C. Spannfellner, G. M. Spiczak, C. Spiering, M. Stamatikos, T. Stanev, R. Stein, T. Stezelberger, T. Stürwald, T. Stuttard, G. W. Sullivan, I. Taboada, S. Ter-Antonyan, W. G. Thompson, J. Thwaites, S. Tilav, K. Tollefson, C. Tönnis, S. Toscano, D. Tosi, A. Trettin, C. F. Tung, R. Turcotte, J. P. Twagirayezu, B. Ty, M. A. Unland Elorrieta, K. Upshaw, N. Valtonen-Mattila, J. Vandenbroucke, N. van Eijndhoven, D. Vannerom, J. van Santen, J. Vara, J. Veitch-Michaelis, Stef Verpoest, D. Veske, C. Walck, W. Wang, T. B. Watson, C. Weaver, P. Weigel, A. Weindl, J. Weldert, C. Wendt, J. Werthebach, M. Weyrauch, N. Whitehorn, C. H. Wiebusch, N. Willey, D. R. Williams, M. Wolf, G. Wrede, J. Wulff, X. W. Xu, J. P. Yanez, E. Yildizci, S. Yoshida, S. Yu, T. Yuan, Z. Zhang, P. Zhelnin and [ missing ] on behalf of the IceCube Collaboration
- Organization
- Abstract
- Beginning in 2016, the IceCube Neutrino Observatory has sent out alerts in real time containing the information of high-energy (E & GSIM; 100 TeV) neutrino candidate events with moderate to high (& GSIM;30%) probability of astrophysical origin. In this work, we use a recent catalog of such alert events, which, in addition to events announced in real time, includes events that were identified retroactively and covers the time period of 2011-2020. We also search for additional, lower-energy neutrinos from the arrival directions of these IceCube alerts. We show how performing such an analysis can constrain the contribution of rare populations of cosmic neutrino sources to the diffuse astrophysical neutrino flux. After searching for neutrino emission coincident with these alert events on various timescales, we find no significant evidence of either minute-scale or day-scale transient neutrino emission or of steady neutrino emission in the direction of these alert events. This study also shows how numerous a population of neutrino sources has to be to account for the complete astrophysical neutrino flux. Assuming that sources have the same luminosity, an E (-2.5) neutrino spectrum, and number densities that follow star formation rates, the population of sources has to be more numerous than 7 x 10(-9) Mpc(-3). This number changes to 3 x 10(-7) Mpc(-3) if number densities instead have no cosmic evolution.
- Keywords
- Space and Planetary Science, Astronomy and Astrophysics, HIGH-ENERGY NEUTRINOS, FLUX, COINCIDENT, BURSTS, ORIGIN
Downloads
-
Abbasi 2023 ApJ 951 45.pdf
- full text (Published version)
- |
- open access
- |
- |
- 1.96 MB
Citation
Please use this url to cite or link to this publication: http://hdl.handle.net/1854/LU-01H819A8AAN51RY7V65HVWCVMY
- MLA
- Abbasi, R., et al. “Constraints on Populations of Neutrino Sources from Searches in the Directions of IceCube Neutrino Alerts.” ASTROPHYSICAL JOURNAL, vol. 951, no. 1, 2023, doi:10.3847/1538-4357/acd2ca.
- APA
- Abbasi, R., Ackermann, M., Adams, J., Aggarwal, N., Aguilar, J. A., Ahlers, M., … on behalf of the IceCube Collaboration, [ missing ]. (2023). Constraints on populations of neutrino sources from searches in the directions of IceCube neutrino alerts. ASTROPHYSICAL JOURNAL, 951(1). https://doi.org/10.3847/1538-4357/acd2ca
- Chicago author-date
- Abbasi, R., M. Ackermann, J. Adams, N. Aggarwal, J. A. Aguilar, M. Ahlers, J. M. Alameddine, et al. 2023. “Constraints on Populations of Neutrino Sources from Searches in the Directions of IceCube Neutrino Alerts.” ASTROPHYSICAL JOURNAL 951 (1). https://doi.org/10.3847/1538-4357/acd2ca.
- Chicago author-date (all authors)
- Abbasi, R., M. Ackermann, J. Adams, N. Aggarwal, J. A. Aguilar, M. Ahlers, J. M. Alameddine, A. A. Alves, N. M. Amin, K. Andeen, T. Anderson, G. Anton, C. Argüelles, Y. Ashida, S. Athanasiadou, S. N. Axani, X. Bai, A. Balagopal V., M. Baricevic, S. W. Barwick, V. Basu, R. Bay, J. J. Beatty, K.-H. Becker, J. Becker Tjus, J. Beise, C. Bellenghi, S. Benda, S. BenZvi, D. Berley, E. Bernardini, D. Z. Besson, G. Binder, D. Bindig, E. Blaufuss, S. Blot, F. Bontempo, J. Y. Book, J. Borowka, C. Boscolo Meneguolo, S. Böser, O. Botner, J. Böttcher, E. Bourbeau, J. Braun, B. Brinson, J. Brostean-Kaiser, R. T. Burley, R. S. Busse, M. A. Campana, E. G. Carnie-Bronca, C. Chen, Z. Chen, D. Chirkin, K. Choi, B. A. Clark, L. Classen, A. Coleman, G. H. Collin, A. Connolly, J. M. Conrad, P. Coppin, P. Correa, S. Countryman, D. F. Cowen, R. Cross, C. Dappen, P. Dave, C. De Clercq, J. J. DeLaunay, D. Delgado López, H. Dembinski, K. Deoskar, A. Desai, P. Desiati, K. D. de Vries, G. de Wasseige, T. DeYoung, A. Diaz, J. C. Díaz-Vélez, M. Dittmer, H. Dujmovic, M. A. DuVernois, T. Ehrhardt, P. Eller, R. Engel, H. Erpenbeck, J. Evans, P. A. Evenson, K. L. Fan, A. R. Fazely, A. Fedynitch, N. Feigl, S. Fiedlschuster, A. T. Fienberg, C. Finley, L. Fischer, D. Fox, A. Franckowiak, E. Friedman, A. Fritz, P. Fürst, T. K. Gaisser, J. Gallagher, E. Ganster, A. Garcia, S. Garrappa, L. Gerhardt, A. Ghadimi, C. Glaser, T. Glauch, T. Glüsenkamp, N. Goehlke, J. G. Gonzalez, S. Goswami, D. Grant, S. J. Gray, T. Grégoire, S. Griswold, C. Günther, P. Gutjahr, C. Haack, A. Hallgren, R. Halliday, L. Halve, F. Halzen, H. Hamdaoui, M. Ha Minh, K. Hanson, J. Hardin, A. A. Harnisch, P. Hatch, A. Haungs, K. Helbing, J. Hellrung, F. Henningsen, L. Heuermann, S. Hickford, A. Hidvegi, C. Hill, G. C. Hill, K. D. Hoffman, K. Hoshina, W. Hou, T. Huber, K. Hultqvist, M. Hünnefeld, R. Hussain, K. Hymon, S. In, N. Iovine, A. Ishihara, M. Jansson, G. S. Japaridze, M. Jeong, M. Jin, B. J. P. Jones, D. Kang, W. Kang, X. Kang, A. Kappes, D. Kappesser, L. Kardum, T. Karg, M. Karl, A. Karle, U. Katz, M. Kauer, J. L. Kelley, A. Kheirandish, K. Kin, J. Kiryluk, S. R. Klein, A. Kochocki, R. Koirala, H. Kolanoski, T. Kontrimas, L. Köpke, C. Kopper, D. J. Koskinen, P. Koundal, M. Kovacevich, M. Kowalski, T. Kozynets, E. Krupczak, E. Kun, N. Kurahashi, N. Lad, C. Lagunas Gualda, M. J. Larson, F. Lauber, J. P. Lazar, J. W. Lee, K. Leonard, A. Leszczyńska, M. Lincetto, Q. R. Liu, M. Liubarska, E. Lohfink, C. Love, C. J. Lozano Mariscal, L. Lu, F. Lucarelli, A. Ludwig, W. Luszczak, Y. Lyu, W. Y. Ma, J. Madsen, K. B. M. Mahn, Y. Makino, S. Mancina, W. Marie Sainte, I. C. Mariş, S. Marka, Z. Marka, M. Marsee, I. Martinez-Soler, R. Maruyama, T. McElroy, F. McNally, J. V. Mead, K. Meagher, S. Mechbal, A. Medina, M. Meier, S. Meighen-Berger, Y. Merckx, J. Micallef, D. Mockler, T. Montaruli, R. W. Moore, R. Morse, M. Moulai, T. Mukherjee, R. Naab, R. Nagai, U. Naumann, A. Nayerhoda, J. Necker, M. Neumann, H. Niederhausen, M. U. Nisa, A. Noell, S. C. Nowicki, A. Obertacke Pollmann, M. Oehler, Bob Oeyen, A. Olivas, R. Orsoe, J. Osborn, E. O’Sullivan, H. Pandya, D. V. Pankova, N. Park, G. K. Parker, E. N. Paudel, L. Paul, C. Pérez de los Heros, L. Peters, J. Peterson, S. Philippen, S. Pieper, A. Pizzuto, M. Plum, Y. Popovych, Alessio Porcelli, M. Prado Rodriguez, B. Pries, R. Procter-Murphy, G. T. Przybylski, C. Raab, J. Rack-Helleis, M. Rameez, K. Rawlins, Z. Rechav, A. Rehman, P. Reichherzer, G. Renzi, E. Resconi, S. Reusch, W. Rhode, M. Richman, B. Riedel, E. J. Roberts, S. Robertson, S. Rodan, G. Roellinghoff, M. Rongen, C. Rott, T. Ruhe, L. Ruohan, Dirk Ryckbosch, D. Rysewyk Cantu, I. Safa, J. Saffer, D. Salazar-Gallegos, P. Sampathkumar, S. E. Sanchez Herrera, A. Sandrock, M. Santander, S. Sarkar, S. Sarkar, J. Savelberg, M. Schaufel, H. Schieler, S. Schindler, B. Schlueter, T. Schmidt, J. Schneider, F. G. Schröder, L. Schumacher, G. Schwefer, S. Sclafani, S. Seunarine, A. Sharma, S. Shefali, N. Shimizu, M. Silva, B. Skrzypek, B. Smithers, R. Snihur, J. Soedingrekso, A. Søgaard, D. Soldin, C. Spannfellner, G. M. Spiczak, C. Spiering, M. Stamatikos, T. Stanev, R. Stein, T. Stezelberger, T. Stürwald, T. Stuttard, G. W. Sullivan, I. Taboada, S. Ter-Antonyan, W. G. Thompson, J. Thwaites, S. Tilav, K. Tollefson, C. Tönnis, S. Toscano, D. Tosi, A. Trettin, C. F. Tung, R. Turcotte, J. P. Twagirayezu, B. Ty, M. A. Unland Elorrieta, K. Upshaw, N. Valtonen-Mattila, J. Vandenbroucke, N. van Eijndhoven, D. Vannerom, J. van Santen, J. Vara, J. Veitch-Michaelis, Stef Verpoest, D. Veske, C. Walck, W. Wang, T. B. Watson, C. Weaver, P. Weigel, A. Weindl, J. Weldert, C. Wendt, J. Werthebach, M. Weyrauch, N. Whitehorn, C. H. Wiebusch, N. Willey, D. R. Williams, M. Wolf, G. Wrede, J. Wulff, X. W. Xu, J. P. Yanez, E. Yildizci, S. Yoshida, S. Yu, T. Yuan, Z. Zhang, P. Zhelnin, and [ missing ] on behalf of the IceCube Collaboration. 2023. “Constraints on Populations of Neutrino Sources from Searches in the Directions of IceCube Neutrino Alerts.” ASTROPHYSICAL JOURNAL 951 (1). doi:10.3847/1538-4357/acd2ca.
- Vancouver
- 1.Abbasi R, Ackermann M, Adams J, Aggarwal N, Aguilar JA, Ahlers M, et al. Constraints on populations of neutrino sources from searches in the directions of IceCube neutrino alerts. ASTROPHYSICAL JOURNAL. 2023;951(1).
- IEEE
- [1]R. Abbasi et al., “Constraints on populations of neutrino sources from searches in the directions of IceCube neutrino alerts,” ASTROPHYSICAL JOURNAL, vol. 951, no. 1, 2023.
@article{01H819A8AAN51RY7V65HVWCVMY, abstract = {{ Beginning in 2016, the IceCube Neutrino Observatory has sent out alerts in real time containing the information of high-energy (E & GSIM; 100 TeV) neutrino candidate events with moderate to high (& GSIM;30%) probability of astrophysical origin. In this work, we use a recent catalog of such alert events, which, in addition to events announced in real time, includes events that were identified retroactively and covers the time period of 2011-2020. We also search for additional, lower-energy neutrinos from the arrival directions of these IceCube alerts. We show how performing such an analysis can constrain the contribution of rare populations of cosmic neutrino sources to the diffuse astrophysical neutrino flux. After searching for neutrino emission coincident with these alert events on various timescales, we find no significant evidence of either minute-scale or day-scale transient neutrino emission or of steady neutrino emission in the direction of these alert events. This study also shows how numerous a population of neutrino sources has to be to account for the complete astrophysical neutrino flux. Assuming that sources have the same luminosity, an E (-2.5) neutrino spectrum, and number densities that follow star formation rates, the population of sources has to be more numerous than 7 x 10(-9) Mpc(-3). This number changes to 3 x 10(-7) Mpc(-3) if number densities instead have no cosmic evolution.}}, articleno = {{45}}, author = {{Abbasi, R. and Ackermann, M. and Adams, J. and Aggarwal, N. and Aguilar, J. A. and Ahlers, M. and Alameddine, J. M. and Alves, A. A. and Amin, N. M. and Andeen, K. and Anderson, T. and Anton, G. and Argüelles, C. and Ashida, Y. and Athanasiadou, S. and Axani, S. N. and Bai, X. and V., A. Balagopal and Baricevic, M. and Barwick, S. W. and Basu, V. and Bay, R. and Beatty, J. J. and Becker, K.-H. and Tjus, J. Becker and Beise, J. and Bellenghi, C. and Benda, S. and BenZvi, S. and Berley, D. and Bernardini, E. and Besson, D. Z. and Binder, G. and Bindig, D. and Blaufuss, E. and Blot, S. and Bontempo, F. and Book, J. Y. and Borowka, J. and Meneguolo, C. Boscolo and Böser, S. and Botner, O. and Böttcher, J. and Bourbeau, E. and Braun, J. and Brinson, B. and Brostean-Kaiser, J. and Burley, R. T. and Busse, R. S. and Campana, M. A. and Carnie-Bronca, E. G. and Chen, C. and Chen, Z. and Chirkin, D. and Choi, K. and Clark, B. A. and Classen, L. and Coleman, A. and Collin, G. H. and Connolly, A. and Conrad, J. M. and Coppin, P. and Correa, P. and Countryman, S. and Cowen, D. F. and Cross, R. and Dappen, C. and Dave, P. and De Clercq, C. and DeLaunay, J. J. and Delgado López, D. and Dembinski, H. and Deoskar, K. and Desai, A. and Desiati, P. and de Vries, K. D. and de Wasseige, G. and DeYoung, T. and Diaz, A. and Díaz-Vélez, J. C. and Dittmer, M. and Dujmovic, H. and DuVernois, M. A. and Ehrhardt, T. and Eller, P. and Engel, R. and Erpenbeck, H. and Evans, J. and Evenson, P. A. and Fan, K. L. and Fazely, A. R. and Fedynitch, A. and Feigl, N. and Fiedlschuster, S. and Fienberg, A. T. and Finley, C. and Fischer, L. and Fox, D. and Franckowiak, A. and Friedman, E. and Fritz, A. and Fürst, P. and Gaisser, T. K. and Gallagher, J. and Ganster, E. and Garcia, A. and Garrappa, S. and Gerhardt, L. and Ghadimi, A. and Glaser, C. and Glauch, T. and Glüsenkamp, T. and Goehlke, N. and Gonzalez, J. G. and Goswami, S. and Grant, D. and Gray, S. J. and Grégoire, T. and Griswold, S. and Günther, C. and Gutjahr, P. and Haack, C. and Hallgren, A. and Halliday, R. and Halve, L. and Halzen, F. and Hamdaoui, H. and Minh, M. Ha and Hanson, K. and Hardin, J. and Harnisch, A. A. and Hatch, P. and Haungs, A. and Helbing, K. and Hellrung, J. and Henningsen, F. and Heuermann, L. and Hickford, S. and Hidvegi, A. and Hill, C. and Hill, G. C. and Hoffman, K. D. and Hoshina, K. and Hou, W. and Huber, T. and Hultqvist, K. and Hünnefeld, M. and Hussain, R. and Hymon, K. and In, S. and Iovine, N. and Ishihara, A. and Jansson, M. and Japaridze, G. S. and Jeong, M. and Jin, M. and Jones, B. J. P. and Kang, D. and Kang, W. and Kang, X. and Kappes, A. and Kappesser, D. and Kardum, L. and Karg, T. and Karl, M. and Karle, A. and Katz, U. and Kauer, M. and Kelley, J. L. and Kheirandish, A. and Kin, K. and Kiryluk, J. and Klein, S. R. and Kochocki, A. and Koirala, R. and Kolanoski, H. and Kontrimas, T. and Köpke, L. and Kopper, C. and Koskinen, D. J. and Koundal, P. and Kovacevich, M. and Kowalski, M. and Kozynets, T. and Krupczak, E. and Kun, E. and Kurahashi, N. and Lad, N. and Lagunas Gualda, C. and Larson, M. J. and Lauber, F. and Lazar, J. P. and Lee, J. W. and Leonard, K. and Leszczyńska, A. and Lincetto, M. and Liu, Q. R. and Liubarska, M. and Lohfink, E. and Love, C. and Mariscal, C. J. Lozano and Lu, L. and Lucarelli, F. and Ludwig, A. and Luszczak, W. and Lyu, Y. and Ma, W. Y. and Madsen, J. and Mahn, K. B. M. and Makino, Y. and Mancina, S. and Sainte, W. Marie and Mariş, I. C. and Marka, S. and Marka, Z. and Marsee, M. and Martinez-Soler, I. and Maruyama, R. and McElroy, T. and McNally, F. and Mead, J. V. and Meagher, K. and Mechbal, S. and Medina, A. and Meier, M. and Meighen-Berger, S. and Merckx, Y. and Micallef, J. and Mockler, D. and Montaruli, T. and Moore, R. W. and Morse, R. and Moulai, M. and Mukherjee, T. and Naab, R. and Nagai, R. and Naumann, U. and Nayerhoda, A. and Necker, J. and Neumann, M. and Niederhausen, H. and Nisa, M. U. and Noell, A. and Nowicki, S. C. and Pollmann, A. Obertacke and Oehler, M. and Oeyen, Bob and Olivas, A. and Orsoe, R. and Osborn, J. and O’Sullivan, E. and Pandya, H. and Pankova, D. V. and Park, N. and Parker, G. K. and Paudel, E. N. and Paul, L. and de los Heros, C. Pérez and Peters, L. and Peterson, J. and Philippen, S. and Pieper, S. and Pizzuto, A. and Plum, M. and Popovych, Y. and Porcelli, Alessio and Prado Rodriguez, M. and Pries, B. and Procter-Murphy, R. and Przybylski, G. T. and Raab, C. and Rack-Helleis, J. and Rameez, M. and Rawlins, K. and Rechav, Z. and Rehman, A. and Reichherzer, P. and Renzi, G. and Resconi, E. and Reusch, S. and Rhode, W. and Richman, M. and Riedel, B. and Roberts, E. J. and Robertson, S. and Rodan, S. and Roellinghoff, G. and Rongen, M. and Rott, C. and Ruhe, T. and Ruohan, L. and Ryckbosch, Dirk and Rysewyk Cantu, D. and Safa, I. and Saffer, J. and Salazar-Gallegos, D. and Sampathkumar, P. and Sanchez Herrera, S. E. and Sandrock, A. and Santander, M. and Sarkar, S. and Sarkar, S. and Savelberg, J. and Schaufel, M. and Schieler, H. and Schindler, S. and Schlueter, B. and Schmidt, T. and Schneider, J. and Schröder, F. G. and Schumacher, L. and Schwefer, G. and Sclafani, S. and Seunarine, S. and Sharma, A. and Shefali, S. and Shimizu, N. and Silva, M. and Skrzypek, B. and Smithers, B. and Snihur, R. and Soedingrekso, J. and Søgaard, A. and Soldin, D. and Spannfellner, C. and Spiczak, G. M. and Spiering, C. and Stamatikos, M. and Stanev, T. and Stein, R. and Stezelberger, T. and Stürwald, T. and Stuttard, T. and Sullivan, G. W. and Taboada, I. and Ter-Antonyan, S. and Thompson, W. G. and Thwaites, J. and Tilav, S. and Tollefson, K. and Tönnis, C. and Toscano, S. and Tosi, D. and Trettin, A. and Tung, C. F. and Turcotte, R. and Twagirayezu, J. P. and Ty, B. and Unland Elorrieta, M. A. and Upshaw, K. and Valtonen-Mattila, N. and Vandenbroucke, J. and van Eijndhoven, N. and Vannerom, D. and van Santen, J. and Vara, J. and Veitch-Michaelis, J. and Verpoest, Stef and Veske, D. and Walck, C. and Wang, W. and Watson, T. B. and Weaver, C. and Weigel, P. and Weindl, A. and Weldert, J. and Wendt, C. and Werthebach, J. and Weyrauch, M. and Whitehorn, N. and Wiebusch, C. H. and Willey, N. and Williams, D. R. and Wolf, M. and Wrede, G. and Wulff, J. and Xu, X. W. and Yanez, J. P. and Yildizci, E. and Yoshida, S. and Yu, S. and Yuan, T. and Zhang, Z. and Zhelnin, P. and on behalf of the IceCube Collaboration, [ missing ]}}, issn = {{0004-637X}}, journal = {{ASTROPHYSICAL JOURNAL}}, keywords = {{Space and Planetary Science,Astronomy and Astrophysics,HIGH-ENERGY NEUTRINOS,FLUX,COINCIDENT,BURSTS,ORIGIN}}, language = {{eng}}, number = {{1}}, pages = {{16}}, title = {{Constraints on populations of neutrino sources from searches in the directions of IceCube neutrino alerts}}, url = {{http://doi.org/10.3847/1538-4357/acd2ca}}, volume = {{951}}, year = {{2023}}, }
- Altmetric
- View in Altmetric
- Web of Science
- Times cited: