@inproceedings{01HVRPEV3VVS3BXXZ56CB2J8S2,
  abstract     = {{On 22 September 2017, IceCube reported a high-energy neutrino event which was found to be coincident with a flaring blazar, TXS 0506+056. This multi-messenger observation hinted at blazars contributing to the observed high-energy astrophysical neutrinos and raised a need for extensive correlation studies. Recent work shows that the internal absorption of gamma rays, and their interactions intrinsic to the source and with the extragalactic background, will cause a lack of energetic gamma-ray and neutrino correlation while hinting towards a correlation between neutrinos and lower photon energy observations in the X-ray and radio bands. Studies based on published IceCube alerts and radio observations report a possible radio-neutrino correlation in both gamma-ray bright and gamma-ray dim active galactic nuclei (AGN). However, they have marginal statistical significance due to limited available data. We present a correlation analysis between 15 GHz radio observations of AGN reported in the MOJAVE XV catalog and 10 years of IceCube detector data and discuss the results derived from a time-averaged stacking analysis.}},
  articleno    = {{949}},
  author       = {{Abbasi, R. and  Ackermann, M. and  Adams, J. and  Aguilar, J. A. and  Ahlers, M. and  Ahrens, M. and  Alispach, C. and  Alves, A. A. and  Amin, N. M. and  An, R. and  Andeen, K. and  Anderson, T. and  Anton, G. and  Arguelles, C. and  Ashida, Y. and  Axani, S. and  Bai, X. and  Balagopal, A. and  Barbano, A. and  Barwick, S. W. and  Bastian, B. and  Basu, V. and  Baur, S. and  Bay, R. and  Beatty, J. J. and  Becker, K. -H. and  Tjus, J. Becker and  Bellenghi, C. 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  Boddenberg, M. and  Bontempo, F. and  Borowka, J. and  Boser, S. and  Botner, O. and  Bottcher, J. and  Bourbeau, E. and  Bradascio, F. and  Braun, J. and  Bron, S. and  Brostean-Kaiser, J. and  Browne, S. and  Burgman, A. and  Burley, R. T. and  Busse, R. S. and  Campana, M. A. and  Carnie-Bronca, E. G. and  Chen, C. and  Chirkin, D. and  Choi, K. and  Clark, B. A. and  Clark, K. and  Classen, L. and  Coleman, A. and  Collin, G. H. and  Conrad, J. M. and  Coppin, P. and  Correa, P. and  Cowen, D. F. and  Cross, R. and  Dappen, C. and  Dave, P. and  De Clercq, C. and  DeLaunay, J. J. and  Dembinski, H. and  Deoskar, K. and De Ridder, Sam and  Desai, A. and  Desiati, P. and  de Vries, K. D. and  de Wasseige, G. and  de With, M. and  DeYoung, T. and  Dharani, S. and  Diaz, A. and  Diaz-Velez, J. C. and  Dittmer, M. and  Dujmovic, H. and  Dunkman, M. and  DuVernois, M. A. and  Dvorak, E. 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  Fiedlschuster, S. and  Fienberg, A. T. and  Filimonov, K. and  Finley, C. and  Fischer, L. and  Fox, D. and  Franckowiak, A. and  Friedman, E. and  Fritz, A. and  Furst, 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  Glusenkamp, T. and  Goldschmidt, A. and  Gonzalez, J. G. and  Goswami, S. and  Grant, D. and  Gregoire, T. and  Griswold, S. and  Gunduz, M. and  Gunther, C. and  Haack, C. and  Hallgren, A. and  Halliday, R. and  Halve, L. and  Halzen, F. and  Minh, M. Ha and  Hanson, K. and  Hardin, J. and  Harnisch, A. A. and  Haungs, A. and  Hauser, S. and  Hebecker, D. and  Helbing, K. and  Henningsen, F. and  Hettinger, E. C. and  Hickford, S. and  Hignight, J. and  Hill, C. and  Hill, G. C. and  Hoffman, K. D. and  Hoffmann, R. and  Hoinka, T. and  Hokanson-Fasig, B. and  Hoshina, K. and  Huang, F. and  Huber, M. and  Huber, T. and  Hultqvist, K. and  Hunnefeld, M. and  Hussain, R. and  In, S. and  Iovine, N. and  Ishihara, A. and  Jansson, M. and  Japaridze, G. S. and  Jeong, M. and  Jones, B. J. P. and  Kang, D. and  Kang, W. and  Kang, X. and  Kappes, A. and  Kappesser, D. and  Karg, T. and  Karl, M. and  Karle, A. and  Katz, U. and  Kauer, M. and  Kellermann, M. and  Kelley, J. L. and  Kheirandish, A. and  Kin, K. and  Kintscher, T. and  Kiryluk, J. and  Klein, S. R. and  Koirala, R. and  Kolanoski, H. and  Kontrimas, T. and  Kopke, L. and  Kopper, C. and  Kopper, S. and  Koskinen, D. J. and  Koundal, P. and  Kovacevich, M. and  Kowalski, M. and  Kozynets, T. and  Kun, E. and  Kurahashi, N. and  Lad, N. and  Gualda, C. Lagunas and  Lanfranchi, J. L. and  Larson, M. J. and  Lauber, F. and  Lazar, J. P. and  Lee, J. W. and  Leonard, K. and  Leszczynska, A. and  Li, Y. and  Lincetto, M. and  Liu, Q. R. and  Liubarska, M. and  Lohfink, E. 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  Maris, I. C. and  Maruyama, R. and  Mase, K. and  McElroy, T. and  McNally, F. and  Mead, J. V. and  Meagher, K. and  Medina, A. and  Meier, M. and  Meighen-Berger, S. and  Micallef, J. and  Mockler, D. and  Montaruli, T. and  Moore, R. W. and  Morse, R. and  Moulai, M. and  Naab, R. and  Nagai, R. and  Naumann, U. and  Necker, J. and  Nguyen, L. V. and  Niederhausen, H. and  Nisa, M. U. and  Nowicki, S. C. and  Nygren, D. R. and  Pollmann, A. Obertacke and  Oehler, M. and  Olivas, A. 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. Perez and  Peters, L. and  Peterson, J. and  Philippen, S. and  Pieloth, D. and  Pieper, S. and  Pittermann, M. and  Pizzuto, A. and  Plum, M. and  Popovych, Y. and Porcelli, Alessio and  Rodriguez, M. Prado and  Price, P. B. and  Pries, B. and  Przybylski, G. T. and  Raab, C. and  Raissi, A. and  Rameez, M. and  Rawlins, K. and  Rea, I. C. and  Rehman, A. and  Reichherzer, P. and  Reimann, R. 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  Roellinghoff, G. and  Rongen, M. and  Rott, C. and  Ruhe, T. and Ryckbosch, Dirk and  Cantu, D. Rysewyk and  Safa, I. and  Saffer, J. and  Herrera, S. E. Sanchez and  Sandrock, A. and  Sandroos, J. and  Santander, M. and  Sarkar, S. and  Sarkar, S. and  Satalecka, K. and  Scharf, M. and  Schaufel, M. and  Schieler, H. and  Schindler, S. and  Schlunder, P. and  Schmidt, T. and  Schneider, A. and  Schneider, J. and  Schroder, F. G. and  Schumacher, L. and  Schwefer, G. and  Sclafani, S. and  Seckel, D. and  Seunarine, S. and  Sharma, A. and  Shefali, S. and  Silva, M. and  Skrzypek, B. and  Smithers, B. and  Snihur, R. and  Soedingrekso, J. and  Soldin, D. and  Spannfellner, C. and  Spiczak, G. M. and  Spiering, C. and  Stachurska, J. and  Stamatikos, M. and  Stanev, T. and  Stein, R. and  Stettner, J. and  Steuer, A. and  Stezelberger, T. and  Sturwald, T. and  Stuttard, T. and  Sullivan, G. W. and  Taboada, I. and  Tenholt, F. and  Ter-Antonyan, S. and  Tilav, S. and  Tischbein, F. and  Tollefson, K. and  Tomankova, L. and  Tonnis, C. and  Toscano, S. and  Tosi, D. and  Trettin, A. and  Tselengidou, M. and  Tung, C. F. and  Turcati, A. and  Turcotte, R. and  Turley, C. F. and  Twagirayezu, J. P. and  Ty, B. and  Elorrieta, M. A. Unland and  Valtonen-Mattila, N. and  Vandenbroucke, J. and  van Eijndhoven, N. and  Vannerom, D. and  van Santen, J. and Verpoest, Stef and Vraeghe, Matthias and  Walck, C. and  Watson, T. B. and  Weaver, C. and  Weigel, P. and  Weindl, A. and  Weiss, M. J. and  Weldert, J. and  Wendt, C. and  Werthebach, J. and  Weyrauch, M. and  Whitehorn, N. and  Wiebusch, C. H. and  Williams, D. R. and  Wolf, M. and  Woschnagg, K. and  Wrede, G. and  Wulff, J. and  Xu, X. W. and  Xu, Y. and  Yanez, J. P. and  Yoshida, S. and  Yu, S. and  Yuan, T. and Zhang, Z. and on behalf of the IceCube Collaboration, [ missing ]}},
  booktitle    = {{37TH INTERNATIONAL COSMIC RAY CONFERENCE, ICRC2021}},
  language     = {{eng}},
  location     = {{Berlin}},
  pages        = {{11}},
  title        = {{Testing the AGN radio and neutrino correlation using the MOJAVE catalog and 10 years of IceCube data}},
  year         = {{2022}},
}

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