@article{8757265,
  abstract     = {{Ultraluminous infrared galaxies (ULIRGs) have infrared luminosities L-IR >= 10(12) L-circle dot, making them the most luminous objects in the infrared sky. These dusty objects are generally powered by starbursts with star formation rates that exceed 100M(circle dot) yr(-1), possibly combined with a contribution from an active galactic nucleus. Such environments make ULIRGs plausible sources of astrophysical high-energy neutrinos, which can be observed by the IceCube Neutrino Observatory at the South Pole. We present a stacking search for high-energy neutrinos from a representative sample of 75 ULIRGs with redshift z <= 0.13 using 7.5 yr of IceCube data. The results are consistent with a background-only observation, yielding upper limits on the neutrino flux from these 75 ULIRGs. For an unbroken E-2.5 power-law spectrum, we report an upper limit on the stacked flux Phi(90%)(nu mu+(nu) over bar mu) = 3.24 x 10(-14) TeV-1 cm(-2) S-1 (E/10 TeV)(-2.5) at 90% confidence level. In addition, we constrain the contribution of the ULIRG source population to the observed diffuse astrophysical neutrino flux as well as model predictions.}},
  articleno    = {{59}},
  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., Jr. 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., V 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 Boettcher, 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 Fuerst, 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 Gluesenkamp, 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 Ha Minh, M. 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 Koepke, 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 Li, Y. and Lincetto, M. and Leszczynska, A. 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 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.}},
  issn         = {{0004-637X}},
  journal      = {{ASTROPHYSICAL JOURNAL}},
  keywords     = {{ACTIVE GALACTIC NUCLEI,STAR-FORMATION HISTORY,LUMINOSITY FUNCTIONS,OPTICAL SPECTROSCOPY,JY SAMPLE,AGN,EVOLUTION,FLUX,STARBURST,TELESCOPE}},
  language     = {{eng}},
  number       = {{1}},
  pages        = {{15}},
  title        = {{Search for high-energy neutrinos from ultraluminous infrared galaxies with IceCube}},
  url          = {{http://doi.org/10.3847/1538-4357/ac3cb6}},
  volume       = {{926}},
  year         = {{2022}},
}

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