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The contribution of Fermi-2LAC blazars to the diffuse TeV-PeV neutrino
flux [PDF]
, 2016 The recent discovery of a diffuse cosmic neutrino flux extending up to PeV
energies raises the question of which astrophysical sources generate this
signal. One class of extragalactic sources which may produce such high-energy
neutrinos are blazars.Aartsen, M. G., Abraham, K., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Ahrens, M., Altmann, D., Andeen, K., Anderson, T., Ansseau, I., Anton, G., Archinger, M., Arguelles, C., Argüelles, C., Arlen, T. C., Auffenberg, J., Axani, S., Bai, X., Barwick, S. W., Baum, V., Bay, R., Beatty, J. J., Becker, K. -H., BenZvi, S., Berghaus, P., Berley, D., Bernardini, E., Bernhard, A., Besson, D. Z., Binder, G., Bindig, D., Bissok, M., Blaufuss, E., Blot, S., Boersma, D. J., Bohm, C., Bos, F., Bose, D., Botner, O., Braun, J., Brayeur, L., Bretz, Hans-Peter, Burgman, A., Börner, M., Böser, S., Casey, J., Casier, M., Cheung, E., Chirkin, D., Christov, A., Clark, K., Classen, L., Coenders, S., Collin, G. H., Conrad, J. M., Cowen, D. F., Daughhetee, J., Davis, J. C., Day, M., de André, J. P. A. M., De Clercq, C., De Ridder, S., de Vries, K. D., de Wasseige, G., de With, M., Dembinski, H., Desiati, P., DeYoung, T., di Lorenzo, V., Dujmovic, H., Dumm, J. P., Dunkman, M., Díaz-Vélez, J. C., Eberhardt, B., Ehrhardt, T., Eichmann, B., Euler, S., Evenson, P. A., Fahey, S., Fazely, A. R., Feintzeig, J., Felde, J., Filimonov, K., Finley, C., Flis, S., Franckowiak, A., Fuchs, T., Fösig, C. -C., Gaior, R., Gaisser, T. K., Gallagher, J., Gerhardt, L., Ghorbani, K., Giang, W., Gladstone, L., Glagla, M., Glüsenkamp, T., Goldschmidt, A., Golup, G., Gonzalez, J. G., Grant, D., Griffith, Z., Góra, D., Haack, C., Hallgren, A., Halzen, F., Hansen, E., Hansmann, B., Hansmann, T., Hanson, K., Hebecker, D., Heereman, D., Helbing, K., Hellauer, R., Heros, C. Pérez de los, Herrera, S. E. Sanchez, Hickford, S., Hignight, J., Hill, G. C., Hoffman, K. D., Hoffmann, R., Holzapfel, K., Homeier, A., Hoshina, K., Huang, F., Huber, M., Huelsnitz, W., Hultqvist, K., IceCube Collaboration, IceCube Collaboration, In, S., Ishihara, A., Ismail, A. Haj, Jacobi, E., Japaridze, G. S., Jeong, M., Jero, K., Jones, B. J. P., Jurkovic, M., Kappes, A., Karg, T., Karle, A., Katz, U., Kauer, M., Keivani, A., Kelley, J. L., Kemp, J., Kheirandish, A., Kim, M., Kintscher, T., Kiryluk, J., Kittler, T., Klein, S. R., Kohnen, G., Koirala, R., Kolanoski, H., Konietz, R., Kopper, C., Kopper, S., Koskinen, D. J., Kowalski, M., Krings, K., Kroll, M., Krückl, G., Krüger, C., Kunnen, J., Kunwar, S., Kurahashi, N., Kuwabara, T., Köpke, L., Labare, M., Lanfranchi, J. L., Larson, M. J., Lennarz, D., Lesiak-Bzdak, M., Leuermann, M., Leuner, J., Lu, L., Lünemann, J., Madsen, J., Maggi, G., Mahn, K. B. M., Mancina, S., Mandelartz, M., Maruyama, R., Mase, K., Maunu, R., McNally, F., Meagher, K., Medici, M., Meier, M., Meli, A., Menne, T., Merino, G., Meures, T., Miarecki, S., Middell, E., Mohrmann, L., Montaruli, T., Moulai, M., Nahnhauer, R., Naumann, U., Neer, G., Niederhausen, H., Nowicki, S. C., Nygren, D. R., O'Murchadha, A., Olivas, A., Omairat, A., Palczewski, T., Pandya, H., Pankova, D. V., Penek, Ö., Pepper, J. A., Pfendner, C., Pieloth, D., Pinat, E., Pollmann, A. Obertacke, Posselt, J., Price, P. B., Przybylski, G. T., Quinnan, M., Raab, C., Rameez, M., Rawlins, K., Reimann, R., Relich, M., Resconi, E., Rhode, W., Richman, M., Riedel, B., Robertson, S., Rongen, M., Rosendo, E. del Pino, Rott, C., Ruhe, T., Ryckbosch, D., Rysewyk, D., Rädel, L., Sabbatini, L., Sandrock, A., Sandroos, J., Sarkar, S., Satalecka, K., Schimp, M., Schlunder, P., Schmidt, T., Schoenen, S., Schumacher, L., Schöneberg, S., Schönwald, A., Seckel, D., Seunarine, S., Silva, A. H. Cruz, Soldin, D., Song, M., Spiczak, G. M., Spiering, C., Stahlberg, M., Stamatikos, M., Stanev, T., Stasik, A., Steuer, A., Stezelberger, T., Stokstad, R. G., Strotjohann, N. L., Ström, R., Stößl, A., Sullivan, G. W., Sutherland, M., Taavola, H., Taboada, I., Tatar, J., Ter-Antonyan, S., Terliuk, A., Tešić, G., Tilav, S., Tjus, J. Becker, Toale, P. A., Tobin, M. N., Toscano, S., Tosi, D., Tselengidou, M., Turcati, A., Unger, E., Usner, M., Vallecorsa, S., van Eijndhoven, N., van Rossem, M., van Santen, J., Vandenbroucke, J., Vanheule, S., Veenkamp, J., Vehring, M., Voge, M., Vraeghe, M., Walck, C., Wallace, A., Wallraff, M., Wandkowsky, N., Weaver, Ch., Wendt, C., Westerhoff, S., Whelan, B. J., Wickmann, S., Wiebe, K., Wiebusch, C. H., Wille, L., Williams, D. R., Wills, L., Wissing, H., Wolf, M., Wood, T. R., Woolsey, E., Woschnagg, K., Xu, D. L., Xu, X. W., Xu, Y., Yanez, J. P., Yodh, G., Yoshida, S., Zoll, M. +322 morecore +5 more sourcesA tool to understand emission mechanisms of blazars through their high‐energy gamma‐ray emission [PDF]
Astronomische Nachrichten, Volume 344, Issue 6, August 2023., 2023 The blazar SED is characterized by two energy components. Evidence suggests that the low‐energy component is generated by the synchrotron mechanism, but for the high‐energy component, the mechanism is still uncertain. Two main models have been proposed to explain this emission. According to the leptonic model, a correlation between the emission of both Mabel Osorio, Erick Rangel, J. R. Sacahui, M. M. González +3 moreopenalex +2 more sourcesThe space density of z>4 blazars [PDF]
Monthly notices of the Royal Astronomical Society, 2019 High redshift blazars are an important class of Active Galactic Nuclei (AGN)
that can provide an independent estimate of the supermassive black-hole mass
function in high redshift radio-loud AGN without the bias due to absorption
along the line-of-sight. Antón, Sonia, Ballo, Lucia, Belladitta, Silvia, Caccianiga, Alessandro, Cicone, Claudia, Dallacasa, Daniele, Della Ceca, Roberto, Gargiulo, Adriana, Ighina, Luca, Marchã, Maria J., Moretti, Alberto, Severgnini, Paola +11 morecore +4 more sourcesSearches for Neutrinos in the Direction of Radio-bright Blazars with the ANTARES Telescope [PDF]
Astrophysical Journal, 2023 Active galaxies, especially blazars, are among the most promising extragalactic candidates for high-energy neutrino sources. To date, ANTARES searches included these objects and used GeV–TeV γ-ray flux to select blazars.A. Albert, S. Alves, M. Andr'e, M. Ardid, S. Ardid, J. Aubert, J. Aublin, B. Baret, S. Basa, Y. Becherini, B. Belhorma, M. Bendahman, F. Benfenati, V. Bertin, S. Biagi, M. Bissinger, J. Boumaaza, M. Bouta, M. Bouwhuis, H. Branzacs, R. Bruijn, J. Brunner, J. Busto, B. Caiffi, D. Calvo, S. Campion, A. Capone, L. Caramete, F. Carenini, J. Carr, V. Carretero, S. Celli, L. Cerisy, M. Chabab, R. Moursli, T. Chiarusi, M. Circella, J. Coelho, A. Coleiro, R. Coniglione, P. Coyle, A. Creusot, A. Cruz, A. D'iaz, B. Martino, C. Distefano, I. D. Palma, A. Domi, C. Donzaud, D. Dornic, D. Drouhin, T. Eberl, T. V. Eeden, D. V. Eijk, S. Hedri, N. Khayati, A. Enzenhofer, P. Fermani, G. Ferrara, F. Filippini, L. Fusco, S. Gagliardini, J. Antonio García, C. G. Oliver, P. Gay, N. Geißelbrecht, H. Glotin, R. Gozzini, R. G. Ruiz, K. Graf, C. Guidi, L. Haegel, S. Hallmann, H. Haren, A. Heijboer, Y. Hello, J. J. Hern'andez-Rey, J. Hossl, J. Hofestadt, F. Huang, G. Illuminati, Curtis N. James, B. Jisse-Jung, M. Jong, P. Jong, M. Kadler, O. Kalekin, U. Katz, A. Kouchner, Y. Kovalev, Y. Kovalev, I. Kreykenbohm, V. Kulikovskiy, R. Lahmann, M. Lamoureux, A. Lazo, D. Lefèvre, E. Leonora, G. Levi, S. L. Stum, D. López-Coto, S. Loucatos, L. Maderer, J. Manczak, M. Marcelin, A. Margiotta, A. Marinelli, J. A. Mart'inez-Mora, P. Migliozzi, A. Moussa, R. Muller, S. Navas, E. Nezri, B. Fearraigh, E. Oukacha, A. Puaun, G. E. Puavualacs, S. Pena-Mart'inez, M. Perrin-Terrin, V. Pestel, P. Piattelli, A. Plavin, C. Poirè, V. Popa, T. Pradier, A. Pushkarev, N. Randazzo, D. Real, S. Reck, G. Riccobene, A. Romanov, A. S'anchez-Losa, A. Saina, F. Greus, D. Samtleben, M. Sanguineti, P. Sapienza, J. Schnabel, J. Schumann, F. Schussler, J. Seneca, M. Spurio, T. Stolarczyk, M. Taiuti, Y. Tayalati, S. Tingay, S. Troitsky, B. Vallage, G. Vannoye, V. Elewyck, S. Viola, D. Vivolo, J. Wilms, S. Zavatarelli, A. Zegarelli, J. Zornoza, J. Z'uniga, O. C. T. Hovatta, S. Kiehlmann, I. Liodakis, V. Pavlidou, A. Readhead +161 moresemanticscholar +1 more sourceKinematics of Parsec-scale Jets of Gamma-Ray Blazars at 43 GHz during 10 yr of the VLBA-BU-BLAZAR Program [PDF]
Astrophysical Journal Supplement Series, 2022 We analyze the parsec-scale jet kinematics from 2007 June to 2018 December of a sample of γ-ray bright blazars monitored roughly monthly with the Very Long Baseline Array (VLBA) at 43 GHz under the VLBA-BU-BLAZAR program.Z. Weaver, S. Jorstad, A. Marscher, D. Morozova, I. Troitsky, I. Agudo, J. L. G'omez, A. Lähteenmäki, J. Tammi, M. Tornikoski +9 moresemanticscholar +1 more sourceBASS. XXXIII. Swift-BAT Blazars and Their Jets through Cosmic Time [PDF]
Astrophysical Journal, 2022 We derive the most up-to-date Swift-Burst Alert Telescope (BAT) blazar luminosity function in the 14–195 keV range, making use of a clean sample of 118 blazars detected in the BAT 105 month survey catalog, with newly obtained redshifts from the BAT ...L. Marcotulli, M. Ajello, C. M. Urry, V. Paliya, M. Koss, K. Oh, G. Madejski, Y. Ueda, M. Balokovi'c, B. Trakhtenbrot, F. Ricci, C. Ricci, D. Stern, F. Harrison, M. Powell, Bass Collaboration +15 moresemanticscholar +1 more source
