318 results on '"Larionova L."'
Search Results
102. Variability of the blazar 4C 38.41 (B3 1633+382) from GHz frequencies to GeV energies
- Author
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Raiteri, C. M., primary, Villata, M., additional, Smith, P. S., additional, Larionov, V. M., additional, Acosta-Pulido, J. A., additional, Aller, M. F., additional, D’Ammando, F., additional, Gurwell, M. A., additional, Jorstad, S. G., additional, Joshi, M., additional, Kurtanidze, O. M., additional, Lähteenmäki, A., additional, Mirzaqulov, D. O., additional, Agudo, I., additional, Aller, H. D., additional, Arévalo, M. J., additional, Arkharov, A. A., additional, Bach, U., additional, Benítez, E., additional, Berdyugin, A., additional, Blinov, D. A., additional, Blumenthal, K., additional, Buemi, C. S., additional, Bueno, A., additional, Carleton, T. M., additional, Carnerero, M. I., additional, Carosati, D., additional, Casadio, C., additional, Chen, W. P., additional, Di Paola, A., additional, Dolci, M., additional, Efimova, N. V., additional, Ehgamberdiev, Sh. A., additional, Gómez, J. L., additional, González, A. I., additional, Hagen-Thorn, V. A., additional, Heidt, J., additional, Hiriart, D., additional, Holikov, Sh., additional, Konstantinova, T. S., additional, Kopatskaya, E. N., additional, Koptelova, E., additional, Kurtanidze, S. O., additional, Larionova, E. G., additional, Larionova, L. V., additional, León-Tavares, J., additional, Leto, P., additional, Lin, H. C., additional, Lindfors, E., additional, Marscher, A. P., additional, McHardy, I. M., additional, Molina, S. N., additional, Morozova, D. A., additional, Mujica, R., additional, Nikolashvili, M. G., additional, Nilsson, K., additional, Ovcharov, E. P., additional, Panwar, N., additional, Pasanen, M., additional, Puerto-Gimenez, I., additional, Reinthal, R., additional, Richter, G. M., additional, Ros, J. A., additional, Sakamoto, T., additional, Schwartz, R. D., additional, Sillanpää, A., additional, Smith, N., additional, Takalo, L. O., additional, Tammi, J., additional, Taylor, B., additional, Thum, C., additional, Tornikoski, M., additional, Trigilio, C., additional, Troitsky, I. S., additional, Umana, G., additional, Valcheva, A. T., additional, and Wehrle, A. E., additional
- Published
- 2012
- Full Text
- View/download PDF
103. THE STRUCTURE AND EMISSION MODEL OF THE RELATIVISTIC JET IN THE QUASAR 3C 279 INFERRED FROM RADIO TO HIGH-ENERGY γ-RAY OBSERVATIONS IN 2008-2010
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Hayashida, M., primary, Madejski, G. M., additional, Nalewajko, K., additional, Sikora, M., additional, Wehrle, A. E., additional, Ogle, P., additional, Collmar, W., additional, Larsson, S., additional, Fukazawa, Y., additional, Itoh, R., additional, Chiang, J., additional, Stawarz, Ł., additional, Blandford, R. D., additional, Richards, J. L., additional, Max-Moerbeck, W., additional, Readhead, A., additional, Buehler, R., additional, Cavazzuti, E., additional, Ciprini, S., additional, Gehrels, N., additional, Reimer, A., additional, Szostek, A., additional, Tanaka, T., additional, Tosti, G., additional, Uchiyama, Y., additional, Kawabata, K. S., additional, Kino, M., additional, Sakimoto, K., additional, Sasada, M., additional, Sato, S., additional, Uemura, M., additional, Yamanaka, M., additional, Greiner, J., additional, Kruehler, T., additional, Rossi, A., additional, Macquart, J. P., additional, Bock, D. C.-J., additional, Villata, M., additional, Raiteri, C. M., additional, Agudo, I., additional, Aller, H. D., additional, Aller, M. F., additional, Arkharov, A. A., additional, Bach, U., additional, Benítez, E., additional, Berdyugin, A., additional, Blinov, D. A., additional, Blumenthal, K., additional, Böttcher, M., additional, Buemi, C. S., additional, Carosati, D., additional, Chen, W. P., additional, Paola, A. Di, additional, Dolci, M., additional, Efimova, N. V., additional, Forné, E., additional, Gómez, J. L., additional, Gurwell, M. A., additional, Heidt, J., additional, Hiriart, D., additional, Jordan, B., additional, Jorstad, S. G., additional, Joshi, M., additional, Kimeridze, G., additional, Konstantinova, T. S., additional, Kopatskaya, E. N., additional, Koptelova, E., additional, Kurtanidze, O. M., additional, Lähteenmäki, A., additional, Lamerato, A., additional, Larionov, V. M., additional, Larionova, E. G., additional, Larionova, L. V., additional, Leto, P., additional, Lindfors, E., additional, Marscher, A. P., additional, McHardy, I. M., additional, Molina, S. N., additional, Morozova, D. A., additional, Nikolashvili, M. G., additional, Nilsson, K., additional, Reinthal, R., additional, Roustazadeh, P., additional, Sakamoto, T., additional, Sigua, L. A., additional, Sillanpää, A., additional, Takalo, L., additional, Tammi, J., additional, Taylor, B., additional, Tornikoski, M., additional, Trigilio, C., additional, Troitsky, I. S., additional, and Umana, G., additional
- Published
- 2012
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104. The long-lasting activity of 3C 454.3
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Raiteri, C. M., primary, Villata, M., additional, Aller, M. F., additional, Gurwell, M. A., additional, Kurtanidze, O. M., additional, Lähteenmäki, A., additional, Larionov, V. M., additional, Romano, P., additional, Vercellone, S., additional, Agudo, I., additional, Aller, H. D., additional, Arkharov, A. A., additional, Bach, U., additional, Benítez, E., additional, Berdyugin, A., additional, Blinov, D. A., additional, Borisova, E. V., additional, Böttcher, M., additional, Bravo Calle, O. J. A., additional, Buemi, C. S., additional, Calcidese, P., additional, Carosati, D., additional, Casas, R., additional, Chen, W.-P., additional, Efimova, N. V., additional, Gómez, J. L., additional, Gusbar, C., additional, Hawkins, K., additional, Heidt, J., additional, Hiriart, D., additional, Hsiao, H. Y., additional, Jordan, B., additional, Jorstad, S. G., additional, Joshi, M., additional, Kimeridze, G. N., additional, Koptelova, E., additional, Konstantinova, T. S., additional, Kopatskaya, E. N., additional, Kurtanidze, S. O., additional, Larionova, E. G., additional, Larionova, L. V., additional, Leto, P., additional, Li, Y., additional, Ligustri, R., additional, Lindfors, E., additional, Lister, M., additional, Marscher, A. P., additional, Molina, S. N., additional, Morozova, D. A., additional, Nieppola, E., additional, Nikolashvili, M. G., additional, Nilsson, K., additional, Palma, N., additional, Pasanen, M., additional, Reinthal, R., additional, Roberts, V., additional, Ros, J. A., additional, Roustazadeh, P., additional, Sadun, A. C., additional, Sakamoto, T., additional, Schwartz, R. D., additional, Sigua, L. A., additional, Sillanpää, A., additional, Takalo, L. O., additional, Tammi, J., additional, Taylor, B., additional, Tornikoski, M., additional, Trigilio, C., additional, Troitsky, I. S., additional, Umana, G., additional, Volvach, A., additional, and Yuldasheva, T. A., additional
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- 2011
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105. Identification ofγ-ray emission from 3C 345 and NRAO 512
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Schinzel, F. K., primary, Sokolovsky, K. V., additional, D’Ammando, F., additional, Burnett, T. H., additional, Max-Moerbeck, W., additional, Cheung, C. C., additional, Fegan, S. J., additional, Casandjian, J. M., additional, Reyes, L. C., additional, Villata, M., additional, Raiteri, C. M., additional, Agudo, I., additional, Bravo Calle, O. J. A., additional, Carosati, D., additional, Casas, R., additional, Gómez, J. L., additional, Gurwell, M. A., additional, Hsiao, H. Y., additional, Jorstad, S. G., additional, Kimeridze, G., additional, Konstantinova, T. S., additional, Kopatskaya, E. N., additional, Koptelova, E., additional, Kurtanidze, O. M., additional, Kurtanidze, S. O., additional, Larionov, V. M., additional, Larionova, E. G., additional, Larionova, L. V., additional, Marscher, A. P., additional, Morozova, D. A., additional, Nikolashvili, M. G., additional, Roca-Sogorb, M., additional, Ros, J. A., additional, Sigua, L. A., additional, Spiridonova, O., additional, Troitsky, I. S., additional, Vlasyuk, V. V., additional, Lobanov, A. P., additional, and Zensus, J. A., additional
- Published
- 2011
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106. FERMILARGE AREA TELESCOPE AND MULTI-WAVELENGTH OBSERVATIONS OF THE FLARING ACTIVITY OF PKS 1510-089 BETWEEN 2008 SEPTEMBER AND 2009 JUNE
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Abdo, A. A., primary, Ackermann, M., additional, Agudo, I., additional, Ajello, M., additional, Allafort, A., additional, Aller, H. D., additional, Aller, M. F., additional, Antolini, E., additional, Arkharov, A. A., additional, Axelsson, M., additional, Bach, U., additional, Baldini, L., additional, Ballet, J., additional, Barbiellini, G., additional, Bastieri, D., additional, Bechtol, K., additional, Bellazzini, R., additional, Berdyugin, A., additional, Berenji, B., additional, Blandford, R. D., additional, Blinov, D. A., additional, Bloom, E. D., additional, Boettcher, M., additional, Bonamente, E., additional, Borgland, A. W., additional, Bouvier, A., additional, Bregeon, J., additional, Brez, A., additional, Brigida, M., additional, Bruel, P., additional, Buehler, R., additional, Buemi, C. S., additional, Burnett, T. H., additional, Buson, S., additional, Caliandro, G. A., additional, Cameron, R. A., additional, Caraveo, P. A., additional, Carosati, D., additional, Carrigan, S., additional, Casandjian, J. M., additional, Cavazzuti, E., additional, Cecchi, C., additional, Çelik, Ö., additional, Chekhtman, A., additional, Chen, W. P., additional, Cheung, C. C., additional, Chiang, J., additional, Ciprini, S., additional, Claus, R., additional, Cohen-Tanugi, J., additional, Conrad, J., additional, Corbel, S., additional, Costamante, L., additional, Dermer, C. D., additional, de Angelis, A., additional, de Palma, F., additional, Donato, D., additional, do Couto e Silva, E., additional, Drell, P. S., additional, Dubois, R., additional, Dumora, D., additional, Farnier, C., additional, Favuzzi, C., additional, Fegan, S. J., additional, Ferrara, E. C., additional, Focke, W. B., additional, Forné, E., additional, Fortin, P., additional, Fukazawa, Y., additional, Funk, S., additional, Fusco, P., additional, Gargano, F., additional, Gasparrini, D., additional, Gehrels, N., additional, Germani, S., additional, Giebels, B., additional, Giglietto, N., additional, Giordano, F., additional, Giroletti, M., additional, Glanzman, T., additional, Godfrey, G., additional, Grenier, I. A., additional, Grove, J. E., additional, Guiriec, S., additional, Gurwell, M. A., additional, Gusbar, C., additional, Gómez, J. L., additional, Hadasch, D., additional, Hagen-Thorn, V. A., additional, Hayashida, M., additional, Hays, E., additional, Horan, D., additional, Hughes, R. E., additional, Jóhannesson, G., additional, Johnson, A. S., additional, Johnson, W. N., additional, Kamae, T., additional, Katagiri, H., additional, Kataoka, J., additional, Kawai, N., additional, Kimeridze, G., additional, Knödlseder, J., additional, Konstantinova, T. S., additional, Kopatskaya, E. N., additional, Koptelova, E., additional, Kovalev, Y. Y., additional, Kurtanidze, O. M., additional, Kuss, M., additional, Lahteenmaki, A., additional, Lande, J., additional, Larionov, V. M., additional, Larionova, E. G., additional, Larionova, L. V., additional, Larsson, S., additional, Latronico, L., additional, Lee, S.-H., additional, Leto, P., additional, Lister, M. L., additional, Longo, F., additional, Loparco, F., additional, Lott, B., additional, Lovellette, M. N., additional, Lubrano, P., additional, Madejski, G. M., additional, Makeev, A., additional, Massaro, E., additional, Mazziotta, M. N., additional, McConville, W., additional, McEnery, J. E., additional, McHardy, I. M., additional, Michelson, P. F., additional, Mitthumsiri, W., additional, Mizuno, T., additional, Moiseev, A. A., additional, Monte, C., additional, Monzani, M. E., additional, Morozova, D. A., additional, Morselli, A., additional, Moskalenko, I. V., additional, Murgia, S., additional, Naumann-Godo, M., additional, Nikolashvili, M. G., additional, Nolan, P. L., additional, Norris, J. P., additional, Nuss, E., additional, Ohno, M., additional, Ohsugi, T., additional, Okumura, A., additional, Omodei, N., additional, Orlando, E., additional, Ormes, J. F., additional, Ozaki, M., additional, Paneque, D., additional, Panetta, J. H., additional, Parent, D., additional, Pasanen, M., additional, Pelassa, V., additional, Pepe, M., additional, Pesce-Rollins, M., additional, Piron, F., additional, Porter, T. A., additional, Pushkarev, A. B., additional, Rainò, S., additional, Raiteri, C. M., additional, Rando, R., additional, Razzano, M., additional, Reimer, A., additional, Reimer, O., additional, Reinthal, R., additional, Ripken, J., additional, Ritz, S., additional, Roca-Sogorb, M., additional, Rodriguez, A. Y., additional, Roth, M., additional, Roustazadeh, P., additional, Ryde, F., additional, Sadrozinski, H. F.-W., additional, Sander, A., additional, Scargle, J. D., additional, Sgrò, C., additional, Sigua, L. A., additional, Smith, P. D., additional, Sokolovsky, K., additional, Spandre, G., additional, Spinelli, P., additional, Starck, J.-L., additional, Strickman, M. S., additional, Suson, D. J., additional, Takahashi, H., additional, Takahashi, T., additional, Takalo, L. O., additional, Tanaka, T., additional, Taylor, B., additional, Thayer, J. B., additional, Thayer, J. G., additional, Thompson, D. J., additional, Tibaldo, L., additional, Tornikoski, M., additional, Torres, D. F., additional, Tosti, G., additional, Tramacere, A., additional, Trigilio, C., additional, Troitsky, I. S., additional, Umana, G., additional, Usher, T. L., additional, Vandenbroucke, J., additional, Vasileiou, V., additional, Vilchez, N., additional, Villata, M., additional, Vitale, V., additional, Waite, A. P., additional, Wang, P., additional, Winer, B. L., additional, Wood, K. S., additional, Yang, Z., additional, Ylinen, T., additional, and Ziegler, M., additional
- Published
- 2010
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107. WEBT multiwavelength monitoring and XMM-Newton observations of BL Lacertae in 2007–2008
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Raiteri, C. M., primary, Villata, M., additional, Capetti, A., additional, Aller, M. F., additional, Bach, U., additional, Calcidese, P., additional, Gurwell, M. A., additional, Larionov, V. M., additional, Ohlert, J., additional, Nilsson, K., additional, Strigachev, A., additional, Agudo, I., additional, Aller, H. D., additional, Bachev, R., additional, Benítez, E., additional, Berdyugin, A., additional, Böttcher, M., additional, Buemi, C. S., additional, Buttiglione, S., additional, Carosati, D., additional, Charlot, P., additional, Chen, W. P., additional, Dultzin, D., additional, Forné, E., additional, Fuhrmann, L., additional, Gómez, J. L., additional, Gupta, A. C., additional, Heidt, J., additional, Hiriart, D., additional, Hsiao, W.-S., additional, Jelínek, M., additional, Jorstad, S. G., additional, Kimeridze, G. N., additional, Konstantinova, T. S., additional, Kopatskaya, E. N., additional, Kostov, A., additional, Kurtanidze, O. M., additional, Lähteenmäki, A., additional, Lanteri, L., additional, Larionova, L. V., additional, Leto, P., additional, Latev, G., additional, Le Campion, J.-F., additional, Lee, C.-U., additional, Ligustri, R., additional, Lindfors, E., additional, Marscher, A. P., additional, Mihov, B., additional, Nikolashvili, M. G., additional, Nikolov, Y., additional, Ovcharov, E., additional, Principe, D., additional, Pursimo, T., additional, Ragozzine, B., additional, Robb, R. M., additional, Ros, J. A., additional, Sadun, A. C., additional, Sagar, R., additional, Semkov, E., additional, Sigua, L. A., additional, Smart, R. L., additional, Sorcia, M., additional, Takalo, L. O., additional, Tornikoski, M., additional, Trigilio, C., additional, Uckert, K., additional, Umana, G., additional, Valcheva, A., additional, and Volvach, A., additional
- Published
- 2009
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108. The correlated optical and radio variability of BL Lacertae
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Villata, M., primary, Raiteri, C. M., additional, Larionov, V. M., additional, Nikolashvili, M. G., additional, Aller, M. F., additional, Bach, U., additional, Carosati, D., additional, Hroch, F., additional, Ibrahimov, M. A., additional, Jorstad, S. G., additional, Kovalev, Y. Y., additional, Lähteenmäki, A., additional, Nilsson, K., additional, Teräsranta, H., additional, Tosti, G., additional, Aller, H. D., additional, Arkharov, A. A., additional, Berdyugin, A., additional, Boltwood, P., additional, Buemi, C. S., additional, Casas, R., additional, Charlot, P., additional, Coloma, J. M., additional, Di Paola, A., additional, Di Rico, G., additional, Kimeridze, G. N., additional, Konstantinova, T. S., additional, Kopatskaya, E. N., additional, Kovalev, Yu. A., additional, Kurtanidze, O. M., additional, Lanteri, L., additional, Larionova, E. G., additional, Larionova, L. V., additional, Le Campion, J.-F., additional, Leto, P., additional, Lindfors, E., additional, Marscher, A. P., additional, Marshall, K., additional, McFarland, J. P., additional, McHardy, I. M., additional, Miller, H. R., additional, Nucciarelli, G., additional, Osterman, M. P., additional, Pasanen, M., additional, Pursimo, T., additional, Ros, J. A., additional, Sadun, A. C., additional, Sigua, L. A., additional, Sixtova, L., additional, Takalo, L. O., additional, Tornikoski, M., additional, Trigilio, C., additional, Umana, G., additional, Xie, G. Z., additional, Zhang, X., additional, and Zhou, S. B., additional
- Published
- 2009
- Full Text
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109. Results of WEBT, VLBA and RXTE monitoring of 3C 279 during 2006–2007
- Author
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Larionov, V. M., primary, Jorstad, S. G., additional, Marscher, A. P., additional, Raiteri, C. M., additional, Villata, M., additional, Agudo, I., additional, Aller, M. F., additional, Arkharov, A. A., additional, Asfandiyarov, I. M., additional, Bach, U., additional, Bachev, R., additional, Berdyugin, A., additional, Böttcher, M., additional, Buemi, C. S., additional, Calcidese, P., additional, Carosati, D., additional, Charlot, P., additional, Chen, W.-P., additional, Di Paola, A., additional, Dolci, M., additional, Dogru, S., additional, Doroshenko, V. T., additional, Efimov, Yu. S., additional, Erdem, A., additional, Frasca, A., additional, Fuhrmann, L., additional, Giommi, P., additional, Glowienka, L., additional, Gupta, A. C., additional, Gurwell, M. A., additional, Hagen-Thorn, V. A., additional, Hsiao, W.-S., additional, Ibrahimov, M. A., additional, Jordan, B., additional, Kamada, M., additional, Konstantinova, T. S., additional, Kopatskaya, E. N., additional, Kovalev, Y. Y., additional, Kovalev, Y. A., additional, Kurtanidze, O. M., additional, Lähteenmäki, A., additional, Lanteri, L., additional, Larionova, L. V., additional, Leto, P., additional, Le Campion, P., additional, Lee, C.-U., additional, Lindfors, E., additional, Marilli, E., additional, McHardy, I., additional, Mingaliev, M. G., additional, Nazarov, S. V., additional, Nieppola, E., additional, Nilsson, K., additional, Ohlert, J., additional, Pasanen, M., additional, Porter, D., additional, Pursimo, T., additional, Ros, J. A., additional, Sadakane, K., additional, Sadun, A. C., additional, Sergeev, S. G., additional, Smith, N., additional, Strigachev, A., additional, Sumitomo, N., additional, Takalo, L. O., additional, Tanaka, K., additional, Trigilio, C., additional, Umana, G., additional, Ungerechts, H., additional, Volvach, A., additional, and Yuan, W., additional
- Published
- 2008
- Full Text
- View/download PDF
110. Radio-to-UV monitoring of AO 0235+164 by the WEBT and Swift during the 2006–2007 outburst
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Raiteri, C. M., primary, Villata, M., additional, Larionov, V. M., additional, Aller, M. F., additional, Bach, U., additional, Gurwell, M., additional, Kurtanidze, O. M., additional, Lähteenmäki, A., additional, Nilsson, K., additional, Volvach, A., additional, Aller, H. D., additional, Arkharov, A. A., additional, Bachev, R., additional, Berdyugin, A., additional, Böttcher, M., additional, Buemi, C. S., additional, Calcidese, P., additional, Cozzi, E., additional, Di Paola, A., additional, Dolci, M., additional, Fan, J. H., additional, Forné, E., additional, Foschini, L., additional, Gupta, A. C., additional, Hagen-Thorn, V. A., additional, Hooks, L., additional, Hovatta, T., additional, Joshi, M., additional, Kadler, M., additional, Kimeridze, G. N., additional, Konstantinova, T. S., additional, Kostov, A., additional, Krichbaum, T. P., additional, Lanteri, L., additional, Larionova, L. V., additional, Lee, C.-U., additional, Leto, P., additional, Lindfors, E., additional, Montagni, F., additional, Nesci, R., additional, Nieppola, E., additional, Nikolashvili, M. G., additional, Ohlert, J., additional, Oksanen, A., additional, Ovcharov, E., additional, Pääkkönen, P., additional, Pasanen, M., additional, Pursimo, T., additional, Ros, J. A., additional, Semkov, E., additional, Sigua, L. A., additional, Smart, R. L., additional, Strigachev, A., additional, Takalo, L. O., additional, Torii, K., additional, Torniainen, I., additional, Tornikoski, M., additional, Trigilio, C., additional, Tsunemi, H., additional, Umana, G., additional, and Valcheva, A., additional
- Published
- 2008
- Full Text
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111. The Outburst of the Blazar AO 0235+164 in 2006 December: Shock‐in‐Jet Interpretation
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Hagen‐Thorn, V. A., primary, Larionov, V. M., additional, Jorstad, S. G., additional, Arkharov, A. A., additional, Hagen‐Thorn, E. I., additional, Efimova, N. V., additional, Larionova, L. V., additional, and Marscher, A. P., additional
- Published
- 2008
- Full Text
- View/download PDF
112. The WEBT Campaign on the Blazar 3C 279 in 2006
- Author
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Bottcher, M., primary, Basu, S., additional, Joshi, M., additional, Villata, M., additional, Arai, A., additional, Aryan, N., additional, Asfandiyarov, I. M., additional, Bach, U., additional, Bachev, R., additional, Berduygin, A., additional, Blaek, M., additional, Buemi, C., additional, Castro‐Tirado, A. J., additional, De Ugarte Postigo, A., additional, Frasca, A., additional, Fuhrmann, L., additional, Hagen‐Thorn, V. A., additional, Henson, G., additional, Hovatta, T., additional, Hudec, R., additional, Ibrahimov, M., additional, Ishii, Y., additional, Ivanidze, R., additional, Jelinek, M., additional, Kamada, M., additional, Kapanadze, B., additional, Katsuura, M., additional, Kotaka, D., additional, Kovalev, Y. Y., additional, Kovalev, Yu. A., additional, Kubanek, P., additional, Kurosaki, M., additional, Kurtanidze, O., additional, Lahteenmaki, A., additional, Lanteri, L., additional, Larionov, V. M., additional, Larionova, L., additional, Lee, C.‐U., additional, Leto, P., additional, Lindfors, E., additional, Marilli, E., additional, Marshall, K., additional, Miller, H. R., additional, Mingaliev, M. G., additional, Mirabal, N., additional, Mizoguchi, S., additional, Nakamura, K., additional, Nieppola, E., additional, Nikolashvili, M., additional, Nilsson, K., additional, Nishiyama, S., additional, Ohlert, J., additional, Osterman, M. A., additional, Pak, S., additional, Pasanen, M., additional, Peters, C. S., additional, Pursimo, T., additional, Raiteri, C. M., additional, Robertson, J., additional, Robertson, T., additional, Ryle, W. T., additional, Sadakane, K., additional, Sadun, A., additional, Sigua, L., additional, Sohn, B.‐W., additional, Strigachev, A., additional, Sumitomo, N., additional, Takalo, L. O., additional, Tamesue, Y., additional, Tanaka, K., additional, Thorstensen, J. R., additional, Tosti, G., additional, Trigilio, C., additional, Umana, G., additional, Vennes, S., additional, Vitek, S., additional, Volvach, A., additional, Webb, J., additional, Yamanaka, M., additional, and Yim, H.‐S., additional
- Published
- 2007
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- View/download PDF
113. The radio delay of the exceptional 3C 454.3 outburst
- Author
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Villata, M., primary, Raiteri, C. M., additional, Aller, M. F., additional, Bach, U., additional, Ibrahimov, M. A., additional, Kovalev, Y. Y., additional, Kurtanidze, O. M., additional, Larionov, V. M., additional, Lee, C.-U., additional, Leto, P., additional, Lähteenmäki, A., additional, Nilsson, K., additional, Pursimo, T., additional, Ros, J. A., additional, Sumitomo, N., additional, Volvach, A., additional, Aller, H. D., additional, Arai, A., additional, Buemi, C. S., additional, Coloma, J. M., additional, Doroshenko, V. T., additional, Efimov, Yu. S., additional, Fuhrmann, L., additional, Hagen-Thorn, V. A., additional, Kamada, M., additional, Katsuura, M., additional, Konstantinova, T., additional, Kopatskaya, E., additional, Kotaka, D., additional, Kovalev, Yu. A., additional, Kurosaki, M., additional, Lanteri, L., additional, Larionova, L., additional, Mingaliev, M. G., additional, Mizoguchi, S., additional, Nakamura, K., additional, Nikolashvili, M. G., additional, Nishiyama, S., additional, Sadakane, K., additional, Sergeev, S. G., additional, Sigua, L. A., additional, Sillanpää, A., additional, Smart, R. L., additional, Takalo, L. O., additional, Tanaka, K., additional, Tornikoski, M., additional, Trigilio, C., additional, and Umana, G., additional
- Published
- 2007
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114. Detection of optical linear polarization in the SN 2006aj/XRF 060218 non-spherical expansion
- Author
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Gorosabel, J., primary, Larionov, V., additional, Castro-Tirado, A. J., additional, Guziy, S., additional, Larionova, L., additional, Del Olmo, A., additional, Martínez, M. A., additional, Cepa, J., additional, Cedrés, B., additional, de Ugarte Postigo, A., additional, Jelínek, M., additional, Bogdanov, O., additional, and LLorente, A., additional
- Published
- 2006
- Full Text
- View/download PDF
115. The unprecedented optical outburst of the quasar 3C 454.3
- Author
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Villata, M., primary, Raiteri, C. M., additional, Balonek, T. J., additional, Aller, M. F., additional, Jorstad, S. G., additional, Kurtanidze, O. M., additional, Nicastro, F., additional, Nilsson, K., additional, Aller, H. D., additional, Arai, A., additional, Arkharov, A., additional, Bach, U., additional, Benítez, E., additional, Berdyugin, A., additional, Buemi, C. S., additional, Böttcher, M., additional, Carosati, D., additional, Casas, R., additional, Caulet, A., additional, Chen, W. P., additional, Chiang, P.-S., additional, Chou, Y., additional, Ciprini, S., additional, Coloma, J. M., additional, Di Rico, G., additional, Díaz, C., additional, Efimova, N. V., additional, Forsyth, C., additional, Frasca, A., additional, Fuhrmann, L., additional, Gadway, B., additional, Gupta, S., additional, Hagen-Thorn, V. A., additional, Harvey, J., additional, Heidt, J., additional, Hernandez-Toledo, H., additional, Hroch, F., additional, Hu, C.-P., additional, Hudec, R., additional, Ibrahimov, M. A., additional, Imada, A., additional, Kamata, M., additional, Kato, T., additional, Katsuura, M., additional, Konstantinova, T., additional, Kopatskaya, E., additional, Kotaka, D., additional, Kovalev, Y. Y., additional, Kovalev, Yu. A., additional, Krichbaum, T. P., additional, Kubota, K., additional, Kurosaki, M., additional, Lanteri, L., additional, Larionov, V. M., additional, Larionova, L., additional, Laurikainen, E., additional, Lee, C.-U., additional, Leto, P., additional, Lähteenmäki, A., additional, López-Cruz, O., additional, Marilli, E., additional, Marscher, A. P., additional, McHardy, I. M., additional, Mondal, S., additional, Mullan, B., additional, Napoleone, N., additional, Nikolashvili, M. G., additional, Ohlert, J. M., additional, Postnikov, S., additional, Pursimo, T., additional, Ragni, M., additional, Ros, J. A., additional, Sadakane, K., additional, Sadun, A. C., additional, Savolainen, T., additional, Sergeeva, E. A., additional, Sigua, L. A., additional, Sillanpää, A., additional, Sixtova, L., additional, Sumitomo, N., additional, Takalo, L. O., additional, Teräsranta, H., additional, Tornikoski, M., additional, Trigilio, C., additional, Umana, G., additional, Volvach, A., additional, Voss, B., additional, and Wortel, S., additional
- Published
- 2006
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116. Modulation radiometer operating at 1.35 cm
- Author
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Khrulev, V. V., Samoilov, R. A., Fedyantsev, B. K., Zborovskii, V. S., and Larionova, L. F.
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- 1978
- Full Text
- View/download PDF
117. WEBT multiwavelength monitoring and XMM-Newton observations of BL Lacertaein 2007–2008*
- Author
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Raiteri, C. M., Villata, M., Capetti, A., Aller, M. F., Bach, U., Calcidese, P., Gurwell, M. A., Larionov, V. M., Ohlert, J., Nilsson, K., Strigachev, A., Agudo, I., Aller, H. D., Bachev, R., Benítez, E., Berdyugin, A., Böttcher, M., Buemi, C. S., Buttiglione, S., Carosati, D., Charlot, P., Chen, W. P., Dultzin, D., Forné, E., Fuhrmann, L., Gómez, J. L., Gupta, A. C., Heidt, J., Hiriart, D., Hsiao, W.-S., Jelínek, M., Jorstad, S. G., Kimeridze, G. N., Konstantinova, T. S., Kopatskaya, E. N., Kostov, A., Kurtanidze, O. M., Lähteenmäki, A., Lanteri, L., Larionova, L. V., Leto, P., Latev, G., Le Campion, J.-F., Lee, C.-U., Ligustri, R., Lindfors, E., Marscher, A. P., Mihov, B., Nikolashvili, M. G., Nikolov, Y., Ovcharov, E., Principe, D., Pursimo, T., Ragozzine, B., Robb, R. M., Ros, J. A., Sadun, A. C., Sagar, R., Semkov, E., Sigua, L. A., Smart, R. L., Sorcia, M., Takalo, L. O., Tornikoski, M., Trigilio, C., Uckert, K., Umana, G., Valcheva, A., Volvach, A., Raiteri, C. M., Villata, M., Capetti, A., Aller, M. F., Bach, U., Calcidese, P., Gurwell, M. A., Larionov, V. M., Ohlert, J., Nilsson, K., Strigachev, A., Agudo, I., Aller, H. D., Bachev, R., Benítez, E., Berdyugin, A., Böttcher, M., Buemi, C. S., Buttiglione, S., Carosati, D., Charlot, P., Chen, W. P., Dultzin, D., Forné, E., Fuhrmann, L., Gómez, J. L., Gupta, A. C., Heidt, J., Hiriart, D., Hsiao, W.-S., Jelínek, M., Jorstad, S. G., Kimeridze, G. N., Konstantinova, T. S., Kopatskaya, E. N., Kostov, A., Kurtanidze, O. M., Lähteenmäki, A., Lanteri, L., Larionova, L. V., Leto, P., Latev, G., Le Campion, J.-F., Lee, C.-U., Ligustri, R., Lindfors, E., Marscher, A. P., Mihov, B., Nikolashvili, M. G., Nikolov, Y., Ovcharov, E., Principe, D., Pursimo, T., Ragozzine, B., Robb, R. M., Ros, J. A., Sadun, A. C., Sagar, R., Semkov, E., Sigua, L. A., Smart, R. L., Sorcia, M., Takalo, L. O., Tornikoski, M., Trigilio, C., Uckert, K., Umana, G., Valcheva, A., and Volvach, A.
- Abstract
Context. BL Lacertaeis the prototype of the blazar subclass named after it. Yet, it has occasionally shown a peculiar behaviour that has questioned a simple interpretation of its broad-band emission in terms of synchrotron plus synchrotron self-Compton (SSC) radiation.
- Published
- 2009
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- View/download PDF
118. Results of WEBT, VLBA and RXTE monitoring of 3C 279during 2006–2007*
- Author
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Larionov, V. M., Jorstad, S. G., Marscher, A. P., Raiteri, C. M., Villata, M., Agudo, I., Aller, M. F., Arkharov, A. A., Asfandiyarov, I. M., Bach, U., Bachev, R., Berdyugin, A., Böttcher, M., Buemi, C. S., Calcidese, P., Carosati, D., Charlot, P., Chen, W.-P., Di Paola, A., Dolci, M., Dogru, S., Doroshenko, V. T., Efimov, Yu. S., Erdem, A., Frasca, A., Fuhrmann, L., Giommi, P., Glowienka, L., Gupta, A. C., Gurwell, M. A., Hagen-Thorn, V. A., Hsiao, W.-S., Ibrahimov, M. A., Jordan, B., Kamada, M., Konstantinova, T. S., Kopatskaya, E. N., Kovalev, Y. Y., Kovalev, Y. A., Kurtanidze, O. M., Lähteenmäki, A., Lanteri, L., Larionova, L. V., Leto, P., Le Campion, P., Lee, C.-U., Lindfors, E., Marilli, E., McHardy, I., Mingaliev, M. G., Nazarov, S. V., Nieppola, E., Nilsson, K., Ohlert, J., Pasanen, M., Porter, D., Pursimo, T., Ros, J. A., Sadakane, K., Sadun, A. C., Sergeev, S. G., Smith, N., Strigachev, A., Sumitomo, N., Takalo, L. O., Tanaka, K., Trigilio, C., Umana, G., Ungerechts, H., Volvach, A., Yuan, W., Larionov, V. M., Jorstad, S. G., Marscher, A. P., Raiteri, C. M., Villata, M., Agudo, I., Aller, M. F., Arkharov, A. A., Asfandiyarov, I. M., Bach, U., Bachev, R., Berdyugin, A., Böttcher, M., Buemi, C. S., Calcidese, P., Carosati, D., Charlot, P., Chen, W.-P., Di Paola, A., Dolci, M., Dogru, S., Doroshenko, V. T., Efimov, Yu. S., Erdem, A., Frasca, A., Fuhrmann, L., Giommi, P., Glowienka, L., Gupta, A. C., Gurwell, M. A., Hagen-Thorn, V. A., Hsiao, W.-S., Ibrahimov, M. A., Jordan, B., Kamada, M., Konstantinova, T. S., Kopatskaya, E. N., Kovalev, Y. Y., Kovalev, Y. A., Kurtanidze, O. M., Lähteenmäki, A., Lanteri, L., Larionova, L. V., Leto, P., Le Campion, P., Lee, C.-U., Lindfors, E., Marilli, E., McHardy, I., Mingaliev, M. G., Nazarov, S. V., Nieppola, E., Nilsson, K., Ohlert, J., Pasanen, M., Porter, D., Pursimo, T., Ros, J. A., Sadakane, K., Sadun, A. C., Sergeev, S. G., Smith, N., Strigachev, A., Sumitomo, N., Takalo, L. O., Tanaka, K., Trigilio, C., Umana, G., Ungerechts, H., Volvach, A., and Yuan, W.
- Abstract
Context. The quasar 3C 279is among the most extreme blazars in terms of luminosity and variability of flux at all wavebands. Its variations in flux and polarization are quite complex and therefore require intensive monitoring observations at multiple wavebands to characterise and interpret the observed changes.
- Published
- 2008
- Full Text
- View/download PDF
119. Radio-to-UV monitoring of AO 0235+164by the WEBT and Swift during the 2006–2007 outburst
- Author
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Raiteri, C. M., Villata, M., Larionov, V. M., Aller, M. F., Bach, U., Gurwell, M., Kurtanidze, O. M., Lähteenmäki, A., Nilsson, K., Volvach, A., Aller, H. D., Arkharov, A. A., Bachev, R., Berdyugin, A., Böttcher, M., Buemi, C. S., Calcidese, P., Cozzi, E., Di Paola, A., Dolci, M., Fan, J. H., Forné, E., Foschini, L., Gupta, A. C., Hagen-Thorn, V. A., Hooks, L., Hovatta, T., Joshi, M., Kadler, M., Kimeridze, G. N., Konstantinova, T. S., Kostov, A., Krichbaum, T. P., Lanteri, L., Larionova, L. V., Lee, C.-U., Leto, P., Lindfors, E., Montagni, F., Nesci, R., Nieppola, E., Nikolashvili, M. G., Ohlert, J., Oksanen, A., Ovcharov, E., Pääkkönen, P., Pasanen, M., Pursimo, T., Ros, J. A., Semkov, E., Sigua, L. A., Smart, R. L., Strigachev, A., Takalo, L. O., Torii, K., Torniainen, I., Tornikoski, M., Trigilio, C., Tsunemi, H., Umana, G., Valcheva, A., Raiteri, C. M., Villata, M., Larionov, V. M., Aller, M. F., Bach, U., Gurwell, M., Kurtanidze, O. M., Lähteenmäki, A., Nilsson, K., Volvach, A., Aller, H. D., Arkharov, A. A., Bachev, R., Berdyugin, A., Böttcher, M., Buemi, C. S., Calcidese, P., Cozzi, E., Di Paola, A., Dolci, M., Fan, J. H., Forné, E., Foschini, L., Gupta, A. C., Hagen-Thorn, V. A., Hooks, L., Hovatta, T., Joshi, M., Kadler, M., Kimeridze, G. N., Konstantinova, T. S., Kostov, A., Krichbaum, T. P., Lanteri, L., Larionova, L. V., Lee, C.-U., Leto, P., Lindfors, E., Montagni, F., Nesci, R., Nieppola, E., Nikolashvili, M. G., Ohlert, J., Oksanen, A., Ovcharov, E., Pääkkönen, P., Pasanen, M., Pursimo, T., Ros, J. A., Semkov, E., Sigua, L. A., Smart, R. L., Strigachev, A., Takalo, L. O., Torii, K., Torniainen, I., Tornikoski, M., Trigilio, C., Tsunemi, H., Umana, G., and Valcheva, A.
- Abstract
Context.The blazar AO 0235+164was claimed to show a quasi-periodic behaviour in the radio and optical bands in the past, with the main outbursts repeating every 5–6 years. However, the predicted 2004 outburst did not occur, and further analysis suggested a longer time scale, according to which the next event would have occurred in the 2006–2007 observing season. Moreover, an extra emission component contributing to the UV and soft X-ray flux was detected, whose nature is not yet clear. An optical outburst was observed in late 2006–early 2007, which triggered a Whole Earth Blazar Telescope (WEBT) campaign as well as target of opportunity (ToO) observations by the Swift satellite.
- Published
- 2008
- Full Text
- View/download PDF
120. Detection of optical linear polarization in the SN 2006aj/XRF 060218non-spherical expansion
- Author
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Gorosabel, J., Larionov, V., Castro-Tirado, A. J., Guziy, S., Larionova, L., Del Olmo, A., Martínez, M. A., Cepa, J., Cedrés, B., de Ugarte Postigo, A., Jelínek, M., Bogdanov, O., LLorente, A., Gorosabel, J., Larionov, V., Castro-Tirado, A. J., Guziy, S., Larionova, L., Del Olmo, A., Martínez, M. A., Cepa, J., Cedrés, B., de Ugarte Postigo, A., Jelínek, M., Bogdanov, O., and LLorente, A.
- Abstract
Aims.We have performed optical polarimetric observations of the SN 2006aj associated to the X-ray flash (XRF) of February 18, 2006, XRF 060218that provide information on its expansion geometry.
- Published
- 2006
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- View/download PDF
121. Surface abundances of light elements for a large sample of early B-type stars -- I. Spectral observations of 123 stars; measurements of hydrogen and helium lines; infrared photometry
- Author
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Lyubimkov, L. S., primary, Lambert, D. L., additional, Rachkovskaya, T. M., additional, Rostopchin, S. I., additional, Tarasov, A. E., additional, Poklad, D. B., additional, Larionov, V. M., additional, and Larionova, L. V., additional
- Published
- 2000
- Full Text
- View/download PDF
122. Development of an automated unit for extraction-chromatographic separation of the Mo/Tc generator couple.
- Author
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Skuridin, V., Stasyuk, E., Rogov, A., Nesterov, E., Sadkin, V., Varlamova, N., and Larionova, L.
- Subjects
CHROMATOGRAPHIC analysis ,EXTRACTION (Chemistry) ,MEDICAL radiology ,AUTOMATIC control systems ,RADIOPHARMACEUTICALS ,MEDICAL laboratories - Abstract
The design and automatic control scheme were developed for an extraction-chromatographic unit for producing Tc preparations. The unit is intended for operation under the conditions of medical radiological laboratories. Technical trials showed that the mean time of preparation of sodium [Tc]pertechnetate radiopharmaceutical did not exceed 25 min. [ABSTRACT FROM AUTHOR]
- Published
- 2014
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- View/download PDF
123. Statistical characteristics of radio sources connected with high latitude galactic population of objects
- Author
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Larionov, M. G., primary, Sidorenkov, V. N., additional, Larionova, L. N., additional, and Ugol'kova, L. S., additional
- Published
- 1999
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124. Long-term variability of the Be/X-ray binary A0535+26 -- III. Photometry
- Author
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Clark, J. S., primary, Lyuty, V. M., additional, Zaitseva, G. V., additional, Larionov, V. M., additional, Larionova, L. V., additional, Finger, M., additional, Tarasov, A. E., additional, Roche, P., additional, and Coe, M. J., additional
- Published
- 1999
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- View/download PDF
125. Long-term variability of the Be/X-ray binary A 0535+26 -- I. Optical and UV spectroscopy
- Author
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Clark, J. S., primary, Tarasov, A. E., additional, Steele, I. A., additional, Coe, M. J., additional, Roche, P., additional, Shrader, C., additional, Buckley, D. A. H., additional, Larionov, V., additional, Larionova, L., additional, Lyuty, V. M., additional, Zaitseva, G. V., additional, Grunsfeld, J., additional, Fabregat, J., additional, and Parise, R., additional
- Published
- 1998
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- View/download PDF
126. Studying the General Toxicity and Cumulative Properties of a Radiopharmaceutical Nanocolloid, Tc-AlO.
- Author
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Varlamova, N., Churin, A., Fomina, T., Ermolaeva, L., Vetoshkina, T., Dubskaya, T., Lamzina, T., Fedorova, E., Neupokoeva, O., Skuridin, V., Nesterov, E., Larionova, L., and Chernov, V.
- Subjects
RADIOPHARMACEUTICALS ,ACUTE toxicity testing ,COLLOIDS ,BONE marrow ,SENTINEL lymph nodes ,NANOSTRUCTURED materials - Abstract
We studied toxicity of a new Russian radiopharmaceutical Nanocolloid, Tc-AlO. Tests for acute toxicity showed that this agent belongs to a class of moderate-toxicity substances and does not have cumulative properties. The evaluation of subchronic toxicity after subcutaneous injection of this product to rats (0.04, 0.2, and 0.4 ml/kg) and rabbits (0.02 and 0.2 ml/kg) for 7 days did not reveal changes in the general state, temperature, body weight, indices of the peripheral blood and bone marrow, functions of the heart, liver, kidneys, and nervous system, and morphological characteristics of the internal organs in animals. The drug does not produce a local irritant effect. [ABSTRACT FROM AUTHOR]
- Published
- 2016
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- View/download PDF
127. Insights into the High-energy γ-ray Emission of Markarian 501 from Extensive Multifrequency Observations in the Fermi Era
- Author
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Abdo, A. A., Ackermann, M., Ajello, M., Allafort, A., Baldini, Luca, Ballet, J., Barbiellini, G., Baring, M. G., Bastieri, D., Bechtol, K., Bellazzini, R., Berenji, B., Blandford, R. D., Bloom, E. D., Bonamente, E., Borgland, A. W., Bouvier, A., Brandt, T. J., Bregeon, J., Brez, A., Brigida, M., Bruel, P., Buehler, R., Buson, S., Caliandro, G. A., Cameron, R. A., Cannon, A., Caraveo, P. A., Carrigan, S., Casandjian, J. M., Cavazzuti, E., Cecchi, C., Celik, O. ., Charles, E., Chekhtman, A., Cheung, C. C., Chiang, J., Ciprini, S., Claus, R., Cohen Tanugi, J., Conrad, J., Cutini, S., Dermer, C. D., de Palma, F., do Couto, e. Silva E., Drell, P. S., Dubois, R., Dumora, D., Favuzzi, C., Fegan, S. J., Ferrara, E. C., Focke, W. B., Fortin, P., Frailis, M., Fuhrmann, L., Fukazawa, Y., Funk, S., Fusco, P., Gargano, F., Gasparrini, D., Gehrels, N., Germani, S., Giglietto, N., Giordano, F., Giroletti, M., Glanzman, T., Godfrey, G., Grenier, I. A., Guillemot, L., Guiriec, S., Hayashida, M., Hays, E., Horan, D., Hughes, R. E., Johannesson, G., Johnson, A. S., Johnson, W. N., Kadler, M., Kamae, T., Katagiri, H., Kataoka, J., Knoedlseder, J., Kuss, M., Lande, J., Latronico, L., Lee, S. H., Lemoine Goumard, M., Longo, F., Loparco, F., Lott, B., Lovellette, M. N., Lubrano, P., Madejski, G. M., Makeev, A., Max Moerbeck, W., Mazziotta, M. N., Mcenery, J. E., Mehault, J., Michelson, P. F., Mitthumsiri, W., Mizuno, T., Moiseev, A. A., Monte, C., Monzani, M. E., Morselli, A., Moskalenko, I. V., Murgia, S., Naumann Godo, M., Nishino, S., Nolan, P. L., Norris, J. P., Nuss, E., Ohsugi, T., Okumura, A., Omodei, N., Orlando, E., Ormes, J. F., Paneque, D., Panetta, J. H., Parent, D., Pavlidou, V., Pearson, T. J., Pelassa, V., Pepe, M., Pesce Rollins, M., Piron, F., Porter, T. A., Raino, S., Rando, R., Razzano, Massimiliano, Readhead, A., Reimer, A., Reimer, O., Richards, J. L., Ripken, J., Ritz, S., Roth, M., Sadrozinski, H. F. W., Sanchez, D., Sander, A., Scargle, J. D., Sgro, C., Siskind, E. J., Smith, P. D., Spandre, G., Spinelli, P., Stawarz, L., Stevenson, M., Strickman, M. S., Sokolovsky, K. V., Suson, D. J., Takahashi, H., Takahashi, T., Tanaka, T., Thayer, J. B., Thayer, J. G., Thompson, D. J., Tibaldo, L., Torres, F., Tosti, G., Tramacere, A., Uchiyama, Y., Usher, T. L., Vandenbroucke, J., Vasileiou, V., Vilchez, N., Vitale, V., Waite, A. P., Wang, P., Wehrle, A. E., Winer, B. L., Wood, K. S., Yang, Z., Ylinen, T., Zensus, J. A., Ziegler, M., Aleksic, J., Antonelli, L. A., Antoranz, P., Backes, M., Barrio, J. A., Becerra, Gonzalez J., Bednarek, W., Berdyugin, A., Berger, K., Bernardini, E., Biland, A., Blanch, O., Bock, R. K., Boller, A., Bonnoli, G., Bordas, P., Borla, Tridon D., Bosch Ramon, V., Bose, D., Braun, I., Bretz, T., Camara, M., Carmona, E., Carosi, A., Colin, P., Colombo, E., Contreras, J. L., Cortina, J., Covino, S., Dazzi, F., de Angelis, A., De Cea, del Pozo E., De Lotto, B., De Maria, M., De Sabata, F., Delgado, Mendez C., Diago, Ortega A., Doert, M., Dominguez, A., Dominis, Prester D., Dorner, D., Doro, M., Elsaesser, D., Ferenc, D., Fonseca, M. V., Font, L., Garcia, Lopen R. J., Garczarczyk, M., Gaug, M., Giavitto, G., Godinovi, N., Hadasch, D., Herrero, A., Hildebrand, D., Hoehne Moench, D., Hose, J., Hrupec, D., Jogler, T., Klepser, S., Kraehenbuehl, T., Kranich, D., Krause, J., La Barbera, A., Leonardo, E., Lindfors, E., Lombardi, S., Lopez, M., Lorenz, E., Majumdar, P., Makariev, E., Maneva, G., Mankuzhiyil, N., Mannheim, K., Maraschi, L., Mariotti, M., Martinez, M., Mazin, D., Meucci, M., Miranda, J. M., Mirzoyan, R., Miyamoto, H., Moldon, J., Moralejo, A., Nieto, D., Nilsson, K., Orito, R., Oya, I., Paoletti, R., Paredes, J. M., Partini, S., Pasanen, M., Pauss, F., Pegna, R. G., Perez Torres, M. A., Persic, M., Peruzzo, J., Pochon, J., PRADA MORONI, PIER GIORGIO, Prada, F., Prandini, E., Puchades, N., Puljak, I., Reichardt, T., Reinthal, R., Rhode, W., Ribo, M., Rico, J., Rissi, M., Ruegamer, S., Saggion, A., Saito, K., Saito, T. Y., Salvati, M., Sanchez Conde, M., Satalecka, K., Scalzotto, V., Scapin, V., Schultz, C., Schweizer, T., Shayduk, M., Shore, STEVEN NEIL, Sierpowska Bartosik, A., Sillanpaa, A., Sitarek, J., Sobczynska, D., Spanier, F., Spiro, S., Stamerra, A., Steinke, B., Storz, J., Strah, N., Struebig, J. C., Suric, T., Takalo, L. O., Tavecchio, F., Temnikov, P., Terzic, T., Tescaro, D., Teshima, M., Vankov, H., Wagner, R. M., Weitzel, Q., Zabalza, V., Zandanel, F., Zanin, R., Acciari, V. A., Arlen, T., Aune, T., Benbow, W., Boltuch, D., Bradbury, S. M., Buckley, J. H., Bugaev, V., Cesarini, A., Ciupik, L., Cui, W., Dickherber, R., Errando, M., Falcone, A., Finley, J. P., Finnegan, G., Fortson, L., Furniss, A., Galante, N., Gall, D., Gillanders, G. 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C., Sakamoto, T., Tornikoski, M., Yatsu, Y., tschke V, Zook A., Raab, Fj, Rabeling, Ds, Racz, I, Radkins, H, Raffai, P, Rakhmanov, M, Ramet, Cr, Rankins, B, Rapagnani, P, Raymond, V, Re, V, Redwine, K, Reed, Cm, Reed, T, Regimbau, T, Reid, S, Reitze, Dh, Ricci, F, Riesen, R, Riles, K, Roberts, P, Robertson, Na, Robinet, F, Robinson, C, Robinson, El, Rocchi, A, Roddy, S, Rolland, L, Rollins, J, Romano, Jd, Romano, R, Romie, Jh, Rosinska, D, Rover, C, Rowan, S, Udiger, Ar, Ruggi, P, Ryan, K, Sakata, S, Sakosky, M, Salemi, F, Salit, M, Sammut, L, de la Jordana LS, Sandberg, V, Sannibale, V, Santamaria, L, Santiago Prieto, I, Santostasi, G, Saraf, S, Sassolas, B, Sathyaprakash, Bs, Sato, S, Satterthwaite, M, Saulson, Pr, Savage, R, Schilling, R, Schlamminger, S, Schnabel, R, Schofield, Rms, Schulz, B, Schutz, Bf, Schwinberg, P, Scott, J, Scott, Sm, Searle, Ac, Seifert, F, Sellers, D, Sengupta, As, Sentenac, D, Sergeev, A, Shaddock, Da, Shaltev, M, Shapiro, B, Shawhan, P, Weerathunga, Ts, Shoemaker, Dh, Sibley, A, Siemens, X, Sigg, D, Singer, A, Singer, L, Sintes, Am, Skelton, G, Slagmolen, Bjj, Slutsky, J, Smith, Jr, Smith, Mr, Smith, Nd, Smith, R, Somiya, K, Sorazu, B, Soto, J, Speirits, Fc, Sperandio, L, Stefszky, M, Stein, Aj, Steinlechner, J, Steinlechner, S, Steplewski, S, Stochino, A, Stone, R, Strain, Ka, Strigin, S, Stroeer, As, Sturani, R, Stuver, Al, Summerscales, Tz, Sung, M, Susmithan, S, Sutton, Pj, Swinkels, B, Szokoly, Gp, Tacca, M, Talukder, D, Tanner, Db, Tarabrin, Sp, Taylor, Jr, Taylor, R, Thomas, P, Thorne, Ka, Thorne, Ks, Thrane, E, Thuring, A, Titsler, C, Tokmakov, Kv, Toncelli, A, Tonelli, M, Torre, O, Torres, C, Torrie, Ci, Tournefier, E, Travasso, F, Traylor, G, Trias, M, Tseng, K, Turner, L, Ugolini, D, Urbanek, K, Vahlbruch, H, Vaishnav, B, Vajente, G, Vallisneri, M, van den Brand JFJ, Van Den Broeck, C, van der Putten, S, van der Sluys MV, van Veggel AA, Vass, S, Vasuth, M, Vaulin, R, Vavoulidis, M, Vecchio, A, Vedovato, G, Veitch, J, Veitch, Pj, Veltkamp, C, Verkindt, D, Vetrano, F, Vicere, A, Villar, Ae, Vinet, Jy, Vocca, H, Vorvick, C, Vyachanin, Sp, Waldman, Sj, Wallace, L, Wanner, A, Ward, Rl, Was, M, Wei, P, Weinert, M, Weinstein, Aj, Weiss, R, Wen, L, Wen, S, Wessels, P, West, M, Westphal, T, Wette, K, Whelan, Jt, Whitcomb, Se, White, D, Whiting, Bf, Wilkinson, C, Willems, Pa, Williams, Hr, Williams, L, Willke, B, Winkelmann, L, Winkler, W, Wipf, Cc, Wiseman, Ag, Woan, G, Wooley, R, Worden, J, Yablon, J, Yakushin, I, Yamamoto, H, Yamamoto, K, Yang, H, Yeaton Massey, D, Yoshida, S, Yu, P, Yvert, M, Zanolin, M, Zhang, L, Zhang, Z, Zhao, C, Zotov, N, Zucker, Me, Zweizig, J, Aptekar, Rl, Boynton, Wv, Briggs, Ms, Cline, Tl, Connaughton, V, Frederiks, Dd, Gehrels, N, Goldsten, Jo, Golovin, D, van der Horst AJ, Hurley, Kc, Kaneko, Y, von Kienlin, A, Kouveliotou, C, Krimm, Ha, Lin, L, Mitrofanov, I, Ohno, M, Pal'Shin, Vd, Rau, A, Sanin, A, Tashiro, Ms, Terada, Y, Yamaoka Kn, Y. A., Kus, V., Kuykendall, W., Kuze, M., Kuzhir, P., Kvasnicka, O., Kwee, R., La Rosa, A., La Rotonda, L., Labarga, L., Labbe, J., Lacasta, C., Lacava, F., Lacker, H., Lacour, D., Lacuesta, V. R., Ladygin, E., Lafaye, R., Laforge, B., Lagouri, T., Lai, S., Laisne, E., Lamanna, M., Lampen, C. L., Lampl, W., Lancon, E., Landgraf, U., Landon, M. P. J., Landsman, H., Lane, J. L., Lange, C., Lankford, A. J., Lanni, F., Lantzsch, K., Lapin, V. V., Laplace, S., Lapoire, C., Laporte, J. F., Lari, T., Larionov, A. V., Larner, A., Lasseur, C., Lassnig, M., Lau, W., Laurelli, P., Lavorato, A., Lavrijsen, W., Laycock, P., Lazarev, A. B., Lazzaro, A., Le Dortz, O., Le Guirriec, E., Le Maner, C., Le Menedeu, E., Leahu, M., Lebedev, A., Lebel, C., Lecompte, T., Ledroit Guillon, F., Lee, H., Lee, J. S. H., Lee, S. C., Lee, L., Lefebvre, M., Legendre, M., Leger, A., Legeyt, B. C., Legger, F., Leggett, C., Lehmacher, M., Lehmann, Miotto G., Lei, X., Leite, M. A. L., Leitner, R., Lellouch, D., Lellouch, J., Leltchouk, M., Lendermann, V., Leney, K. J. C., Lenz, T., Lenzen, G., Lenzi, B., Leonhardt, K., Leontsinis, S., Leroy, C., Lessard, J. R., Lesser, J., Lester, C. G., Leung Fook, Cheong A., Leveque, J., Levin, D., Levinson, L. J., Levitski, M. S., Lewandowska, M., Lewis, G. H., Leyton, M., Li, B., Li, H., Li, S., Li, X., Liang, Z., Liberti, B., Lichard, P., Lichtnecker, M., Lie, K., Liebig, W., Lifshitz, R., Lilley, J. N., Limosani, A., Limper, M., Lin, S. C., Linde, F., Linnemann, J. T., Lipeles, E., Lipinsky, L., Lipniacka, A., Liss, T. M., Lissauer, D., Lister, A., Litke, A. M., Liu, C., Liu, D., Liu, H., Liu, J. B., Liu, M., Liu, S., Liu, Y., Livan, M., Livermore, S. S. A., Lleres, A., Lloyd, S. L., Lobodzinska, E., Loch, P., Lockman, W. S., Lockwitz, S., Loddenkoetter, T., Loebinger, F. K., Loginov, A., Loh, C. W., Lohse, T., Lohwasser, K., Lokajicek, M., Loken, J., Lombardo, V. P., Long, R. E., Lopes, L., Lopez, Mateos D., Losada, M., Loscutoff, P., Lo Sterzo, F., Losty, M. J., Lou, X., Lounis, A., Loureiro, K. F., Love, J., Love, P. A., Lowe, A. J., Lu, F., Lu, J., Lu, L., Lubatti, H. J., Luci, C., Lucotte, A., Ludwig, A., Ludwig, D., Ludwig, I., Ludwig, J., Luehring, F., Luijckx, G., Lumb, D., Luminari, L., Lund, E., Lund Jensen, B., Lundberg, B., Lundberg, J., Lundquist, J., Lungwitz, M., Lupi, A., Lutz, G., Lynn, D., Lys, J., Lytken, E., Ma, H., L. L., Ma, Macana, Goia J. A., Maccarrone, G., Macchiolo, A., Macek, B., Machado Miguens, J., Macina, D., Mackeprang, R., Madaras, R. J., Mader, W. F., Maenner, R., Maeno, T., Maettig, P., Maettig, S., Magalhaes Martins, P. J., Magnoni, L., Magradze, E., Magrath, C. A., Mahalalel, Y., Mahboubi, K., Mahout, G., Maiani, C., Maidantchik, C., Maio, A., Majewski, S., Makida, Y., Makovec, N., Mal, P., Malecki, Pa, Malecki, P., Maleev, V. P., Malek, F., Mallik, U., Malon, D., Maltezos, S., Malyshev, V., Malyukov, S., Mameghani, R., Mamuzic, J., Manabe, A., Mandelli, L., Mandic, I., Mandrysch, R., Maneira, J., Mangeard, P. S., Manjavidze, I. D., Mann, A., Manning, P. M., Manousakis Katsikakis, A., Mansoulie, B., Manz, A., Mapelli, A., Mapelli, L., March, L., Marchand, J. F., Marchese, F., Marchesotti, M., Marchiori, G., Marcisovsky, M., Marin, A., Marino, C. P., Marroquim, F., Marshall, R., Marshall, Z., Martens, F. K., Marti Garcia, S., Martin, A. J., Martin, B., Martin, F. F., Martin, J. P., Martin, Ph, Universitat de Barcelona, Astrophysique Interprétation Modélisation (AIM (UMR_7158 / UMR_E_9005 / UM_112)), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7), Centre d'étude spatiale des rayonnements (CESR), Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), Laboratoire Leprince-Ringuet (LLR), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Théorique et Astroparticules (LPTA), Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Fermi-LAT, Abdo, A. A., Ackermann, M., Ajello, M., Allafort, A., Baldini, L., Ballet, J., Barbiellini, G., Baring, M. G., Bastieri, D., Bechtol, K., Bellazzini, R., Berenji, B., Blandford, R. D., Bloom, E. D., Bonamente, E., Borgland, A. W., Bouvier, A., Brandt, T. J., Bregeon, J., Brez, A., Brigida, M., Bruel, P., Buehler, R., Buson, S., Caliandro, G. A., Cameron, R. A., Cannon, A., Caraveo, P. A., Carrigan, S., Casandjian, J. M., Cavazzuti, E., Cecchi, C., Çelik, Ö., Charles, E., Chekhtman, A., Cheung, C. C., Chiang, J., Ciprini, S., Claus, R., Cohen Tanugi, J., Conrad, J., Cutini, S., Dermer, C. D., de Palma, F., Silva, E. do Couto e., Drell, P. S., Dubois, R., Dumora, D., Favuzzi, C., Fegan, S. J., Ferrara, E. C., Focke, W. B., Fortin, P., Frailis, M., Fuhrmann, L., Fukazawa, Y., Funk, S., Fusco, P., Gargano, F., Gasparrini, D., Gehrels, N., Germani, S., Giglietto, N., Giordano, F., Giroletti, M., Glanzman, T., Godfrey, G., Grenier, I. A., Guillemot, L., Guiriec, S., Hayashida, M., Hays, E., Horan, D., Hughes, R. E., Jóhannesson, G., Johnson, A. S., Johnson, W. N., Kadler, M., Kamae, T., Katagiri, H., Kataoka, J., Knödlseder, J., Kuss, M., Lande, J., Latronico, L., Lee, S. H., Lemoine Goumard, M., Longo, Francesco, Loparco, F., Lott, B., Lovellette, M. N., Lubrano, P., Madejski, G. M., Makeev, A., Max Moerbeck, W., Mazziotta, M. N., Mcenery, J. E., Mehault, J., Michelson, P. F., Mitthumsiri, W., Mizuno, T., Moiseev, A. A., Monte, C., Monzani, M. E., Morselli, A., Moskalenko, I. V., Murgia, S., Naumann Godo, M., Nishino, S., Nolan, P. L., Norris, J. P., Nuss, E., Ohsugi, T., Okumura, A., Omodei, N., Orlando, E., Ormes, J. F., Paneque, D., Panetta, J. H., Parent, D., Pavlidou, V., Pearson, T. J., Pelassa, V., Pepe, M., Pesce Rollins, M., Piron, F., Porter, T. A., Rainò, S., Rando, R., Razzano, M., Readhead, A., Reimer, A., Reimer, O., Richards, J. L., Ripken, J., Ritz, S., Roth, M., Sadrozinski, H. F. W., Sanchez, D., Sander, A., Scargle, J. D., Sgrò, C., Siskind, E. J., Smith, P. D., Spandre, G., Spinelli, P., Stawarz, Ł., Stevenson, M., Strickman, M. S., Sokolovsky, K. V., Suson, D. J., Takahashi, H., Takahashi, T., Tanaka, T., Thayer, J. B., Thayer, J. G., Thompson, D. J., Tibaldo, L., Torres, D. F., Tosti, G., Tramacere, A., Uchiyama, Y., Usher, T. L., Vandenbroucke, J., Vasileiou, V., Vilchez, N., Vitale, V., Waite, A. P., Wang, P., Wehrle, A. E., Winer, B. L., Wood, K. S., Yang, Z., Ylinen, T., Zensus, J. A., Ziegler, M., Aleksić, J., Antonelli, L. A., Antoranz, P., Backes, M., Barrio, J. A., Becerra González, J., Bednarek, W., Berdyugin, A., Berger, K., Bernardini, E., Biland, A., Blanch, O., Bock, R. K., Boller, A., Bonnoli, G., Bordas, P., Borla Tridon, D., Bosch Ramon, V., Bose, D., Braun, I., Bretz, T., Camara, M., Carmona, E., Carosi, A., Colin, P., Colombo, E., Contreras, J. L., Cortina, J., Covino, S., Dazzi, F., de Angelis, A., De Cea del Pozo, E., De Lotto, B., De Maria, M., De Sabata, F., Delgado Mendez, C., Diago Ortega, A., Doert, M., Domínguez, A., Dominis Prester, D., Dorner, D., Doro, M., Elsaesser, D., Ferenc, D., Fonseca, M. V., Font, L., García López, R. J., Garczarczyk, M., Gaug, M., Giavitto, G., Godinovi, N., Hadasch, D., Herrero, A., Hildebrand, D., Höhne Mönch, D., Hose, J., Hrupec, D., Jogler, T., Klepser, S., Krähenbühl, T., Kranich, D., Krause, J., La Barbera, A., Leonardo, E., Lindfors, E., Lombardi, S., López, M., Lorenz, E., Majumdar, P., Makariev, E., Maneva, G., Mankuzhiyil, N., Mannheim, K., Maraschi, L., Mariotti, M., Martínez, M., Mazin, D., Meucci, M., Miranda, J. M., Mirzoyan, R., Miyamoto, H., Moldón, J., Moralejo, A., Nieto, D., Nilsson, K., Orito, R., Oya, I., Paoletti, R., Paredes, J. M., Partini, S., Pasanen, M., Pauss, F., Pegna, R. G., Perez Torres, M. A., Persic, M., Peruzzo, J., Pochon, J., Prada Moroni, P. G., Prada, F., Prandini, E., Puchades, N., Puljak, I., Reichardt, T., Reinthal, R., Rhode, W., Ribó, M., Rico, J., Rissi, M., Rügamer, S., Saggion, A., Saito, K., Saito, T. Y., Salvati, M., Sánchez Conde, M., Satalecka, K., Scalzotto, V., Scapin, V., Schultz, C., Schweizer, T., Shayduk, M., Shore, S. N., Sierpowska Bartosik, A., Sillanpää, A., Sitarek, J., Sobczynska, D., Spanier, F., Spiro, S., Stamerra, A., Steinke, B., Storz, J., Strah, N., Struebig, J. C., Suric, T., Takalo, L. O., Tavecchio, F., Temnikov, P., Terzić, T., Tescaro, D., Teshima, M., Vankov, H., Wagner, R. M., Weitzel, Q., Zabalza, V., Zandanel, F., Zanin, R., Acciari, V. A., Arlen, T., Aune, T., Benbow, W., Boltuch, D., Bradbury, S. M., Buckley, J. H., Bugaev, V., Cesarini, A., Ciupik, L., Cui, W., Dickherber, R., Errando, M., Falcone, A., Finley, J. P., Finnegan, G., Fortson, L., Furniss, A., Galante, N., Gall, D., Gillanders, G. H., Godambe, S., Grube, J., Guenette, R., Gyuk, G., Hanna, D., Holder, J., Huang, D., Hui, C. M., Humensky, T. B., Kaaret, P., Karlsson, N., Kertzman, M., Kieda, D., Konopelko, A., Krawczynski, H., Krennrich, F., Lang, M. J., Maier, G., Mcarthur, S., Mccann, A., Mccutcheon, M., Moriarty, P., Mukherjee, R., Ong, R., Otte, A. N., Pandel, D., Perkins, J. S., Pichel, A., Pohl, M., Quinn, J., Ragan, K., Reyes, L. C., Reynolds, P. T., Roache, E., Rose, H. J., Rovero, A. C., Schroedter, M., Sembroski, G. H., Senturk, G. D., Steele, D., Swordy, S. P., Tešić, G., Theiling, M., Thibadeau, S., Varlotta, A., Vincent, S., Wakely, S. P., Ward, J. E., Weekes, T. C., Weinstein, A., Weisgarber, T., Williams, D. A., Wood, M., Zitzer, B., Villata, M., Raiteri, C. M., Aller, H. D., Aller, M. F., Arkharov, A. A., Blinov, D. A., Calcidese, P., Chen, W. P., Efimova, N. V., Kimeridze, G., Konstantinova, T. S., Kopatskaya, E. N., Koptelova, E., Kurtanidze, O. M., Kurtanidze, S. O., Lähteenmäki, A., Larionov, V. M., Larionova, E. G., Larionova, L. V., Ligustri, R., Morozova, D. A., Nikolashvili, M. G., Sigua, L. A., Troitsky, I. S., Angelakis, E., Capalbi, M., Carramiñana, A., Carrasco, L., Cassaro, P., de la Fuente, E., Gurwell, M. A., Kovalev, Y. Y., Kovalev, Y. u. A., Krichbaum, T. P., Krimm, H. A., Leto, P., Lister, M. L., Maccaferri, G., Moody, J. W., Mori, Y., Nestoras, I., Orlati, A., Pagani, C., Pace, C., Pearson R., Iii, Perri, M., Piner, B. G., Pushkarev, A. B., Ros, E., Sadun, A. C., Sakamoto, T., Tornikoski, M., Yatsu, Y., Zook, A., Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Université Sciences et Technologies - Bordeaux 1 (UB)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées, and Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)
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BL Lacertae objects: individual (Mrk 501) ,Photon ,PARTICLE-ACCELERATION ,Astrophysics ,Electron ,01 natural sciences ,CHERENKOV TELESCOPE SYSTEM ,LARGE-AREA TELESCOPE ,Raigs gamma ,individual: Mrk 501 [BL Lacertae objects] ,EARLY-TYPE GALAXIES ,010303 astronomy & astrophysics ,acceleration of particle ,MAGNETOSONIC SHOCK-WAVES ,acceleration of particles ,High Energy Astrophysical Phenomena (astro-ph.HE) ,Physics ,Spectral index ,TEV VARIABILITY ,[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE] ,Acceleradors de partícules ,Gamma ray ,individual (Mrk 501) [BL Lacertae objects] ,non-thermal [radiation mechanisms] ,BL LACERTAE OBJECTS ,ACTIVE GALACTIC NUCLEI ,LOG-PARABOLIC SPECTRA ,X-RAY ,active [galaxies] ,Eddington luminosity ,BL Lacertae objects: individual: Mrk 501 ,symbols ,Spectral energy distribution ,Electrónica ,Física nuclear ,Electricidad ,Astrophysics - High Energy Astrophysical Phenomena ,[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE] ,Astrophysics::High Energy Astrophysical Phenomena ,galaxies: active ,FOS: Physical sciences ,Astrophysics::Cosmology and Extragalactic Astrophysics ,symbols.namesake ,0103 physical sciences ,Blazar ,98.70.Rz, 98.54.Cm, 98.62.Py ,BL Lacertae objects: general ,gamma rays: general ,radiation mechanisms: non-thermal ,general [BL Lacertae objects] ,010308 nuclear & particles physics ,Gamma rays ,Institut für Physik und Astronomie ,Astronomy and Astrophysics ,Galaxies ,Particle accelerators ,Galàxies ,Space and Planetary Science ,ddc:520 ,general [gamma rays] ,Fermi Gamma-ray Space Telescope - Abstract
著者人数:451名, Accepted: 2010-11-19, 資料番号: SA1002653000
128. FORMOLIZATION OF PURIFIED AND CONCENTRATED DIPHTHERIA TOXIN
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ARMY FOREIGN SCIENCE AND TECHNOLOGY CENTER CHARLOTTESVILLE VA, Larionova, L. V., Vasilev, N. N., Vorobev, A. A., Kalinskaya, N. A., Chebotareva, S. V., ARMY FOREIGN SCIENCE AND TECHNOLOGY CENTER CHARLOTTESVILLE VA, Larionova, L. V., Vasilev, N. N., Vorobev, A. A., Kalinskaya, N. A., and Chebotareva, S. V.
- Abstract
A method for detoxication of diphtheria toxin by a preliminary culture formolization followed by purification of the antigen and final detoxication of the toxin in a purified, concentrated condition is discussed. (Author), Trans. of Vaktsiny i Syvorotki: Materialy po Proizvodstvu (USSR) n6 p81-91 1966.
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- 1968
129. DETOXICATION OF A PURIFIED AND CONCENTRATED DIPHTHERIA TOXIN BY FORMALIN
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ARMY FOREIGN SCIENCE AND TECHNOLOGY CENTER WASHINGTON D C, Larionova,L. V., Vasilev,N. N., Vorobev,A. A., Kalinskaya,N. A., Chevotareva,S. V., ARMY FOREIGN SCIENCE AND TECHNOLOGY CENTER WASHINGTON D C, Larionova,L. V., Vasilev,N. N., Vorobev,A. A., Kalinskaya,N. A., and Chevotareva,S. V.
- Abstract
Results are presented from a study of the preparation of purified and concentrated diphtheria anatoxin by detoxication of purified toxin. Acid precipitation was used to purify the toxin. Loss of activity in the supernatant fluid and the precipitate did not exceed 8-10%. Depigmented, sterile solutions of purified diphtheria toxin were used for further study of conditions of detoxication, including the role of pH in the conversion of purified toxin to anatoxin. The most favorable results of detoxication were obtained at pH 7.0-7.2. (Author)
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- 1969
130. Optical and near-IR brightening of the blazar PKS 1510-08 observed by the GASP
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Massimo Villata, Raiteri, C. M., Larionov, V. M., Gorshanov, D., Konstantinova, T. S., Kopatskaya, E. N., Larionova, L. V., Chen, W. P., Koptelova, E., Nilsson, K., and Pasanen, M.
131. Investigation of the correlation patterns and the Compton dominance variability of Mrk 421 in 2017
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Acciari, V. A., Ansoldi, S., Antonelli, L. A., Engels, A. Arbet, Artero, M., Asano, K., Babi��, A., Baquero, A., de Almeida, U. Barres, Barrio, J. A., Batkovi��, I., Gonz��lez, J. Becerra, Bednarek, W., Bellizzi, L., Bernardini, E., Bernardos, M., Berti, A., Besenrieder, J., Bhattacharyya, W., Bigongiari, C., Blanch, O., Bo��njak, Z., Busetto, G., Carosi, R., Ceribella, G., Cerruti, M., Chai, Y., Chilingarian, A., Cikota, S., Colak, S. M., Colombo, E., Contreras, J. L., Cortina, J., Covino, S., D'Amico, G., D'Elia, V., Da Vela, P., Dazzi, F., De Angelis, A., De Lotto, B., Delfino, M., Delgado, J., Mendez, C. Delgado, Depaoli, D., Di Pierro, F., Di Venere, L., Do Souto Espi��eira, E., Prester, D. Dominis, Donini, A., Doro, M., Ramazani, V. Fallah, Fattorini, A., Ferrara, G., Fonseca, M. V., Font, L., Fruck, C., Fukami, S., L��pez, R. J. Garc��a, Garczarczyk, Markus, Gasparyan, S., Gaug, M., Giglietto, N., Giordano, F., Gliwny, P., Godinovi��, N., Green, J. G., Green, D., Hadasch, D., Hahn, A., Heckmann, L., Herrera, J., Hoang, J., Hrupec, D., H��tten, M., Inada, T., Inoue, S., Ishio, K., Iwamura, Y., Jim��nez, I., Jormanainen, J., Jouvin, L., Kajiwara, Y., Karjalainen, M., Kerszberg, D., Kobayashi, Y., Kubo, H., Kushida, J., Lamastra, A., Lelas, D., Leone, F., Lindfors, E., Lombardi, S., Longo, F., L��pez-Coto, R., L��pez-Moya, M., L��pez-Oramas, A., Loporchio, S., de Oliveira Fraga, B. Machado, Maggio, C., Majumdar, P., Makariev, M., Mallamaci, M., Maneva, G., Manganaro, M., Maraschi, L., Mariotti, M., Mart��nez, M., Mazin, D., Menchiari, S., Mender, S., Mi��anovi��, S., Miceli, D., Miener, T., Minev, M., Miranda, J. M., Mirzoyan, R., Molina, E., Moralejo, A., Morcuende, D., Moreno, V., Moretti, E., Neustroev, V., Nigro, C., Nilsson, K., Nishijima, K., Noda, K., Nozaki, S., Ohtani, Y., Oka, T., Otero-Santos, J., Paiano, S., Palatiello, M., Paneque, D., Paoletti, R., Paredes, J. M., Pavleti��, L., Pe��il, P., Perennes, C., Persic, M., Moroni, P. G. Prada, Prandini, E., Priyadarshi, C., Puljak, I., Rib��, M., Rico, J., Righi, C., Rugliancich, A., Saha, L., Sahakyan, N., Saito, T., Sakurai, S., Satalecka, K., Saturni, F. G., Schmidt, K., Schweizer, T., Sitarek, J., ��nidari��, I., Sobczynska, D., Spolon, A., Stamerra, A., Strom, D., Strzys, M., Suda, Y., Suri��, T., Takahashi, M., Tavecchio, F., Temnikov, P., Terzi��, T., Teshima, M., Tosti, L., Truzzi, S., Tutone, A., Ubach, S., van Scherpenberg, J., Vanzo, G., Acosta, M. Vazquez, Ventura, S., Verguilov, V., Vigorito, C. F., Vitale, V., Vovk, I., Will, M., Wunderlich, C., Zari��, D., Baack, D., Balbo, M., Biederbeck, N., Biland, A., Bretz, T., Buss, J., Dorner, D., Eisenberger, L., Elsaesser, D., Hildebrand, D., Iotov, R., Mannheim, K., Neise, D., Noethe, M., Paravac, A., Rhode, W., Schleicher, B., Sliusar, V., Walter, R., D'Ammando, F., Horan, D., Lien, A. Y., Balokovi��, M., Madejski, G. M., Perri, M., Verrecchia, F., Leto, C., L��hteenm��ki, A., Tornikoski, M., Ramakrishnan, V., J��rvel��, E., Vera, R. J. C., Chamani, W., Villata, M., Raiteri, C. M., Gupta, A. C., Pandey, A., Fuentes, A., Agudo, I., Casadio, C., Semkov, E., Ibryamov, S., Marchini, A., Bachev, R., Strigachev, A., Ovcharov, E., Bozhilov, V., Valcheva, A., Zaharieva, E., Damljanovic, G., Vince, O., Larionov, V. M., Borman, G. A., Grishina, T. S., Hagen-Thorn, V. A., Kopatskaya, E. N., Larionova, E. G., Larionova, L. V., Morozova, D. A., Nikiforova, A. A., Savchenko, S. S., Troitskiy, I. S., Troitskaya, Y. V., Vasilyev, A. A., Merkulova, O. A., Chen, W. P., Samal, M., Lin, H. C., Moody, J. W., Sadun, A. C., Jorstad, S. G., Marscher, A. P., Weaver, Z. R., Feige, M., Kania, J., Kopp, M., Kunkel, L., Reinhart, D., Scherbantin, A., Schneider, L., Lorey, C., Acosta-Pulido, J. A., Carnerero, M. I., Carosati, D., Kurtanidze, S. O., Kurtanidze, O. M., Nikolashvili, M. G., Chanishvili, R. G., Chigladze, R. A., Ivanidze, R. Z., Kimeridze, G. N., Sigua, L. A., Joner, M. D., Spencer, M., Giroletti, M., Marchili, N., Righini, S., Rizzi, N., and Bonnoli, G.
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electron ,galaxies: active ,flux: correlation ,GeV ,radiation mechanisms: non-thermal ,7. Clean energy ,MAGIC ,GLAST ,blazar ,gamma ray: VHE ,ultraviolet ,optical ,spectral ,TeV ,BL Lacertae objects: individual: Mrk 421 ,X-ray: flux ,model: leptonic ,Lorentz - Abstract
Astronomy and astrophysics 655, A89 (2021). doi:10.1051/0004-6361/202141004, Aims. We present a detailed characterisation and theoretical interpretation of the broadband emission of the paradigmatic TeV blazar Mrk 421, with a special focus on the multi-band flux correlations.Methods. The dataset has been collected through an extensive multi-wavelength campaign organised between 2016 December and 2017 June. The instruments involved are MAGIC, FACT, Fermi-LAT, Swift, GASP-WEBT, OVRO, Medicina, and Mets��hovi. Additionally, four deep exposures (several hours long) with simultaneous MAGIC and NuSTAR observations allowed a precise measurement of the falling segments of the two spectral components.Results. The very-high-energy (VHE; E > 100 GeV) gamma rays and X-rays are positively correlated at zero time lag, but the strength and characteristics of the correlation change substantially across the various energy bands probed. The VHE versus X-ray fluxes follow different patterns, partly due to substantial changes in the Compton dominance for a few days without a simultaneous increase in the X-ray flux (i.e., orphan gamma-ray activity). Studying the broadband spectral energy distribution (SED) during the days including NuSTAR observations, we show that these changes can be explained within a one-zone leptonic model with a blob that increases its size over time. The peak frequency of the synchrotron bump varies by two orders of magnitude throughout the campaign. Our multi-band correlation study also hints at an anti-correlation between UV-optical and X-ray at a significance higher than 3��. A VHE flare observed on MJD 57788 (2017 February 4) shows gamma-ray variability on multi-hour timescales, with a factor ten increase in the TeV flux but only a moderate increase in the keV flux. The related broadband SED is better described by a two-zone leptonic scenario rather than by a one-zone scenario. We find that the flare can be produced by the appearance of a compact second blob populated by high energetic electrons spanning a narrow range of Lorentz factors, from �����$_{min}$=2��10$^4$ to �����$_{max}$=6��10$^5$.Key words: galaxies: active / BL Lacertae objects: individual: Mrk 421 / radiation mechanisms: non-thermal��� Light curves and spectral energy distributions data are only available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/cat/J/A+A/655/A89������ Corresponding authors: A. Arbet Engels and D. Paneque; e-mail: contact.magic@mpp.mpg.de.��������� Also member of the MAGIC Collaboration.������������ Also member of the FACT Collaboration., Published by EDP Sciences, Les Ulis
132. Optical rebrightening of the blazar AO 0235+16 observed by the GASP
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Villata, M., Claudia Maria Raiteri, Larionov, V. M., Konstantinova, T. S., Kopatskaya, E. N., Larionova, L., Chen, W. P., Koptelova, E., Nilsson, K., Pasanen, M., Ligustri, R., Böttcher, M., Roustazadeh, P., and Diltz, C.
133. Observations of the recent disc loss in X Persei: Photometry and polarimetry
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Roche, P., Larionov, V., Tarasov, A. E., Fabregat, J., Clark, J. S., Coe, M. J., Kalv, P., Larionova, L., Negueruela, I., Norton, A. J., and Pablo Reig
134. VizieR Online Data Catalog: Mrk 421 multi-wavelength variability, 2007-2009 (Ahnen+, 2016)
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Ahnen, M. L., Ansoldi, S., Antonelli, L. A., Antoranz, P., Babic, A., Banerjee, B., Bangale, P., Barres Almeida, U., Barrio, J. A., Becerra Gonzalez, J., Bednarek, W., Bernardini, E., Biasuzzi, B., Biland, A., Blanch, O., Bonnefoy, S., Bonnoli, G., Borracci, F., Bretz, T., Buson, S., Carosi, A., Chatterjee, A., Clavero, R., Colin, P., Colombo, E., Contreras, J. L., Cortina, J., Covino, S., Da Vela, P., Dazzi, F., Angelis, A., Lotto, B., Ona Wilhelmi, E., Di Pierro, F., Dominguez, A., Dominis Prester, D., Dorner, D., Doro, M., Einecke, S., Eisenacher Glawion, D., Elsaesser, D., Fernandez-Barral, A., Fidalgo, D., Fonseca, M. V., Font, L., Frantzen, K., Fruck, C., Galindo, D., Garcia Lopez, R. J., Garczarczyk, M., Garrido Terrats, D., Gaug, M., Giammaria, P., Godinovic, N., Gonzalez Munoz, A., Gora, D., Guberman, D., Hadasch, D., Hahn, A., Hanabata, Y., Hayashida, M., Herrera, J., Hose, J., Hrupec, D., Hughes, G., Idec, W., Kodani, K., Konno, Y., Kubo, H., Kushida, J., La Barbera, A., Lelas, D., Lindfors, E., Lombardi, S., Longo, F., Lopez, M., Lopez-Coto, R., Majumdar, P., Makariev, M., Mallot, K., Maneva, G., Manganaro, M., Mannheim, K., Maraschi, L., Benito Marcote, Mariotti, M., Martinez, M., Mazin, D., Menzel, U., Miranda, J. M., Mirzoyan, R., Moralejo, A., Moretti, E., Nakajima, D., Neustroev, V., Niedzwiecki, A., Nievas Rosillo, M., Nilsson, K., Nishijima, K., Noda, K., Nogues, L., Orito, R., Overkemping, A., Paiano, S., Palacio, J., Palatiello, M., Paneque, D., Paoletti, R., Paredes, J. M., Paredes-Fortuny, X., Pedaletti, G., Perri, L., Persic, M., Poutanen, J., Prada Moroni, P. G., Prandini, E., Puljak, I., Rhode, W., Ribo, M., Rico, J., Rodriguez Garcia, J., Saito, T., Satalecka, K., Schultz, C., Schweizer, T., Shore, S. N., Sillanpaa, A., Sitarek, J., Snidaric, I., Sobczynska, D., Stamerra, A., Steinbring, T., Strzys, M., Takalo, L., Takami, H., Tavecchio, F., Temnikov, P., Terzic, T., Tescaro, D., Teshima, M., Thaele, J., Torres, D. F., Toyama, T., Treves, A., Verguilov, V., Vovk, I., Ward, J. E., Will, M., Wu, M. H., Zanin, R., Magic, Collaboration, Blinov, D. A., Chen, W. P., Efimova, N. V., Forne, E., Grishina, T. S., Hovatta, T., Jordan, B., Kimeridze, G. N., Kopatskaya, E. N., Koptelova, E., Kurtanidze, O. M., Kurtanidze, S. O., Lahteenmaki, A., Larionov, V. M., Larionova, E. G., Larionova, L. V., Ligustri, R., Lin, H. C. Mcbreen B., Morozova, D. A., Nikolashvili, M. G., Raiteri, C. M., Ros, J. A., Sadun, A. C., Sigua, L. A., Tornikoski, M., Troitsky, I. S., and Villata, M.
135. GASP detection of an optical flare of the blazar S5 0716+71
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Carosati, D., Larionov, V. M., Larionova, L., Ros, J. A., Massimo Villata, and Raiteri, C. M.
136. Unravelling the complex behavior of Mrk 421 with simultaneous X-ray and VHE observations during an extreme flaring activity in April 2013
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Acciari, V. A., Ansoldi, S., Antonelli, L. A., Arbet Engels, A., Baack, D., Babić, A., Banerjee, B., Barres De Almeida, U., Barrio, J. A., Becerra González, J., Bednarek, W., Bellizzi, L., Bernardini, E., Berti, A., Besenrieder, J., Bhattacharyya, W., Bigongiari, C., Biland, A., Blanch, O., Bonnoli, G., Bošnjak, Ž., Busetto, G., Carosi, R., Ceribella, G., Cerruti, M., Chai, Y., Chilingarian, A., Cikota, S., Colak, S. M., Colin, U., Colombo, E., Contreras, J. L., Cortina, J., Covino, S., D'Elia, V., Da Vela, P., Dazzi, F., De Angelis, A., De Lotto, B., Del Puppo, F., Delfino, M., Delgado, J., Depaoli, D., Di Pierro, F., Di Venere, L., Do Souto Espiñeira, E., Dominis Prester, D., Donini, A., Dorner, D., Doro, M., Elsaesser, D., Fallah Ramazani, V., Fattorini, A., Ferrara, G., Foffano, L., Fonseca, M. V., Font, L., Fruck, C., Fukami, S., García López, R. J., Garczarczyk, Markus, Gasparyan, S., Gaug, M., Giglietto, N., Giordano, F., Gliwny, P., Godinović, N., Green, D., Hadasch, D., Hahn, A., Herrera, J., Hoang, J., Hrupec, D., Hütten, M., Inada, T., Inoue, S., Ishio, K., Iwamura, Y., Jouvin, L., Kajiwara, Y., Kerszberg, D., Kobayashi, Y., Kubo, H., Kushida, J., Lamastra, A., Lelas, D., Leone, F., Lindfors, E., Lombardi, S., Longo, F., López, M., López-Coto, R., López-Oramas, A., Loporchio, S., Machado De Oliveira Fraga, B., Maggio, C., Majumdar, P., Makariev, M., Mallamaci, M., Maneva, G., Manganaro, M., Mannheim, K., Maraschi, L., Mariotti, M., Martínez, M., Mazin, D., Mender, S., Mićanović, S., Miceli, D., Miener, T., Minev, M., Miranda, J. M., Mirzoyan, R., Molina, E., Moralejo, A., Morcuende, D., Moreno, V., Moretti, E., Munar-Adrover, P., Neustroev, V., Nigro, C., Nilsson, K., Ninci, D., Nishijima, K., Noda, K., Nogués, L., Nozaki, S., Ohtani, Y., Oka, T., Otero-Santos, J., Palatiello, M., Paneque, D., Paoletti, R., Paredes, J. M., Pavletić, L., Peñil, P., Peresano, M., Persic, M., Prada Moroni, P. G., Prandini, E., Puljak, I., Rhode, W., Ribó, M., Rico, J., Righi, C., Rugliancich, A., Saha, L., Sahakyan, N., Saito, T., Sakurai, S., Satalecka, K., Schleicher, B., Schmidt, K., Schweizer, T., Sitarek, J., Šnidarić, I., Sobczynska, D., Spolon, A., Stamerra, A., Strom, D., Strzys, M., Suda, Y., Surić, T., Takahashi, M., Tavecchio, F., Temnikov, P., Terzić, T., Teshima, M., Torres-Albà, N., Tosti, L., Van Scherpenberg, J., Vanzo, G., Vazquez Acosta, M., Ventura, S., Verguilov, V., Vigorito, C. F., Vitale, V., Vovk, I., Will, M., Zarić, D., Petropoulou, M., Finke, J., D'Ammando, F., Baloković, M., Madejski, G., Mori, K., Puccetti, Simonetta, Leto, C., Perri, M., Verrecchia, F., Villata, M., Raiteri, C. M., Agudo, I., Bachev, R., Berdyugin, A., Blinov, D. A., Chanishvili, R., Chen, W. P., Chigladze, R., Damljanovic, G., Eswaraiah, C., Grishina, T. S., Ibryamov, S., Jordan, B., Jorstad, S. G., Joshi, M., Kopatskaya, E. N., Kurtanidze, O. M., Kurtanidze, S. O., Larionova, E. G., Larionova, L. V., Larionov, V. M., Latev, G., Lin, H. C., Marscher, A. P., Mokrushina, A. A., Morozova, D. A., Nikolashvili, M. G., Semkov, E., Smith, P. S., Strigachev, A., Troitskaya, Yu. V., Troitsky, I. S., Vince, O., Barnes, J., Güver, T., Moody, J. W., Sadun, A. C., Hovatta, T., Richards, J. L., Max-Moerbeck, W., Readhead, A. C. R., Lähteenmäki, A., Tornikoski, M., Tammi, J., Ramakrishnan, V., and Reinthal, R.
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13. Climate action ,7. Clean energy - Abstract
The astrophysical journal / Supplement series Supplement series 248(2), 29 - (2020). doi:10.3847/1538-4365/ab89b5, We report on a multiband variability and correlation study of the TeV blazar Mrk 421 during an exceptional flaring activity observed from 2013 April 11 to 19. The study uses, among others, data from GLAST-AGILE Support Program (GASP) of the Whole Earth Blazar Telescope (WEBT), Swift, Nuclear Spectroscopic Telescope Array (NuSTAR), Fermi Large Area Telescope, Very Energetic Radiation Imaging Telescope Array System (VERITAS), and Major Atmospheric Gamma Imaging Cherenkov (MAGIC). The large blazar activity and the 43 hr of simultaneous NuSTAR and MAGIC/VERITAS observations permitted variability studies on 15 minute time bins over three X-ray bands (3–7 keV, 7–30 keV, and 30–80 keV) and three very-high-energy (VHE; >0.1 TeV) gamma-ray bands (0.2–0.4 TeV, 0.4–0.8 TeV, and >0.8 TeV). We detected substantial flux variations on multi-hour and sub-hour timescales in all of the X-ray and VHE gamma-ray bands. The characteristics of the sub-hour flux variations are essentially energy independent, while the multi-hour flux variations can have a strong dependence on the energy of the X-rays and the VHE gamma-rays. The three VHE bands and the three X-ray bands are positively correlated with no time lag, but the strength and characteristics of the correlation change substantially over time and across energy bands. Our findings favor multi-zone scenarios for explaining the achromatic/chromatic variability of the fast/slow components of the light curves, as well as the changes in the flux–flux correlation on day-long timescales. We interpret these results within a magnetic reconnection scenario, where the multi-hour flux variations are dominated by the combined emission from various plasmoids of different sizes and velocities, while the sub-hour flux variations are dominated by the emission from a single small plasmoid moving across the magnetic reconnection layer., Published by Univ. of Chicago Press11033, Chicago, Ill. [u.a.]
137. Optical and near-IR brightening of the blazar 3C 66A detected by the GASP
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Larionov, V. M., Massimo Villata, Raiteri, C. M., Gorshanov, D., Konstantinova, T. S., Kopatskaya, E. N., Larionova, L., Chen, W. P., and Koptelova, E.
138. Multi-wavelength characterization of the blazar S5 0716+714 during an unprecedented outburst phase
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Ahnen, M. L., Ansoldi, S., Antonelli, L. A., Arcaro, C., Baack, D., Babić, A., Banerjee, B., Bangale, P., Barres De Almeida, U., Barrio, J. A., Becerra González, J., Bednarek, W., Bernardini, E., Ch Berse, R., Berti, A., Bhattacharyya, W., Biland, A., Blanch, O., Bonnoli, G., Carosi, R., Carosi, A., Ceribella, G., Chatterjee, A., Colak, S. M., Colin, P., Colombo, E., Contreras, J. L., Cortina, J., Covino, S., Cumani, P., Da Vela, P., Dazzi, F., De Angelis, A., De Lotto, B., Delfino, M., Delgado, J., Di Pierro, F., Domínguez, A., Dominis Prester, D., Dorner, D., Doro, M., Einecke, S., Elsaesser, D., Fallah Ramazani, V., Fernández-Barral, A., Fidalgo, D., Fonseca, M. V., Font, L., Fruck, C., Galindo, D., Gallozzi, S., García López, R. J., Garczarczyk, M., Gaug, M., Giammaria, P., Godinović, N., Gora, D., Guberman, D., Hadasch, D., Hahn, A., Hassan, T., Hayashida, M., Herrera, J., Hose, J., Hrupec, D., Ishio, K., Konno, Y., Kubo, H., Kushida, J., Kuveždić, D., Lelas, D., Lindfors, E., Lombardi, S., Longo, F., López, M., Maggio, C., Majumdar, P., Makariev, M., Maneva, G., Manganaro, M., Mannheim, K., Maraschi, L., Mariotti, M., Martínez, M., Masuda, S., Mazin, D., Mielke, K., Minev, M., Miranda, J. M., Mirzoyan, R., Moralejo, A., Moreno, V., Moretti, E., Nagayoshi, T., Neustroev, V., Niedzwiecki, A., Nievas Rosillo, M., Nigro, C., Nilsson, K., Ninci, D., Nishijima, K., Noda, K., Nogués, L., Paiano, S., Palacio, J., Paneque, D., Paoletti, R., Paredes, J. M., Pedaletti, G., Peresano, M., Persic, M., Prada Moroni, P. G., Prandini, E., Puljak, I., Garcia, J. R., Reichardt, I., Rhode, W., Ribó, M., Rico, J., Righi, C., Rugliancich, A., Saito, T., Satalecka, K., Schweizer, T., Sitarek, J., Šnidarić, I., Sobczynska, D., Stamerra, A., Strzys, M., Surić, T., Takahashi, M., Takalo, L., Tavecchio, F., Temnikov, P., Terzić, T., Teshima, M., Torres-Albà, N., Treves, A., Tsujimoto, S., Vanzo, G., Vazquez Acosta, M., Vovk, I., Ward, J. E., Will, M., Zarić, D., Bastieri, D., Gasparrini, D., Lott, B., Rani, B., Thompson, D. J., Agudo, I., Angelakis, E., Borman, G. A., Casadio, C., Grishina, T. S., Gurwell, M., Hovatta, T., Itoh, R., Järvelä, E., Jermak, H., Jorstad, S., Kopatskaya, E. N., Kraus, A., Krichbaum, T. P., Kuin, N. P. M., Lähteenmäki, A., Larionov, V. M., Larionova, L. V., Lien, A. Y., Madejski, G., Marscher, A., Myserlis, I., Max-Moerbeck, W., Molina, S. N., Morozova, D. A., Nalewajko, K., Pearson, T. J., Ramakrishnan, V., Readhead, A. C. S., Reeves, R. A., Savchenko, S. S., Steele, I. A., Tornikoski, M., Troitskaya, Yu. V., Troitsky, I., Vasilyev, A. A., and Anton Zensus, J.
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7. Clean energy - Abstract
Astronomy and astrophysics 619, A45 (2018). doi:10.1051/0004-6361/201832677, Context. The BL Lac object S5 0716+714, a highly variable blazar, underwent an impressive outburst in January 2015 (Phase A), followed by minor activity in February (Phase B). The MAGIC observations were triggered by the optical flux observed in Phase A, corresponding to the brightest ever reported state of the source in the R-band.Aims.The comprehensive dataset collected is investigated in order to shed light on the mechanism of the broadband emission.Methods. Multi-wavelength light curves have been studied together with the broadband spectral energy distributions (SEDs). The sample includes data from Effelsberg, OVRO, Metsähovi, VLBI, CARMA, IRAM, SMA, Swift-UVOT, KVA, Tuorla, Steward, RINGO3, KANATA, AZT-8+ST7, Perkins, LX-200, Swift-XRT, NuSTAR, Fermi-LAT and MAGIC.Results. The flaring state of Phase A was detected in all the energy bands, providing for the first time a multi-wavelength sample of simultaneous data from the radio band to the very-high-energy (VHE, E > 100 GeV). In the constructed SED, the Swift-XRT+NuSTAR data constrain the transition between the synchrotron and inverse Compton components very accurately, while the second peak is constrained from 0.1 GeV to 600 GeV by Fermi+MAGIC data. The broadband SED cannot be described with a one-zone synchrotron self-Compton model as it severely underestimates the optical flux in order to reproduce the X-ray to γ-ray data. Instead we use a two-zone model. The electric vector position angle (EVPA) shows an unprecedented fast rotation. An estimation of the redshift of the source by combined high-energy (HE, 0.1 GeV < E < 100 GeV) and VHE data provides a value of z = 0.31 ± 0.02$_{stats}$ ± 0.05$_{sys}$, confirming the literature value.Conclusions. The data show the VHE emission originating in the entrance and exit of a superluminal knot in and out of a recollimation shock in the inner jet. A shock–shock interaction in the jet seems responsible for the observed flares and EVPA swing. This scenario is also consistent with the SED modeling., Published by EDP Sciences, Les Ulis
139. GASP detection of a high optical state of the blazar PKS 1510-08
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Carosati, D., Larionov, V. M., Larionova, L., Villata, M., and Claudia Maria Raiteri
140. GASP observation of a spectacular optical-to-radio brightening of the blazar AO 0235+16
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Villata, M., Claudia Maria Raiteri, Carosati, D., Chen, W. P., Koptelova, E., Larionov, V. M., Gorshanov, D., Konstantinova, T. S., Kopatskaya, E. N., Larionova, L., Nilsson, K., Pasanen, M., Gurwell, M. A., Leto, P., Buemi, C. S., Trigilio, C., Umana, G., Aller, M. F., and Aller, H. D.
141. MAGIC and H.E.S.S. detect VHE gamma rays from the blazar OT 081 for the first time: a deep multiwavelength study
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Seglar-Arroyo, M., Sanchez, D., Esteban Gutierrez, A., Agudo, I., Ciprini, S., Filippenko, A. V., Hovatta, T., Jermak, H., Jorstad, S. G., Kopatskaya, E. N., Lähteenmäki, A., Larionov, V. M., Larionova, L. V., Marscher, A., Morozova, D. A., Pahljina, M., Tornikoski, M., Troitskaya, Yu V., Troitsky, I., Verrecchia, F., Weaver, Z. R., Xiao, H. B., Zheng, W., Acciari, V. A., Ansoldi, S., Antonelli, L. A., Arbet Engels, A., Artero, M., Asano, K., Baack, D., Babić, A., Baquero, A., Barres Almeida, U., Barrio, J. A., Batković, I., Becerra González, J., Bednarek, W., Bellizzi, L., Bernardini, E., Bernardos, M., Berti, A., Besenrieder, J., Bhattacharyya, W., Bigongiari, C., Biland, A., Blanch, O., Bökenkamp, H., Bonnoli, G., Bošnjak, Ž, Busetto, G., Carosi, R., Ceribella, G., Cerruti, M., Chai, Y., Chilingarian, A., Cikota, S., Colak, S. M., Colombo, E., Contreras, J. L., Cortina, J., Covino, S., D Amico, G., D Elia, V., Da Vela, P., Dazzi, F., Angelis, A., Lotto, B., Delfino, M., Delgado, J., Delgado Mendez, C., Depaoli, D., Di Pierro, F., Di Venere, L., Do Souto Espiñeira, E., Dominis Prester, D., Donini, A., Dorner, D., Doro, M., Elsaesser, D., Fallah Ramazani, V., Fattorini, A., Fonseca, M. V., Font, L., Fruck, C., Fukami, S., Fukazawa, Y., García López, R. J., Garczarczyk, M., Gasparyan, S., Gaug, M., Giglietto, N., Giordano, F., Gliwny, P., Godinović, N., Green, J. G., Green, D., Hadasch, D., Hahn, A., Heckmann, L., Herrera, J., Hoang, J., Hrupec, D., Hütten, M., Inada, T., Ishio, K., Iwamura, Y., Jiménez Martínez, I., Jormanainen, J., Jouvin, L., Karjalainen, M., Kerszberg, D., Kobayashi, Y., Kubo, H., Kushida, J., Lamastra, A., Lelas, D., Leone, F., Lindfors, E., Linhoff, L., Lombardi, S., Longo, F., López-Coto, R., López-Moya, M., López-Oramas, A., Loporchio, S., Machado Oliveira Fraga, B., Maggio, C., Majumdar, P., Makariev, M., Mallamaci, M., Maneva, G., Manganaro, M., Mannheim, K., Maraschi, L., Mariotti, M., Martínez, M., Mazin, D., Menchiari, S., Mender, S., Mićanović, S., Miceli, D., Miener, T., Miranda, J. M., Mirzoyan, R., Molina, E., Moralejo, A., Morcuende, D., Moreno, V., Moretti, E., Nakamori, T., Nava, L., Neustroev, V., Nigro, C., Nilsson, K., Nishijima, K., Noda, K., Nozaki, S., Ohtani, Y., Oka, T., Otero-Santos, J., Paiano, S., Palatiello, M., Paneque, D., Paoletti, R., Paredes, J. M., Pavletić, L., Peñil, P., Persic, M., Pihet, M., Prada Moroni, P. G., Prandini, E., Priyadarshi, C., Puljak, I., Rhode, W., Ribó, M., Rico, J., Righi, C., Rugliancich, A., Sahakyan, N., Saito, T., Sakurai, S., Satalecka, K., Saturni, F. G., Schleicher, B., Schmidt, K., Schweizer, T., Sitarek, J., Šnidarić, I., Dorota Sobczynska, Spolon, A., Stamerra, A., Strišković, J., Strom, D., Strzys, M., Suda, Y., Surić, T., Takahashi, M., Takeishi, R., Tavecchio, F., Temnikov, P., Terzić, T., Teshima, M., Tosti, L., Truzzi, S., Tutone, A., Ubach, S., Scherpenberg, J., Vanzo, G., Vazquez Acosta, M., Ventura, S., Verguilov, V., Vigorito, C. F., Vitale, V., Vovk, I., Will, M., Wunderlich, C., Yamamoto, T., and Zarić, D.
142. AGILE, Fermi, Swift, and GASP/WEBT multi-wavelength observations of the high-redshift blazar 4C +71.07 in outburst
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Vercellone S., Romano P., Piano G., Vittorini V., Donnarumma I., Munar-Adrover P., Raiteri C., Villata M., Verrecchia F., Lucarelli F., Pittori C., Bulgarelli A., Fioretti V., Tavani M., Acosta-Pulido J., Agudo I., Arkharov A., Bach U., Bachev R., Borman G., Butuzova M., Carnerero M., Casadio C., Damljanovic G., D'Ammando F., Di Paola A., Doroshenko V., Efimova N., Ehgamberdiev S., Giroletti M., Gómez J., Grishina T., Järvelä E., Klimanov S., Kopatskaya E., Kurtanidze O., Lähteenmäki A., Larionov V., Larionova L., Mihov B., Mirzaqulov D., Molina S., Morozova D., Nazarov S., Orienti M., Righini S., Savchenko S., Semkov E., Slavcheva-Mihova L., Strigachev A., Tornikoski M., Troitskaya Y., Vince O., Cattaneo P., Colafrancesco S., Longo F., Morselli A., Paoletti F., Parmiggiani N., Vercellone S., Romano P., Piano G., Vittorini V., Donnarumma I., Munar-Adrover P., Raiteri C., Villata M., Verrecchia F., Lucarelli F., Pittori C., Bulgarelli A., Fioretti V., Tavani M., Acosta-Pulido J., Agudo I., Arkharov A., Bach U., Bachev R., Borman G., Butuzova M., Carnerero M., Casadio C., Damljanovic G., D'Ammando F., Di Paola A., Doroshenko V., Efimova N., Ehgamberdiev S., Giroletti M., Gómez J., Grishina T., Järvelä E., Klimanov S., Kopatskaya E., Kurtanidze O., Lähteenmäki A., Larionov V., Larionova L., Mihov B., Mirzaqulov D., Molina S., Morozova D., Nazarov S., Orienti M., Righini S., Savchenko S., Semkov E., Slavcheva-Mihova L., Strigachev A., Tornikoski M., Troitskaya Y., Vince O., Cattaneo P., Colafrancesco S., Longo F., Morselli A., Paoletti F., and Parmiggiani N.
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© ESO 2019. Context. The flat-spectrum radio quasar 4C +71.07 is a high-redshift (z = 2.172), γ-loud blazar whose optical emission is dominated by thermal radiation from the accretion disc. Aims. 4C +71.07 has been detected in outburst twice by the AGILE γ-ray satellite during the period from the end of October to mid-November 2015, when it reached a γ-ray flux of the order of F(E > 100 MeV)=(1.2 ± 0.3)×10 -6 photons cm -2 s -1 and F(E > 100 MeV)=(3.1 ± 0.6)×10 -6 photons cm -2 s -1 , respectively, allowing us to investigate the properties of the jet and the emission region. Methods. We investigated its spectral energy distribution by means of almost-simultaneous observations covering the cm, mm, near-infrared, optical, ultraviolet, X-ray, and γ-ray energy bands obtained by the GASP-WEBT Consortium and the Swift, AGILE, and Fermi satellites. Results. The spectral energy distribution of the second γ-ray flare (whose energy coverage is more dense) can be modelled by means of a one-zone leptonic model, yielding a total jet power of about 4 × 10 47 erg s -1 . Conclusions. During the most prominent γ-ray flaring period our model is consistent with a dissipation region within the broad-line region. Moreover, this class of high-redshift, flat-spectrum radio quasars with high-mass black holes might be good targets for future γ-ray satellites such as e-ASTROGAM.
143. Multiwavelength temporal and spectral variability of the blazar OJ 287 during and after the 2015 December flare: A major accretion disc contribution
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Hirochi J., Itoh R., Kawabata M., Kopatskaya E., Kurtanidze S., Larionova E., Larionova L., Mishra A., Morozova D., Nakaoka T., Nikolashvili M., Savchenko S., Troitskaya Y., Troitsky I., Vasilyev A., Hirochi J., Itoh R., Kawabata M., Kopatskaya E., Kurtanidze S., Larionova E., Larionova L., Mishra A., Morozova D., Nakaoka T., Nikolashvili M., Savchenko S., Troitskaya Y., Troitsky I., and Vasilyev A.
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© 2018 The Author(s). We present a multiwavelength spectral and temporal analysis of the blazar OJ 287 during its recent activity between 2015 December and 2016 May, showing strong variability in the nearinfrared (NIR) to X-ray energies with detection at γ -ray energies as well. Most of the optical flux variations exhibit strong changes in polarization angle and degree. All the interband time lags are consistent with simultaneous emissions. Interestingly, on days with excellent data coverage in the NIR-UV bands, the spectral energy distributions (SEDs) show signatures of bumps in the visible-UV bands, never seen before in this source. The optical bump can be explained as accretion-disc emission associated with the primary black hole of mass ~1.8 × 1010M⊙ while the little bump feature in the optical-UV appears consistent with line emission. Further, the broad-band SEDs extracted during the first flare and during a quiescent period during this span show very different γ -ray spectra compared to previously observed flare or quiescent spectra. The probable thermal bump in the visible seems to have been clearly present since 2013 May, as found by examining all available NIR-optical observations, and favours the binary supermassive black hole model. The simultaneous multiwavelength variability and relatively weak γ -ray emission that shows a shift in the SED peak is consistent with γ -ray emission originating from inverse Compton scattering of photons from the line emission that apparently contributes to the little blue bump.
144. The Bright γ-ray Flare of 3C 279 in 2015 June: AGILE Detection and Multifrequency Follow-up Observations
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Chen W., Ehgamberdiev S., Goded A., Grishina T., Hiriart D., Hsiao H., Jorstad S., Kimeridze G., Kopatskaya E., Kurtanidze O., Kurtanidze S., Larionov V., Larionova L., Marscher A., Mirzaqulov D., Morozova D., Nilsson K., Samal M., Sigua L., Spassov B., Strigachev A., Takalo L., Antonelli L., Bulgarelli A., Cattaneo P., Colafrancesco S., Giommi P., Longo F., Morselli A., Paoletti F., Chen W., Ehgamberdiev S., Goded A., Grishina T., Hiriart D., Hsiao H., Jorstad S., Kimeridze G., Kopatskaya E., Kurtanidze O., Kurtanidze S., Larionov V., Larionova L., Marscher A., Mirzaqulov D., Morozova D., Nilsson K., Samal M., Sigua L., Spassov B., Strigachev A., Takalo L., Antonelli L., Bulgarelli A., Cattaneo P., Colafrancesco S., Giommi P., Longo F., Morselli A., and Paoletti F.
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© 2018. The American Astronomical Society. All rights reserved.. We report the AGILE detection and the results of the multifrequency follow-up observations of a bright γ-ray flare of the blazar 3C 279 in 2015 June. We use AGILE and Fermi gamma-ray data, together with Swift X-ray andoptical-ultraviolet data, and ground-based GASP-WEBT optical observations, including polarization information, to study the source variability and the overall spectral energy distribution during the γ-ray flare. The γ-ray flaring data, compared with as yet unpublished simultaneous optical data that will allow constraints on the big blue bump disk luminosity, show very high Compton dominance values of ∼100, with the ratio of γ-ray to optical emission rising by a factor of three in a few hours. The multiwavelength behavior of the source during the flare challenges one-zone leptonic theoretical models. The new observations during the 2015 June flare are also compared with already published data and nonsimultaneous historical 3C 279 archival data.
145. Polarization angle swings in blazars: The case of 3C 279
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Kiehlmann S., Savolainen T., Jorstad S., Sokolovsky K., Schinzel F., Marscher A., Larionov V., Agudo I., Akitaya H., Benítez E., Berdyugin A., Blinov D., Bochkarev N., Borman G., Burenkov A., Casadio C., Doroshenko V., Efimova N., Fukazawa Y., Gómez J., Grishina T., Hagen-Thorn V., Heidt J., Hiriart D., Itoh R., Joshi M., Kawabata K., Kimeridze G., Kopatskaya E., Korobtsev I., Krajci T., Kurtanidze O., Kurtanidze S., Larionova E., Larionova L., Lindfors E., López J., McHardy I., Molina S., Moritani Y., Morozova D., Nazarov S., Nikolashvili M., Nilsson K., Pulatova N., Reinthal R., Sadun A., Sasada M., Savchenko S., Sergeev S., Sigua L., Smith P., Sorcia M., Spiridonova O., Takaki K., Takalo L., Taylor B., Troitsky I., Uemura M., Ugolkova L., Ui T., Yoshida M., Zensus J., Zhdanova V., Kiehlmann S., Savolainen T., Jorstad S., Sokolovsky K., Schinzel F., Marscher A., Larionov V., Agudo I., Akitaya H., Benítez E., Berdyugin A., Blinov D., Bochkarev N., Borman G., Burenkov A., Casadio C., Doroshenko V., Efimova N., Fukazawa Y., Gómez J., Grishina T., Hagen-Thorn V., Heidt J., Hiriart D., Itoh R., Joshi M., Kawabata K., Kimeridze G., Kopatskaya E., Korobtsev I., Krajci T., Kurtanidze O., Kurtanidze S., Larionova E., Larionova L., Lindfors E., López J., McHardy I., Molina S., Moritani Y., Morozova D., Nazarov S., Nikolashvili M., Nilsson K., Pulatova N., Reinthal R., Sadun A., Sasada M., Savchenko S., Sergeev S., Sigua L., Smith P., Sorcia M., Spiridonova O., Takaki K., Takalo L., Taylor B., Troitsky I., Uemura M., Ugolkova L., Ui T., Yoshida M., Zensus J., and Zhdanova V.
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© ESO, 2016.Context. Over the past few years, on several occasions, large, continuous rotations of the electric vector position angle (EVPA) of linearly polarized optical emission from blazars have been reported. These events are often coincident with high energy γ-ray flares and they have attracted considerable attention, since they could allow us to probe the magnetic field structure in the γ-ray emitting region of the jet. The flat-spectrum radio quasar 3C 279 is one of the most prominent examples showing this behaviour. Aims. Our goal is to study the observed EVPA rotations and to distinguish between a stochastic and a deterministic origin of the polarization variability. Methods. We have combined multiple data sets of R-band photometry and optical polarimetry measurements of 3C 279, yielding exceptionally well-sampled flux density and polarization curves that cover a period of 2008-2012. Several large EVPA rotations are identified in the data. We introduce a quantitative measure for the EVPA curve smoothness, which is then used to test a set of simple random walk polarization variability models against the data. Results. 3C 279 shows different polarization variation characteristics during an optical low-flux state and a flaring state. The polarization variation during the flaring state, especially the smooth ∼360° rotation of the EVPA in mid-2011, is not consistent with the tested stochastic processes. Conclusions. We conclude that, during the two different optical flux states, two different processes govern polarization variation, which is possibly a stochastic process during the low-brightness state and a deterministic process during the flaring activity.
146. Multiwavelength behaviour of the blazar OJ 248 from radio to γ -rays
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Carnerero M., Raiteri C., Villata M., Acosta-Pulido J., D'Ammando F., Smith P., Larionov V., Agudo I., Arévalo M., Arkharov A., Bach U., Bachev R., Benítez E., Blinov D., Bozhilov V., Buemi C., Bueno Bueno A., Carosati D., Casadio C., Chen W., Damljanovic G., Di Paola A., Efimova N., Ehgamberdiev S., Giroletti M., Gómez J., González-Morales P., Grinon-Marin A., Grishina T., Gurwell M., Hiriart D., Hsiao H., Ibryamov S., Jorstad S., Joshi M., Kopatskaya E., Kurtanidze O., Kurtanidze S., Lähteenmäki A., Larionova E., Larionova L., Lázaro C., Leto P., Lin C., Lin H., Manilla-Robles A., Marscher A., McHardy I., Metodieva Y., Mirzaqulov D., Mokrushina A., Molina S., Morozova D., Nikolashvili M., Orienti M., Ovcharov E., Panwar N., Pastor Yabar A., Puerto Giménez I., Ramakrishnan V., Richter G., Rossini M., Sigua L., Strigachev A., Taylor B., Tornikoski M., Trigilio C., Troitskaya Y., Troitsky I., Umana G., Valcheva A., Velasco S., Vince O., Wehrle A., Wiesemeyer H., Carnerero M., Raiteri C., Villata M., Acosta-Pulido J., D'Ammando F., Smith P., Larionov V., Agudo I., Arévalo M., Arkharov A., Bach U., Bachev R., Benítez E., Blinov D., Bozhilov V., Buemi C., Bueno Bueno A., Carosati D., Casadio C., Chen W., Damljanovic G., Di Paola A., Efimova N., Ehgamberdiev S., Giroletti M., Gómez J., González-Morales P., Grinon-Marin A., Grishina T., Gurwell M., Hiriart D., Hsiao H., Ibryamov S., Jorstad S., Joshi M., Kopatskaya E., Kurtanidze O., Kurtanidze S., Lähteenmäki A., Larionova E., Larionova L., Lázaro C., Leto P., Lin C., Lin H., Manilla-Robles A., Marscher A., McHardy I., Metodieva Y., Mirzaqulov D., Mokrushina A., Molina S., Morozova D., Nikolashvili M., Orienti M., Ovcharov E., Panwar N., Pastor Yabar A., Puerto Giménez I., Ramakrishnan V., Richter G., Rossini M., Sigua L., Strigachev A., Taylor B., Tornikoski M., Trigilio C., Troitskaya Y., Troitsky I., Umana G., Valcheva A., Velasco S., Vince O., Wehrle A., and Wiesemeyer H.
- Abstract
© 2015 The Authors. We present an analysis of the multiwavelength behaviour of the blazar OJ 248 at z = 0.939 in the period 2006-2013. We use low-energy data (optical, near-infrared, and radio) obtained by 21 observatories participating in the Gamma-Ray Large Area Space Telescope (GLAST)-AGILE Support Program of the Whole Earth Blazar Telescope, as well as data from the Swift (optical-UV and X-rays) and Fermi (γ -rays) satellites, to study flux and spectral variability and correlations among emissions in different bands. We take into account the effect of absorption by the Damped Lyman α intervening system at z = 0.525. Two major outbursts were observed in 2006-2007 and in 2012-2013 at optical and near-IR wavelengths, while in the high-frequency radio light curves prominent radio outbursts are visible peaking at the end of 2010 and beginning of 2013, revealing a complex radio-optical correlation. Crosscorrelation analysis suggests a delay of the optical variations after the γ -ray ones of about a month, which is a peculiar behaviour in blazars. We also analyse optical polarimetric and spectroscopic data. The average polarization percentage P is less than 3 per cent, but it reaches~19 per cent during the early stage of the 2012-2013 outburst.Avague correlation of P with brightness is observed. There is no preferred electric vector polarization angle and during the outburst the linear polarization vector shows wide rotations in both directions, suggesting a complex behaviour/structure of the jet and possible turbulence. The analysis of 140 optical spectra acquired at the Steward Observatory reveals a strong Mg II broad emission line with an essentially stable flux of 6.2 × 10-15 erg cm-2 s-1 and a full width at half-maximum of 2053 km s-1.
147. Variability of the blazar 4C 38.41 (B3 1633+382) from GHz frequencies to GeV energies
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Raiteri C., Villata M., Smith P., Larionov V., Acosta-Pulido J., Aller M., D'Ammando F., Gurwell M., Jorstad S., Joshi M., Kurtanidze O., Lähteenmäki A., Mirzaqulov D., Agudo I., Aller H., Arévalo M., Arkharov A., Bach U., Benítez E., Berdyugin A., Blinov D., Blumenthal K., Buemi C., Bueno A., Carleton T., Carnerero M., Carosati D., Casadio C., Chen W., Di Paola A., Dolci M., Efimova N., Ehgamberdiev S., Gómez J., González A., Hagen-Thorn V., Heidt J., Hiriart D., Holikov S., Konstantinova T., Kopatskaya E., Koptelova E., Kurtanidze S., Larionova E., Larionova L., León-Tavares J., Leto P., Lin H., Lindfors E., Marscher A., McHardy I., Molina S., Morozova D., Mujica R., Nikolashvili M., Nilsson K., Ovcharov E., Panwar N., Pasanen M., Puerto-Gimenez I., Reinthal R., Richter G., Ros J., Sakamoto T., Schwartz R., Sillanpää A., Smith N., Takalo L., Tammi J., Taylor B., Thum C., Tornikoski M., Trigilio C., Troitsky I., Umana G., Valcheva A., Wehrle A., Raiteri C., Villata M., Smith P., Larionov V., Acosta-Pulido J., Aller M., D'Ammando F., Gurwell M., Jorstad S., Joshi M., Kurtanidze O., Lähteenmäki A., Mirzaqulov D., Agudo I., Aller H., Arévalo M., Arkharov A., Bach U., Benítez E., Berdyugin A., Blinov D., Blumenthal K., Buemi C., Bueno A., Carleton T., Carnerero M., Carosati D., Casadio C., Chen W., Di Paola A., Dolci M., Efimova N., Ehgamberdiev S., Gómez J., González A., Hagen-Thorn V., Heidt J., Hiriart D., Holikov S., Konstantinova T., Kopatskaya E., Koptelova E., Kurtanidze S., Larionova E., Larionova L., León-Tavares J., Leto P., Lin H., Lindfors E., Marscher A., McHardy I., Molina S., Morozova D., Mujica R., Nikolashvili M., Nilsson K., Ovcharov E., Panwar N., Pasanen M., Puerto-Gimenez I., Reinthal R., Richter G., Ros J., Sakamoto T., Schwartz R., Sillanpää A., Smith N., Takalo L., Tammi J., Taylor B., Thum C., Tornikoski M., Trigilio C., Troitsky I., Umana G., Valcheva A., and Wehrle A.
- Abstract
Context. After years of modest optical activity, the quasar-type blazar 4C 38.41 (B3 1633+382) experienced a large outburst in 2011, which was detected throughout the entire electromagnetic spectrum, renewing interest in this source. Aims. We present the results of low-energy multifrequency monitoring by the GLAST-AGILE Support Program (GASP) of the Whole Earth Blazar Telescope (WEBT) consortium and collaborators, as well as those of spectropolarimetric/ spectrophotometric monitoring at the Steward Observatory. We also analyse high-energy observations of the Swift and Fermi satellites. This combined study aims to provide insights into the source broad-band emission and variability properties. Methods. We assemble optical, near-infrared, millimetre, and radio light curves and investigate their features and correlations. In the optical, we also analyse the spectroscopic and polarimetric properties of the source. We then compare the low-energy emission behaviour with that at high energies. Results. In the optical-UV band, several results indicate that there is a contribution from a quasi-stellar-object (QSO) like emission component, in addition to both variable and polarised jet emission. In the optical, the source is redder-when-brighter, at least for R a3; 16. The optical spectra display broad emission lines, whose flux is constant in time. The observed degree of polarisation increases with flux and is higher in the red than the blue. The spectral energy distribution reveals a bump peaking around the U band. The unpolarised emission component is likely thermal radiation from the accretion disc that dilutes the jet polarisation. We estimate its brightness to be R QSO ∼ 17.85-18 and derive the intrinsic jet polarisation degree. We find no clear correlation between the optical and radio light curves, while the correlation between the optical and γ-ray flux apparently fades in time, likely because of an increasing optical to γ-ray flux ratio. Conclusions. As suggested fo
148. Dissecting the long-term emission behaviour of the BL Lac object Mrk 421
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Carnerero M., Raiteri C., Villata M., Acosta-Pulido J., Larionov V., Smith P., D'Ammando F., Agudo I., Arévalo M., Bachev R., Barnes J., Boeva S., Bozhilov V., Carosati D., Casadio C., Chen W., Damljanovic G., Eswaraiah E., Forné E., Gantchev G., Gómez J., González-Morales P., Griñón-Marín A., Grishina T., Holden M., Ibryamov S., Joner M., Jordan B., Jorstad S., Joshi M., Kopatskaya E., Koptelova E., Kurtanidze O., Kurtanidze S., Larionova E., Larionova L., Latev G., Lázaro C., Ligustri R., Lin H., Marscher A., Martínez-Lombilla C., McBreen B., Mihov B., Molina S., Moody J., Morozova D., Nikolashvili M., Nilsson K., Ovcharov E., Pace C., Panwar N., Pastor Yabar A., Pearson R., Pinna F., Protasio C., Rizzi N., Redondo-Lorenzo F., Rodríguez-Coira G., Ros J., Sadun A., Savchenko S., Semkov E., Slavcheva-Mihova L., Smith N., Strigachev A., Troitskaya Y., Troitsky I., Vasilyev A., Vince O., Carnerero M., Raiteri C., Villata M., Acosta-Pulido J., Larionov V., Smith P., D'Ammando F., Agudo I., Arévalo M., Bachev R., Barnes J., Boeva S., Bozhilov V., Carosati D., Casadio C., Chen W., Damljanovic G., Eswaraiah E., Forné E., Gantchev G., Gómez J., González-Morales P., Griñón-Marín A., Grishina T., Holden M., Ibryamov S., Joner M., Jordan B., Jorstad S., Joshi M., Kopatskaya E., Koptelova E., Kurtanidze O., Kurtanidze S., Larionova E., Larionova L., Latev G., Lázaro C., Ligustri R., Lin H., Marscher A., Martínez-Lombilla C., McBreen B., Mihov B., Molina S., Moody J., Morozova D., Nikolashvili M., Nilsson K., Ovcharov E., Pace C., Panwar N., Pastor Yabar A., Pearson R., Pinna F., Protasio C., Rizzi N., Redondo-Lorenzo F., Rodríguez-Coira G., Ros J., Sadun A., Savchenko S., Semkov E., Slavcheva-Mihova L., Smith N., Strigachev A., Troitskaya Y., Troitsky I., Vasilyev A., and Vince O.
- Abstract
© 2017 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. We report on long-term multiwavelength monitoring of blazar Mrk 421 by the GLAST-AGILE Support Program of the Whole Earth Blazar Telescope (GASP-WEBT) collaboration and Steward Observatory, and by the Swift and Fermi satellites. We study the source behaviour in the period 2007-2015, characterized by several extreme flares. The ratio between the optical, X-ray and γ-ray fluxes is very variable. The γ-ray flux variations show a fair correlation with the optical ones starting from 2012. We analyse spectropolarimetric data and find wavelength-dependence of the polarization degree (P), which is compatible with the presence of the host galaxy, and no wavelength dependence of the electric vector polarization angle (EVPA). Optical polarimetry shows a lack of simple correlation between P and flux and wide rotations of the EVPA. We build broad-band spectral energy distributions with simultaneous near-infrared and optical data from the GASP-WEBT and ultraviolet and X-ray data from the Swift satellite. They show strong variability in both flux and X-ray spectr al shape and suggest a shift of the synchrotron peak up to a factor of ~50 in frequency. The interpretation of the flux and spectral variability is compatible with jet models including at least two emitting regions that can change their orientation with respect to the line of sight.
149. Dissecting the long-term emission behaviour of the BL Lac object Mrk 421
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Carnerero M., Raiteri C., Villata M., Acosta-Pulido J., Larionov V., Smith P., D'Ammando F., Agudo I., Arévalo M., Bachev R., Barnes J., Boeva S., Bozhilov V., Carosati D., Casadio C., Chen W., Damljanovic G., Eswaraiah E., Forné E., Gantchev G., Gómez J., González-Morales P., Griñón-Marín A., Grishina T., Holden M., Ibryamov S., Joner M., Jordan B., Jorstad S., Joshi M., Kopatskaya E., Koptelova E., Kurtanidze O., Kurtanidze S., Larionova E., Larionova L., Latev G., Lázaro C., Ligustri R., Lin H., Marscher A., Martínez-Lombilla C., McBreen B., Mihov B., Molina S., Moody J., Morozova D., Nikolashvili M., Nilsson K., Ovcharov E., Pace C., Panwar N., Pastor Yabar A., Pearson R., Pinna F., Protasio C., Rizzi N., Redondo-Lorenzo F., Rodríguez-Coira G., Ros J., Sadun A., Savchenko S., Semkov E., Slavcheva-Mihova L., Smith N., Strigachev A., Troitskaya Y., Troitsky I., Vasilyev A., Vince O., Carnerero M., Raiteri C., Villata M., Acosta-Pulido J., Larionov V., Smith P., D'Ammando F., Agudo I., Arévalo M., Bachev R., Barnes J., Boeva S., Bozhilov V., Carosati D., Casadio C., Chen W., Damljanovic G., Eswaraiah E., Forné E., Gantchev G., Gómez J., González-Morales P., Griñón-Marín A., Grishina T., Holden M., Ibryamov S., Joner M., Jordan B., Jorstad S., Joshi M., Kopatskaya E., Koptelova E., Kurtanidze O., Kurtanidze S., Larionova E., Larionova L., Latev G., Lázaro C., Ligustri R., Lin H., Marscher A., Martínez-Lombilla C., McBreen B., Mihov B., Molina S., Moody J., Morozova D., Nikolashvili M., Nilsson K., Ovcharov E., Pace C., Panwar N., Pastor Yabar A., Pearson R., Pinna F., Protasio C., Rizzi N., Redondo-Lorenzo F., Rodríguez-Coira G., Ros J., Sadun A., Savchenko S., Semkov E., Slavcheva-Mihova L., Smith N., Strigachev A., Troitskaya Y., Troitsky I., Vasilyev A., and Vince O.
- Abstract
© 2017 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. We report on long-term multiwavelength monitoring of blazar Mrk 421 by the GLAST-AGILE Support Program of the Whole Earth Blazar Telescope (GASP-WEBT) collaboration and Steward Observatory, and by the Swift and Fermi satellites. We study the source behaviour in the period 2007-2015, characterized by several extreme flares. The ratio between the optical, X-ray and γ-ray fluxes is very variable. The γ-ray flux variations show a fair correlation with the optical ones starting from 2012. We analyse spectropolarimetric data and find wavelength-dependence of the polarization degree (P), which is compatible with the presence of the host galaxy, and no wavelength dependence of the electric vector polarization angle (EVPA). Optical polarimetry shows a lack of simple correlation between P and flux and wide rotations of the EVPA. We build broad-band spectral energy distributions with simultaneous near-infrared and optical data from the GASP-WEBT and ultraviolet and X-ray data from the Swift satellite. They show strong variability in both flux and X-ray spectr al shape and suggest a shift of the synchrotron peak up to a factor of ~50 in frequency. The interpretation of the flux and spectral variability is compatible with jet models including at least two emitting regions that can change their orientation with respect to the line of sight.
150. Polarization angle swings in blazars: The case of 3C 279
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Kiehlmann S., Savolainen T., Jorstad S., Sokolovsky K., Schinzel F., Marscher A., Larionov V., Agudo I., Akitaya H., Benítez E., Berdyugin A., Blinov D., Bochkarev N., Borman G., Burenkov A., Casadio C., Doroshenko V., Efimova N., Fukazawa Y., Gómez J., Grishina T., Hagen-Thorn V., Heidt J., Hiriart D., Itoh R., Joshi M., Kawabata K., Kimeridze G., Kopatskaya E., Korobtsev I., Krajci T., Kurtanidze O., Kurtanidze S., Larionova E., Larionova L., Lindfors E., López J., McHardy I., Molina S., Moritani Y., Morozova D., Nazarov S., Nikolashvili M., Nilsson K., Pulatova N., Reinthal R., Sadun A., Sasada M., Savchenko S., Sergeev S., Sigua L., Smith P., Sorcia M., Spiridonova O., Takaki K., Takalo L., Taylor B., Troitsky I., Uemura M., Ugolkova L., Ui T., Yoshida M., Zensus J., Zhdanova V., Kiehlmann S., Savolainen T., Jorstad S., Sokolovsky K., Schinzel F., Marscher A., Larionov V., Agudo I., Akitaya H., Benítez E., Berdyugin A., Blinov D., Bochkarev N., Borman G., Burenkov A., Casadio C., Doroshenko V., Efimova N., Fukazawa Y., Gómez J., Grishina T., Hagen-Thorn V., Heidt J., Hiriart D., Itoh R., Joshi M., Kawabata K., Kimeridze G., Kopatskaya E., Korobtsev I., Krajci T., Kurtanidze O., Kurtanidze S., Larionova E., Larionova L., Lindfors E., López J., McHardy I., Molina S., Moritani Y., Morozova D., Nazarov S., Nikolashvili M., Nilsson K., Pulatova N., Reinthal R., Sadun A., Sasada M., Savchenko S., Sergeev S., Sigua L., Smith P., Sorcia M., Spiridonova O., Takaki K., Takalo L., Taylor B., Troitsky I., Uemura M., Ugolkova L., Ui T., Yoshida M., Zensus J., and Zhdanova V.
- Abstract
© ESO, 2016.Context. Over the past few years, on several occasions, large, continuous rotations of the electric vector position angle (EVPA) of linearly polarized optical emission from blazars have been reported. These events are often coincident with high energy γ-ray flares and they have attracted considerable attention, since they could allow us to probe the magnetic field structure in the γ-ray emitting region of the jet. The flat-spectrum radio quasar 3C 279 is one of the most prominent examples showing this behaviour. Aims. Our goal is to study the observed EVPA rotations and to distinguish between a stochastic and a deterministic origin of the polarization variability. Methods. We have combined multiple data sets of R-band photometry and optical polarimetry measurements of 3C 279, yielding exceptionally well-sampled flux density and polarization curves that cover a period of 2008-2012. Several large EVPA rotations are identified in the data. We introduce a quantitative measure for the EVPA curve smoothness, which is then used to test a set of simple random walk polarization variability models against the data. Results. 3C 279 shows different polarization variation characteristics during an optical low-flux state and a flaring state. The polarization variation during the flaring state, especially the smooth ∼360° rotation of the EVPA in mid-2011, is not consistent with the tested stochastic processes. Conclusions. We conclude that, during the two different optical flux states, two different processes govern polarization variation, which is possibly a stochastic process during the low-brightness state and a deterministic process during the flaring activity.
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