مدل پیامدهای تحصیلی دانش‌آموزان دوره متوسطه با توجه به اثرات روابط معلم- شاگرد و معلم-والدین با نقش میانجی آگاهی فراشناختی... by مرضیه ارغوانی, قاسم آهی, محمد حسن غنی فر, فاطمه شهابی زاده, رضا دستجردی

“…تعداد 392 نفر به همراه یکی از والدین‌شان به عنوان مشارکت‌کنندگان، پرسشنامه‌های ارتباط معلم- شاگرد (Murray & Zvoch, 2010)، ارتباط معلم- والدین (Vickers & Minke, 1995)، آگاهی فراشناختی (Schraw & Dennison, 1994)، سرزندگی تحصیلی (Dehghanizadeh & Chari, 2013)، خرده‌مقیاس یادگیری ادراک‌شده (Alavi, 1994 و Marks, 2000)، خرده‌مقیاس طرح‌ریزی برای فارغ‌التحصیل شدن پرسشنامه ملی درگیری دانش‌آموزی (NSSE)، آمادگی برای ورود به دانشگاه خرده‌مقیاس دانش‌آموز (Sokol, 2000) و خرده‌مقیاس شادی و رفتار در کلاس پرسشنامه ارزیابی ملی پیشرفت‌تحصیلی (Blazar & Kraft, 2015) را تکمیل نمودند. تحلیل داده‌ها با روش‌های آمار توصیفی و روش مدل‌یابی معادلات ساختاری با استفاده از نرم‌افزارهایSPSS22  و LISREL8.8 نشان داد که مدل پیشنهادی با داده‌های پژوهش برازش مناسب دارد. …”
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The Power of (Near) Simultaneous Multi-Frequency Observations for mm-VLBI and Astrometry by María J. Rioja, Richard Dodson, José L. Gómez, Sol N. Molina, Taehyun Jung, Bong Won Sohn

“…These shocks could be responsible for the γ-ray emission in blazar jets.…”
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Untangling Cosmic Magnetic Fields: Faraday Tomography at Metre Wavelengths with LOFAR by Shane P. O’Sullivan, Marcus Brüggen, Cameron L. Van Eck, Martin J. Hardcastle, Marijke Haverkorn, Timothy W. Shimwell, Cyril Tasse, Valentina Vacca, Cathy Horellou, George Heald

“…Other detected source types include an FRI radio galaxy and at least eight blazars. Most sources display simple Faraday spectra, but we highlight one blazar that displays a complex Faraday spectrum, with two close peaks in the Faraday dispersion function.…”
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Constraining the PG 1553+113 Binary Hypothesis: Interpreting Hints of a New, 22 yr Period by S. Adhikari, P. Peñil, J. R. Westernacher-Schneider, A. Domínguez, M. Ajello, S. Buson, A. Rico, J. Zrake

“…PG 1553+113 is a well-known blazar exhibiting evidence of a ∼2.2 yr quasiperiodic oscillation (QPO) in the radio, optical, X-ray, and γ -ray bands. …”
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Hadronic Processes at Work in 5BZB J0630−2406 by Gaëtan Fichet de Clairfontaine, Sara Buson, Leonard Pfeiffer, Stefano Marchesi, Alessandra Azzollini, Vardan Baghmanyan, Andrea Tramacere, Eleonora Barbano, Lenz Oswald

“…In this study, we focus on one object, 5BZB J0630−2406, which is among the blazars recently proposed as associated with neutrino emission during the first 7 yr of IceCube observations. …”
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Revisiting a Core–Jet Laboratory at High Redshift: Analysis of the Radio Jet in the Quasar PKS 2215+020 at <i>z</i> = 3.572 by Sándor Frey, Judit Fogasy, Krisztina Perger, Kateryna Kulish, Petra Benke, Dávid Koller, Krisztina Éva Gabányi

“…These values qualify PKS 2215+020 as a blazar, with rather typical jet properties in a small sample of only about 20 objects at <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mi>z</mi><mo>></mo><mn>3.5</mn></mrow></semantics></math></inline-formula> that have similar measurements to date. …”
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CHANDRA AND HST IMAGING OF THE QUASARS PKS B0106+013 AND 3C 345: INVERSE COMPTON X-RAYS AND MAGNETIZED JETS by Kharb, Preeti, Lister, Matthew L., Hogan, Brandon S., Marshall, Herman

“…We present results from deep (~70 ks) Chandra/ACIS observations and Hubble Space Telescope (HST) Advanced Camera for Surveys F475W observations of two highly optically polarized quasars belonging to the MOJAVE blazar sample, viz., PKS B0106+013 and 1641+399 (3C 345). …”
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Search for steady point-like sources in the astrophysical muon neutrino flux with 8 years of IceCube data by IceCube Collaboration, Aartsen, MG, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Ahrens, M, Altmann, D, Andeen, K, Anderson, T, Ansseau, I, Anton, G, Argüelles, C, Auffenberg, J, Axani, S, Backes, P, Bagherpour, H, Bai, X, Barbano, A, Barron, JP, Barwick, SW, Baum, V, Bay, R, Beatty, JJ, Tjus, JB, Becker, K-H, Benzvi, S, Berley, D, Bernardini, E, Besson, DZ, Binder, G, Bindig, D, Blaufuss, E, Blot, S, Bohm, C, Börner, M, Bos, F, Böser, S, Botner, O, Bourbeau, E, Bourbeau, J, Bradascio, F, Braun, J, Bretz, H-P, Bron, S, Brostean-Kaiser, J, Burgman, A, Busse, RS, Carver, T, Chen, C, Cheung, E, Chirkin, D, Clark, K, Classen, L, Collin, GH, Conrad, JM, Coppin, P, Correa, P, Cowen, DF, Cross, R, Dave, P, Day, M, André, JPAMD, Clercq, CD, Delaunay, JJ, Dembinski, H, Deoskar, K, Ridder, SD, Desiati, P, Vries, KDD, Wasseige, GD, With, MD, Deyoung, T, Díaz-Vélez, JC, Dujmovic, H, Dunkman, M, Dvorak, E, Eberhardt, B, Ehrhardt, T, Eichmann, B, Eller, P, Evenson, PA, Fahey, S, Fazely, AR, Felde, J, Filimonov, K, Finley, C, Franckowiak, A, Friedman, E, Fritz, A, Gaisser, TK, Gallagher, J, Ganster, E, Garrappa, S, Gerhardt, L, Ghorbani, K, Giang, W, Glauch, T, Glüsenkamp, T, Goldschmidt, A, Gonzalez, JG, Grant, D, Griffith, Z, Haack, C, Hallgren, A, Halve, L, Halzen, F, Hanson, K, Hebecker, D, Heereman, D, Helbing, K, Hellauer, R, Hickford, S, Hignight, J, Hill, GC, Hoffman, KD, Hoffmann, R, Hoinka, T, Hokanson-Fasig, B, Hoshina, K, Huang, F, Huber, M, Hultqvist, K, Hünnefeld, M, Hussain, R, In, S, Iovine, N, Ishihara, A, Jacobi, E, Japaridze, GS, Jeong, M, Jero, K, Jones, BJP, Kalaczynski, P, Kang, W, Kappes, A, Kappesser, D, Karg, T, Karle, A, Katz, U, Kauer, M, Keivani, A, Kelley, JL, Kheirandish, A, Kim, J, Kintscher, T, Kiryluk, J, Kittler, T, Klein, SR, Koirala, R, Kolanoski, H, Köpke, L, Kopper, C, Kopper, S, Koskinen, DJ, Kowalski, M, Krings, K, Kroll, M, Krückl, G, Kunwar, S, Kurahashi, N, Kyriacou, A, Labare, M, Lanfranchi, JL, Larson, MJ, Lauber, F, Leonard, K, Leuermann, M, Liu, QR, Lohfink, E, Mariscal, CJL, Lu, L, Lünemann, J, Luszczak, W, Madsen, J, Maggi, G, Mahn, KBM, Makino, Y, Mancina, S, Mariş, IC, Maruyama, R, Mase, K, Maunu, R, Meagher, K, Medici, M, Meier, M, Menne, T, Merino, G, Meures, T, Miarecki, S, Micallef, J, Momenté, G, Montaruli, T, Moore, RW, Moulai, M, Nagai, R, Nahnhauer, R, Nakarmi, P, Naumann, U, Neer, G, Niederhausen, H, Nowicki, SC, Nygren, DR, Pollmann, AO, Olivas, A, O'Murchadha, A, O'Sullivan, E, Palczewski, T, Pandya, H, Pankova, DV, Peiffer, P, Heros, CPDL, Pieloth, D, Pinat, E, Pizzuto, A, Plum, M, Price, PB, Przybylski, GT, Raab, C, Raissi, A, Rameez, M, Rauch, L, Rawlins, K, Rea, IC, Reimann, R, Relethford, B, Renzi, G, Resconi, E, Rhode, W, Richman, M, Robertson, S, Rongen, M, Rott, C, Ruhe, T, Ryckbosch, D, Rysewyk, D, Safa, I, Herrera, SES, Sandrock, A, Sandroos, J, Santander, M, Sarkar, S, Satalecka, K, Schaufel, M, Schlunder, P, Schmidt, T, Schneider, A, Schneider, J, Schöneberg, S, Schumacher, L, Sclafani, S, Seckel, D, Seunarine, S, Soedingrekso, J, Soldin, D, Song, M, Spiczak, GM, Spiering, C, Stachurska, J, Stamatikos, M, Stanev, T, Stasik, A, Stein, R, Stettner, J, Steuer, A, Stezelberger, T, Stokstad, RG, Stößl, A, Strotjohann, NL, Stuttard, T, Sullivan, GW, Sutherland, M, Taboada, I, Tenholt, F, Ter-Antonyan, S, Terliuk, A, Tilav, S, Tobin, MN, Tönnis, C, Toscano, S, Tosi, D, Tselengidou, M, Tung, CF, Turcati, A, Turcotte, R, Turley, CF, Ty, B, Unger, E, Elorrieta, MAU, Usner, M, Vandenbroucke, J, Driessche, WV, Eijk, DV, Eijndhoven, NV, Vanheule, S, Santen, JV, Vraeghe, M, Walck, C, Wallace, A, Wallraff, M, Wandler, FD, Wandkowsky, N, Watson, TB, Weaver, C, Weiss, MJ, Wendt, C, Werthebach, J, Westerhoff, S, Whelan, BJ, Whitehorn, N, Wiebe, K, Wiebusch, CH, Wille, L, Williams, DR, Wills, L, Wolf, M, Wood, J, Wood, TR, Woolsey, E, Woschnagg, K, Wrede, G, Xu, DL, Xu, XW, Xu, Y, Yanez, JP, Yodh, G, Yoshida, S, Yuan, T

“…The IceCube Collaboration has observed a highenergy astrophysical neutrino flux and recently found evidence for neutrino emission from the blazar TXS 0506+056. These results open a new window into the high-energy universe. …”

Discovery of Hydrogen Radio Recombination Lines at z = 0.89 toward PKS 1830-211 by Kimberly L. Emig, Neeraj Gupta, Pedro Salas, Sébastien Muller, Sergei A. Balashev, Françoise Combes, Emmanuel Momjian, Yiqing Song, Preshanth Jagannathan, Partha P. Deka, Gyula I. G. Józsa, Hans-Rainer Klöckner, Abhisek Mohapatra, Pasquier Noterdaeme, Patrick Petitjean, Raghunathan Srianand, Jonah D. Wagenveld

“…The RRL emission originates in a galaxy that intercepts and strongly lenses the radio blazar PKS 1830−211 ( z = 2.5). This is the second detection of RRLs outside of the local Universe and the first clearly associated with hydrogen. …”
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Polarization and Spectral Energy Distribution in OJ 287 during the 2016/17 Outbursts by Mauri Valtonen, Stanislaw Zola, Helen Jermak, Stefano Ciprini, Rene Hudec, Lankeswar Dey, Achamveedu Gopakumar, Daniel L. Reichart, Daniel B. Caton, Kosmas Gazeas, Katsura Matsumoto, Waldemar Ogloza, Marek Drozdz, Fahri Alicavus, Oleksandr Baransky, Andrei Berdyugin, Panos Boumis, Yurii Bufan, Bartlomiej Debski, Huseyin Er, Ahmet Erdem, Vira Godunova, Shirin Haque, Vivian L. Hoette, Jan Janik, Mark Kidger, Tomasz Kundera, Sebastian Kurowski, Alexis Liakos, Isa Mohammed, Kari Nilsson, Urszula Pajdosz, Vilppu Piirola, Tapio Pursimo, Brandon Rajkumar, Andrii O. Simon, Michal Siwak, Eda Sonbas, Ian A. Steele, Volodymir V. Vasylenko, Michal Zejmo, Pawel Zielinski

“…We report optical photometric and polarimetric observations of the blazar OJ 287 gathered during 2016/17. The high level of activity, noticed after the General Relativity Centenary flare, is argued to be part of the follow-up flares that exhibited high levels of polarization and originated in the primary black hole jet. …”
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RadioAstron Space VLBI Imaging of the Jet in M87. I. Detection of High Brightness Temperature at 22 GHz by Jae-Young Kim, Tuomas Savolainen, Petr Voitsik, Evgeniya V. Kravchenko, Mikhail M. Lisakov, Yuri Y. Kovalev, Hendrik Müller, Andrei P. Lobanov, Kirill V. Sokolovsky, Gabriele Bruni, Philip G. Edwards, Cormac Reynolds, Uwe Bach, Leonid I. Gurvits, Thomas P. Krichbaum, Kazuhiro Hada, Marcello Giroletti, Monica Orienti, James M. Anderson, Sang-Sung Lee, Bong Won Sohn, J. Anton Zensus

“…Therefore, this can be evidence for more extreme Doppler boosting due to a blazar-like small jet viewing angle or highly efficient particle acceleration processes occurring already at the base of the outflow.…”
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Search for steady point-like sources in the astrophysical muon neutrino flux with 8 years of IceCube data by Aartsen, M. G, Ackermann, M., Adams, J., Aguilar, J. A, Ahlers, M., Ahrens, M., Altmann, D., Andeen, K., Anderson, T., Ansseau, I., Anton, G., Argüelles, C., Auffenberg, J., Axani, S., Backes, P., Bagherpour, H., Bai, X., Barbano, A., Barron, J. P, Barwick, S. W, Baum, V., Bay, R., Beatty, J. J, Becker Tjus, J., Becker, K.-H., BenZvi, S., Berley, D., Bernardini, E., Besson, D. Z, Binder, G., Bindig, D., Blaufuss, E., Blot, S., Bohm, C., Börner, M., Bos, F., Böser, S., Botner, O., Bourbeau, E., Bourbeau, J., Bradascio, F., Braun, J., Bretz, H.-P., Bron, S., Brostean-Kaiser, J., Burgman, A., Busse, R. S, Carver, T., Chen, C., Cheung, E., Chirkin, D., Clark, K., Classen, L., Collin, G. H, Conrad, J. M, Coppin, P., Correa, P., Cowen, D. F, Cross, R., Dave, P., Day, M., de André, J. P A M, De Clercq, C., DeLaunay, J. J, Dembinski, H., Deoskar, K., De Ridder, S., Desiati, P., de Vries, K. D, de Wasseige, G., de With, M., DeYoung, T., Díaz-Vélez, J. C, Dujmovic, H., Dunkman, M., Dvorak, E., Eberhardt, B., Ehrhardt, T., Eichmann, B., Eller, P., Evenson, P. A, Fahey, S., Fazely, A. R, Felde, J., Filimonov, K., Finley, C., Franckowiak, A., Friedman, E., Fritz, A., Gaisser, T. K, Gallagher, J., Ganster, E., Garrappa, S., Gerhardt, L., Ghorbani, K., Giang, W., Glauch, T., Glüsenkamp, T., Goldschmidt, A., Gonzalez, J. G, Grant, D., Griffith, Z., Haack, C., Hallgren, A., Halve, L., Halzen, F., Hanson, K., Hebecker, D., Heereman, D., Helbing, K., Hellauer, R., Hickford, S., Hignight, J., Hill, G. C, Hoffman, K. D, Hoffmann, R., Hoinka, T., Hokanson-Fasig, B., Hoshina, K., Huang, F., Huber, M., Hultqvist, K., Hünnefeld, M., Hussain, R., In, S., Iovine, N., Ishihara, A., Jacobi, E., Japaridze, G. S, Jeong, M., Jero, K., Jones, B. J P, Kalaczynski, P., Kang, W., Kappes, A., Kappesser, D., Karg, T., Karle, A., Katz, U., Kauer, M., Keivani, A., Kelley, J. L, Kheirandish, A., Kim, J., Kintscher, T., Kiryluk, J., Kittler, T., Klein, S. R, Koirala, R., Kolanoski, H., Köpke, L., Kopper, C., Kopper, S., Koskinen, D. J, Kowalski, M., Krings, K., Kroll, M., Krückl, G., Kunwar, S., Kurahashi, N., Kyriacou, A., Labare, M., Lanfranchi, J. L, Larson, M. J, Lauber, F., Leonard, K., Leuermann, M., Liu, Q. R, Lohfink, E., Mariscal, C. J L, Lu, L., Lünemann, J., Luszczak, W., Madsen, J., Maggi, G., Mahn, K. B M, Makino, Y., Mancina, S., Mariş, I. C, Maruyama, R., Mase, K., Maunu, R., Meagher, K., Medici, M., Meier, M., Menne, T., Merino, G., Meures, T., Miarecki, S., Micallef, J., Momenté, G., Montaruli, T., Moore, R. W, Moulai, M., Nagai, R., Nahnhauer, R., Nakarmi, P., Naumann, U., Neer, G., Niederhausen, H., Nowicki, S. C, Nygren, D. R, Obertacke Pollmann, A., Olivas, A., O’Murchadha, A., O’Sullivan, E., Palczewski, T., Pandya, H., Pankova, D. V, Peiffer, P., Pérez de los Heros, C., Pieloth, D., Pinat, E., Pizzuto, A., Plum, M., Price, P. B, Przybylski, G. T, Raab, C., Rameez, M., Rauch, L., Rawlins, K., Rea, I. C, Reimann, R., Relethford, B., Renzi, G., Resconi, E., Rhode, W., Richman, M., Robertson, S., Rongen, M., Rott, C., Ruhe, T., Ryckbosch, D., Rysewyk, D., Safa, I., Sanchez Herrera, S. E, Sandrock, A., Sandroos, J., Santander, M., Sarkar, S., Sarkar, S., Satalecka, K., Schaufel, M., Schlunder, P., Schmidt, T., Schneider, A., Schneider, J., Schöneberg, S., Schumacher, L., Sclafani, S., Seckel, D., Seunarine, S., Soedingrekso, J., Soldin, D., Song, M., Spiczak, G. M, Spiering, C., Stachurska, J., Stamatikos, M., Stanev, T., Stasik, A., Stein, R., Stettner, J., Steuer, A., Stezelberger, T., Stokstad, R. G, Stößl, A., Strotjohann, N. L, Stuttard, T., Sullivan, G. W, Sutherland, M., Taboada, I., Tenholt, F., Ter-Antonyan, S., Terliuk, A., Tilav, S., Tobin, M. N, Tönnis, C., Toscano, S., Tosi, D., Tselengidou, M., Tung, C. F, Turcati, A., Turcotte, R., Turley, C. F, Ty, B., Unger, E., Unland Elorrieta, M. A, Usner, M., Vandenbroucke, J., Van Driessche, W., van Eijk, D., van Eijndhoven, N., Vanheule, S., van Santen, J., Vraeghe, M., Walck, C., Wallace, A., Wallraff, M., Wandler, F. D, Wandkowsky, N., Watson, T. B, Weaver, C., Weiss, M. J, Wendt, C., Werthebach, J., Westerhoff, S., Whelan, B. J, Whitehorn, N., Wiebe, K., Wiebusch, C. H, Wille, L., Williams, D. R, Wills, L., Wolf, M., Wood, J., Wood, T. R, Woolsey, E., Woschnagg, K., Wrede, G., Xu, D. L, Xu, X. W, Xu, Y., Yanez, J. P, Yodh, G., Yoshida, S., Yuan, T.

“…Abstract The IceCube Collaboration has observed a high-energy astrophysical neutrino flux and recently found evidence for neutrino emission from the blazar TXS 0506 $$+$$ + 056. …”
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Classification of unassociated fermi-LAT sources by Meng Qiyu

“…Among them, 271 have been associated to pulsars, 3436 to blazars, and 1782 remain unassociated sources. Unassociated sources are object for which there is not a clear counterpart in other wavelengths. …”
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X-Ray Polarization of BL Lacertae in Outburst by Abel L. Peirson, Michela Negro, Ioannis Liodakis, Riccardo Middei, Dawoon E. Kim, Alan P. Marscher, Herman L. Marshall, Luigi Pacciani, Roger W. Romani, Kinwah Wu, Alessandro Di Marco, Niccoló Di Lalla, Nicola Omodei, Svetlana G. Jorstad, Iván Agudo, Pouya M. Kouch, Elina Lindfors, Francisco José Aceituno, Maria I. Bernardos, Giacomo Bonnoli, Víctor Casanova, Maya García-Comas, Beatriz Agís-González, César Husillos, Alessandro Marchini, Alfredo Sota, Carolina Casadio, Juan Escudero, Ioannis Myserlis, Albrecht Sievers, Mark Gurwell, Ramprasad Rao, Ryo Imazawa, Mahito Sasada, Yasushi Fukazawa, Koji S. Kawabata, Makoto Uemura, Tsunefumi Mizuno, Tatsuya Nakaoka, Hiroshi Akitaya, Yeon Cheong, Hyeon-Woo Jeong, Sincheol Kang, Sang-Hyun Kim, Sang-Sung Lee, Emmanouil Angelakis, Alexander Kraus, Nicoló Cibrario, Immacolata Donnarumma, Juri Poutanen, Fabrizio Tavecchio, Lucio A. Antonelli, Matteo Bachetti, Luca Baldini, Wayne H. Baumgartner, Ronaldo Bellazzini, Stefano Bianchi, Stephen D. Bongiorno, Raffaella Bonino, Alessandro Brez, Niccoló Bucciantini, Fiamma Capitanio, Simone Castellano, Elisabetta Cavazzuti, Chien-Ting Chen, Stefano Ciprini, Enrico Costa, Alessandra De Rosa, Ettore Del Monte, Laura Di Gesu, Victor Doroshenko, Michal Dovčiak, Steven R. Ehlert, Teruaki Enoto, Yuri Evangelista, Sergio Fabiani, Riccardo Ferrazzoli, Javier A. Garcia, Shuichi Gunji, Kiyoshi Hayashida, Jeremy Heyl, Wataru Iwakiri, Philip Kaaret, Vladimir Karas, Takao Kitaguchi, Jeffery J. Kolodziejczak, Henric Krawczynski, Fabio La Monaca, Luca Latronico, Grzegorz Madejski, Simone Maldera, Alberto Manfreda, Frédéric Marin, Andrea Marinucci, Francesco Massaro, Giorgio Matt, Ikuyuki Mitsuishi, Fabio Muleri, C.-Y. Ng, Stephen L. O’Dell, Chiara Oppedisano, Alessandro Papitto, George G. Pavlov, Matteo Perri, Melissa Pesce-Rollins, Pierre-Olivier Petrucci, Maura Pilia, Andrea Possenti, Simonetta Puccetti, Brian D. Ramsey, John Rankin, Ajay Ratheesh, Oliver J. Roberts, Carmelo Sgró, Patrick Slane, Paolo Soffitta, Gloria Spandre, Douglas A. Swartz, Toru Tamagawa, Roberto Taverna, Yuzuru Tawara, Allyn F. Tennant, Nicholas E. Thomas, Francesco Tombesi, Alessio Trois, Sergey Tsygankov, Roberto Turolla, Jacco Vink, Martin C. Weisskopf, Fei Xie, Silvia Zane

“…Our contemporaneous X-ray data suggest that the IXPE energy band is at the crossover between the low- and high-frequency blazar emission humps. The source displays significant variability during the observation, and we measure polarization in three separate time bins. …”
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ВЕЙВЛЕТ–АНАЛИЗ АКТИВНОСТИ СИСТЕМЫ "ЯДРО-ДЖЕТ" КВАЗАРОВ И БЛАЗАРОВ В САНТИМЕТРОВОМ ДИАПАЗОНЕ by М. И. Рябов, А. Л. Сухарев, А. Е. Вольвач, Л. Н. Вольвач, Р. А. Сыч, М. Аллер

“…Long monitoring of fluxes of a radio emission blazars on centimetric and millimetric waves to be carring out since 1965 on РТ-26 the Radioastronomical observatory of Michigan university (UMRAO) in the USA (4.8, 8 and 14.5 Ggts) and since 1980 on РТ-22 scientific research institute «Crimean astrophysical observatory» (22 and 36.8 Ggts). …”
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Photons to axion-like particles conversion in Active Galactic Nuclei by Fabrizio Tavecchio, Marco Roncadelli, Giorgio Galanti

“…We first remark that AGN which can be detected above 100 GeV are blazars, namely AGN with jets, with one of them pointing towards us. …”
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X-RAY EMISSION OF ICRF SOURCES by V. V. Voitsekhovskiy, A. Tugay, V. V. Tkachuk, S. Yu. Shevchenko

“…Extragalactic frames of the ICRF system are mostly quasars , radio galaxies , blazars and Seyfert galaxies i.e. different types of the active galaxy nuclei (AGN) . …”
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The Radio/Gamma-Ray Connection from 120 MHz to 230 GHz by Marcello Giroletti, Filippo D’Ammando, Monica Orienti, Rocco Lico, The <i>Fermi</i>-LAT Collaboration

“…Radio loud active galactic nuclei are composed of different spatial features, each one characterized by different spectral properties in the radio band. Among them, blazars are the most common class of sources detected at gamma-rays by Fermi, and their radio emission is dominated by the flat spectrum compact core. …”
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Czech Participation in INTEGRAL: 1996–2011 by R. Hudec, M. Blažek, V. Hudcová

“…The results of the first 8 years of investigations of various scientific targets are briefly presented and discussed here, with emphasis on cataclysmic variables and blazars with the ESA INTEGRAL satellite with Czech participation.…”
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Czech Participation in the INTEGRAL Satellite: A Review by R. Hudec, M. Blažek, V. Hudcová

“…The results of the first 7 years of investigations of various scientific targets e.g. cataclysmic variables, blazars, X-ray sources, and GRBs with the ESA INTEGRAL satellite with Czech participation are briefly presented and discussed.…”
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