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The Spectral Energy Distribution of Fermi bright blazars [PDF]
, 2009 (Abridged) We have conducted a detailed investigation of the broad-band
spectral properties of the \gamma-ray selected blazars of the Fermi LAT Bright
AGN Sample (LBAS).A. A. Abdo, A. A. Arkharov, A. A. Moiseev, A. Berdyugin, A. Brez, A. Chekhtman, A. de Angelis, A. Falcone, A. Giuliani, A. K. Harding, A. Makeev, A. Morselli, A. P. Marscher, A. P. Waite, A. Reimer, A. S. Johnson, A. Sadun, A. Sander, A. Sellerholm, A. Tramacere, A. W. Borgland, A. Y. Rodriguez, Abdo, Abdo, Abdo, Abdo, Abdo, Acciari, Acciari, Aharonian, Ajello, Ajello, Albert, Albert, Albert, Angelakis, Atwood, B. Berenji, B. Giebels, B. L. Winer, B. Lott, B. M. Baughman, Baars, Bessel, Blandford, C. Cecchi, C. D. Dermer, C. Farnier, C. Favuzzi, C. Gronwall, C. Meurer, C. Monte, C. Pagani, C. Pittori, C. Raiteri, C. Sgrò, Colafrancesco, Costamante, D. A. Smith, D. Bastieri, D. Burrows, D. Carosati, D. Dultzin, D. Dumora, D. F. Torres, D. Gasparrini, D. Hadasch, D. Hiriart, D. Horan, D. J. Suson, D. J. Thompson, D. Paneque, D. Parent, D. Sanchez, Dermer, Donnarumma, E. A. Hoversten, E. Angelakis, E. Benitez, E. Bonamente, E. Cavazzuti, E. Charles, E. D. Bloom, E. do Couto e Silva, E. Forné, E. Hays, E. J. Siskind, E. Koptelova, E. Lindfors, E. N. Kopatskaya, E. Nuss, E. Orlando, Errando, F. D'ammando, F. de Palma, F. Gargano, F. Giordano, F. Longo, F. Loparco, F. Marshall, F. Piron, F. Rahoui, F. Ryde, F. Verrecchia, Fuhrmann, G. A. Caliandro, G. Barbiellini, G. Chincarini, G. Godfrey, G. Jóhannesson, G. Kimeridze, G. M. Madejski, G. Spandre, G. Stratta, G. Tosti, G. V. Zhekanis, Gehrels, Ghisellini, Giommi, Giommi, Giommi, H. D. Aller, H. F.-W. Sadrozinski, H. Katagiri, H. Tajima, H. Takahashi, Hartman, Healey, Healey, I. A. Grenier, I. Agudo, I. Donnarumma, I. Nestoras, I. V. Moskalenko, J. A. Ros, J. A. Zensus, J. B. Thayer, J. Ballet, J. Bregeon, J. Chiang, J. Cohen-Tanugi, J. Conrad, J. D. Scargle, J. E. Grove, J. E. McEnery, J. F. Ormes, J. G. Thayer, J. H. Panetta, J. Heidt, J. Kataoka, J. Kennea, J. Knödlseder, J. L. Gómez, J. L. Richards, J. Lande, J. M. Casandjian, J. Osborne, J. P. Norris, J.-L. Starck, K. Bechtol, K. Nilsson, K. Page, K. S. Wood, Korolkov, Kovalev, Kovalev, Kovalev, Kubo, L. A. Sigua, L. Baldini, L. Calzoletti, L. Costamante, L. Fuhrmann, L. Guillemot, L. Latronico, L. O. Takalo, L. Pacciani, L. R. Cominsky, L. S. Rochester, L. Tibaldo, Lagage, Lister, M. A. Gurwell, M. Ackermann, M. Ajello, M. Axelsson, M. Boettcher, M. Brigida, M. Capalbi, M. E. Monzani, M. F. Aller, M. Frailis, M. Hayashida, M. Kadler, M. Kerr, M. Kuss, M. L. Kocian, M. N. Lovellette, M. N. Mazziotta, M. Ozaki, M. Pasanen, M. Pepe, M. Perri, M. Pesce-Rollins, M. Razzano, M. Roth, M. S. Jackson, M. S. Shaw, M. S. Strickman, M. Stevenson, M. Villata, M. Ziegler, Marchã, Mazziotta, Monet, Moretti, N. A. Nizhelsky, N. Gehrels, N. Giglietto, N. Kawai, N. Omodei, N. Vilchez, O. M. Kurtanidze, O. Reimer, Ott, P. A. Caraveo, P. Bruel, P. D. Smith, P. F. Michelson, P. Fortin, P. Fusco, P. Giommi, P. L. Nolan, P. Leto, P. Lubrano, P. M. Saz Parkinson, P. Marchegiani, P. Padovani, P. Roustazadeh, P. S. Drell, P. Spinelli, P. Wang, Padovani, Padovani, Poole, R. A. Cameron, R. Bellazzini, R. Claus, R. D. Blandford, R. Deitrick, R. Dubois, R. E. Hughes, R. Itoh, R. Ojha, R. Rando, R. W. Romani, S. Buson, S. Chaty, S. Ciprini, S. Colafrancesco, S. Cutini, S. E. Healey, S. Funk, S. G. Jorstad, S. Germani, S. Guiriec, S. J. Fegan, S. Murgia, S. Piranomonte, S. Puccetti, S. Rainò, S. Ritz, S. W. Digel, Schlegel, Sikora, T. A. Porter, T. Glanzman, T. H. Burnett, T. Kamae, T. L. Usher, T. Mizuno, T. Ohsugi, T. Reposeur, T. S. Konstantinova, T. Takahashi, T. Tanaka, T. Ylinen, Teshima, Tramacere, U. Bach, V. D'Elia, V. M. Larionov, V. Pavlidou, V. Pelassa, V. Vasileiou, V. Vitale, Vercellone, W. B. Focke, W. Max-Moerbeck, W. McConville, W. Mitthumsiri, W. N. Johnson, W. P. Chen, Weekes, Y. Fukazawa, Y. Hanabata, Y. Uchiyama, Y. Y. Kovalev, Yu. A. Kovalev, Ö. Çelik +309 morecore +4 more sourcesNear infrared polarimetry of a sample of blazars*
EPJ Web of Conferences, 2013 Polarization variability is one of the most ubiquitous characteristic of blazars. Near infrared (NIR)polarization measurements of blazars are not common, contrary to the optical ones.Pulido J. A. Acosta, Pereyra A., Agudo I., Agulli I., Carnerero M., Segura N. Castro, Gómez J.L., Jorstad S., Marscher A. +8 moredoaj +1 more sourceBL Lac Contribution to the Extragalactic Gamma-Ray Background [PDF]
, 2007 Very high energy gamma-rays from blazars traversing cosmological distances
through the metagalactic radiation field can convert into electron-positron
pairs in photon-photon collisions. The converted gamma-rays initiate
electromagnetic cascades driven by Aharonian, Aharonian, Aharonian, Bade, Beckmann, Chiang, Coppi, Costamante, Costamante, Fossati, Ghisellini, Gioia, Giommi, Gorbunov, Hunter, K. Mannheim, Kneiske, Kneiske, Kronberg, Laurent-Mühleisen, Maciolek-Niedzwiecki, Mannheim, Mannheim, Protheroe, Protheroe, Rector, Reimer, Reimer, Reimer, Ryu, Sigl, Sreekumar, Stawarz, Stawarz, Stecker, T. M. Kneiske, Waxman, Wei +37 morecore +2 more sourcesDiscovery of Hidden Blazars [PDF]
Science, 2001 Every radio-loud quasar may have blazar activities, according to a unified scheme where the differences in both optical and radio observations of radio-loud quasars are the result of different viewing angles. We have predicted that blazars may be detected using emission line ratio variations caused by variable illumination of gas clouds in the broad ...Ma, Feng, Wills, Beverley J.openaire +3 more sourcesGeneral Physical Properties of Fermi Blazars
The Astrophysical Journal Supplement Series, 2023 We study the general physical properties of Fermi blazars using the Fermi fourth source catalog data (4FGL-DR2). The quasi-simultaneous multiwavelength data of Fermi blazars are fitted by using the one-zone leptonic model to obtain some physical ...Yongyun Chen, Qiusheng Gu, Junhui Fan, Xiaoling Yu, Xiaogu Zhong, Hongyu Liu, Nan Ding, Dingrong Xiong, Xiaotong Guo +8 moredoaj +1 more sourceBlazars in the early Universe [PDF]
, 2011 We investigate the relative occurrence of radio--loud and radio-quiet quasars
in the first billion years of the Universe, powered by black holes heavier than
one billion solar masses. We consider the sample of high-redshfit blazars
detected in the hard X-Abdo, Ajello, Baes, Becker, Bernardi, Bryan, Croton, F. Haardt, Ferrarese, G. Ghisellini, Ghisellini, Ghisellini, Ghisellini, Gültekin, Haiman, Hook, Hopkins, Häring, Jiang, Kormendy, Kormendy, Kurk, Lauer, Lauer, M. Volonteri, Marconi, Marconi, McGreer, Merloni, Pizzella, R. Della Ceca, Rhook, Richards, Richards, Romani, Schneider, Shakura, Shen, Sheth, Treister, Tremaine, Tundo, Volonteri, Volonteri, Willott, Worsley, Worsley, Wyithe, Yuan +48 morecore +1 more sourceExploring the connection between radio and GeV-TeV gamma-ray emission in
the 1FHL and 2FHL AGN samples [PDF]
, 2017 The Fermi Large Area Telescope (LAT) revealed that blazars, representing the
most extreme radio-loud active galactic nuclei (AGN) population, dominate the
census of the gamma-ray sky, and a significant correlation was found between
radio and gamma-ray ...Costamante, L., D'Ammando, F., Giroletti, M., Lico, R., Orienti, M., Pavlidou, V., Tavecchio, F. +6 morecore +2 more sources
