Author Info

A. A. Abdo, Naval Research Laboratory
M. Ackermann, Stanford University
M. Ajello, Stanford University
L. Baldini, Istituto Nazionale di Fisica Nucleare
J. Ballet, Universit´e Paris Diderot
G. Barbiellini, Istituto Nazionale di Fisica Nucleare
D. Bastieri, Istituto Nazionale di Fisica Nucleare
K. Bechtol, Stanford University
R. Bellazzini, Istituto Nazionale di Fisica Nucleare
B. Berenji, Stanford University
R. D. Blandford, Stanford University
E. Bonamente, Istituto Nazionale di Fisica Nucleare
A. W. Borgland, Stanford University
A. Bouvier, Stanford University
J. Bregeon, Istituto Nazionale di Fisica Nucleare
A. Brez, Istituto Nazionale di Fisica Nucleare
M. Brigida, Universit` a e del Politecnico di Bari
P. Bruel, Ecole Polytechnique
R. Buehler, Stanford University
S. Buson, Istituto Nazionale di Fisica Nucleare
G. A. Caliandro, Institut de Ciencies de l’Espai
R. A. Cameron, Stanford University
P. A. Caraveo, INAF-Istituto di Astrofisica Spaziale e Fisica Cosmica
S. Carrigan, Universit`a di Padova
J. M. Casandjian, Universit´e Paris Diderot
E. Cavazzuti, Agenzia Spaziale Italiana
C. Cecchi, Istituto Nazionale di Fisica Nucleare
Ö. Çelik, NASA Goddard Space Flight Center
E. Charles, Stanford University
A. Chekhtman, Naval Research Laboratory
C. C. Cheung, Naval Research Laboratory
J. Chiang, Stanford University
S. Ciprini, Universit`a degli Studi di Perugia
R. Claus, Stanford University
J. Cohen-Tanugi, Universit´e Montpellier 2
J. Conrad, Stockholm University
L. Costamente, Stanford University
S. Cutini, Agenzia Spaziale Italiana (ASI) Science Data Center
D. S. Davis, NASA Goddard Space Flight Center
C. D. Dermer, Naval Research Laboratory
F. de Palma, Universita e del Politecnico di Bari
S. W. Digel, Stanford University
E. Do Couto E Silva, Stanford University
P. S. Drell, Stanford University
R. Dubois, Stanford University
D. Dumora, Centre d’Etudes Nucleaires Bordeaux Gradignan
C. Favuzzi, Universita e del Politecnico di Bari
S. J. Fegan, Ecole Polytechnique
P. Fortin, Ecole Polytechnique
M. Frailis, Universita di Udine and Istituto Nazionale di Fisica Nucleare
L. Fuhrmann, Max-Planck-Institut fur Radioastronomie
Y. Fukazawa, Hiroshima University
S. Funk, Stanford University
P. Fusco, Universita e del Politecnico di Bari
F. Gargano, Istituto Nazionale di Fisica Nucleare
D. Gasparrini, Agenzia Spaziale Italiana (ASI) Science Data Center
N. Gehrels, NASA Goddard Space Flight Center
S. Germani, Istituto Nazionale di Fisica Nucleare
N. Giglietto, Universita e del Politecnico di Bari
P. Giommi, Agenzia Spaziale Italiana (ASI) Science Data Center
F. Giordano, Universita e del Politecnico di Bari
M. Giroletti, INAF Istituto di Radioastronomia
T. Glanzman, Stanford University
G. Godfrey, Stanford University
I. A. Grenier, Universite Paris Diderot
J. E. Grove, Naval Research Laboratory
L. Guillemot, Centre d’ Etudes Nucleaires Bordeaux Gradignan
S. Guiriec, University of Alabama in Huntsville
D. Hadasch, Institut de Ciencies de l’Espai
M. Hayashida, Stanford University
E. Hays, NASA Goddard Space Flight Center
D. Horan, Ecole Polytechnique
R. E. Hughes, Ohio State University - Columbus
R. Itoh, Hiroshima University
G. Jóhannesson, Stanford University
A. S. Johnson, Stanford University
T. J. Johnson, NASA Goddard Space Flight Center
W. N. Johnson, Naval Research Laboratory
T. Kamae, Stanford University
H. Katagiri, Hiroshima University
J. Kataoka, Waseda University
J. Knödlseder, Centre d’ Etude Spatiale des Rayonnements
M. Kuss, Istituto Nazionale di Fisica Nucleare
J. Lande, Stanford University
L. Latronico, Istituto Nazionale di Fisica Nucleare
S.-H. Lee, Stanford University
F. Longo, Istituto Nazionale di Fisica Nucleare
F. Loparco, Universita e del Politecnico di Bari
B. Lott, Centre d’ Etudes Nucleaires Bordeaux Gradignan
M. N. Lovellette, Naval Research Laboratory
P. Lubrano, Istituto Nazionale di Fisica Nucleare
A. Makeev, Naval Research Laboratory
M. N. Mazziotta, Istituto Nazionale di Fisica Nucleare
J. E. McEnery, NASA Goddard Space Flight Center
J. Mehault, Universite Montpellier 2
P. F. Michelson, Stanford University
T. Mizuno, Hiroshima University
A. A. Moiseev, Center for Research and Exploration in Space Science and Technology
C. Monte, Universita e del Politecnico di Bari
M. E. Monzani, Stanford University
A. Morselli, Istituto Nazionale di Fisica Nucleare
I. V. Mosalenko, Stanford University
S. Murgia, Stanford University
T. Nakamori, Waseda University
M. Naumann-Godo, Universite Paris Diderot
I. Nestoras, Max-Planck-Institut fur Radioastronomie
P. L. Nolan, Stanford University
J. P. Norris, University of Denver
E. Nuss, Universite Montpellier 2
T. Ohsugi, Hiroshima University
A. Okumura, Institute of Space and Astronautical Science
N. Omodei, Stanford University
E. Orlando, Max-Planck Institut fur extraterrestrische Physik
J. F. Ormes, University of Denver
M. Ozaki, Institute of Space and Astronautical Science
D. Paneque, Stanford University
J. H. Panetta, Stanford University
D. Parent, Naval Research Laboratory
V. Pelassa, Universite Montpellier 2
M. Pepe, Istituto Nazionale di Fisica Nucleare
M. Pesce-Rollins, Istituto Nazionale di Fisica Nucleare
F. Piron, Universite Montpellier 2
T. A. Porter, Stanford University
S. Rainò, Universita e del Politecnico di Bari
R. Rando, Istituto Nazionale di Fisica Nucleare
M. Razzano, Istituto Nazionale di Fisica Nucleare
A. Reimer, Institut fur Astro-und Teilchenphysik and Institut fur Theoretische Physik
O. Reimer, Institut fur Astro-und Teilchenphysik and Institut fur Theoretische Physik
L. C. Reyes, University of Chicago
J. Ripken, Stockholm University
S. Ritz, Santa Cruz Institute for Particle Physics
R. W. Romani, Stanford University
M. Roth, University of Washington - Seattle Campus
H. F.-W. Sadrozinski, Santa Cruz Institute for Particle Physics
D. Sanchez, Ecole Polytechnique
A. Sander, Ohio State University - Columbus
J. D. Scargle, NASA Ames Research Center
C. Sgrò, Istituto Nazionale di Fisica Nucleare
M. S. Shaw, Stanford University
P. D. Smith, Ohio State University - Columbus
G. Spandre, Istituto Nazionale di Fisica Nucleare
P. Spinelli, Universita e del Politecnico di Bari
M. S. Strickman, Naval Research Laboratory
D. J. Suson, Purdue University Calumet
H. Takahashi, Hiroshima University
T. Tanaka, Stanford University
J. B. Thayer, Stanford University
J. G. Thayer, Stanford University
D. J. Thompson, NASA Goddard Space Flight Center
L. Tibaldo, Universite Paris Diderot
D. F. Torres, Institut de Ciencies de l’Espai
G. Tosti, Istituto Nazionale di Fisica Nucleare
A. Tramacere, Stanford University
T. L. Usher, Stanford University
J. Vandenbroucke, Stanford University
V. Vasileiou, Center for Research and Exploration in Space Science and Technology
N. Vilchez, Centre d’ Etude Spatiale des Rayonnements
V. Vitale, Istituto Nazionale di Fisica Nucleare
A. P. Waite, Stanford University
P. Wang, Stanford University
B. L. Winer, Ohio State University - Columbus
K. S. Wood, Naval Research Laboratory
Z. Yang, Stockholm University
T. Ylinen, The Oskar Klein Centre for Cosmoparticle Physics
M. Ziegler, Santa Cruz Institute for Particle Physics
V. A. Acciari, Harvard-Smithsonian Center for Astrophysics
E. Aliu, Columbia University
T. Arlen, University of California - Los Angeles
T. Aune, University of California - Santa Cruz
M. Beilicke, Washington University
W. Benbow, Harvard-Smithsonian Center for Astrophysics
M. Bottcher, Ohio University
D. Boltuch, University of Delaware
S. M. Bradbury, University of Leeds
J. H. Buckley, Washington University
V. Bugaev, Washington University
K. Byrum, Argonne National Laboratory
A. Cannon, University College Dublin
A. Cesarini, National University of Ireland Galway
J. L. Christiansen, California Polytechnic State University - San Luis ObispoFollow
L. Ciupik, Adler Planetarium and Astronomy Museum
W. Cui, Purdue University
I. De la Calle Perez, European Space Astronomy Centre
R. Dickherber, Washington University
M. Errando, Barnard College
A. Falcone, Pennsylvania State University - Main Campus
J. P. Finley, Purdue University
G. Finnegan, University of Utah
L. Fortson, University of Minnesota - Minneapolis
A. Furniss, University of California - Santa Cruz
N. Galante, Harvard-Smithsonian Center for Astrophysics
D. Gall, Purdue University
G. H. Gillanders, National University of Ireland, Galway
S. Godambe, University of Utah
J. Grube, Adler Planetarium and Astronomy Museum
R. Guenette, McGill University
G. Gyuk, Adler Planetarium and Astronomy Museum
D. Hanna, McGill University
J. Holder, University of Delaware
C. M. Hui, University of Utah
T. B. Humensky, University of Chicago
A. Imran, Iowa State University
P. Kaaret, University of Iowa
N. Karlsson, University of Minnesota - Minneapolis
M. Kertzman, DePauw University
D. Kieda, University of Utah
A. Konopelko, Pittsburg State University
H. Krawczynski, Washington University
F. Krennrich, Iowa State University
M. J. Lang, National University of Ireland, Galway
S. LeBohec, University of Utah
G. Maier, Platanenallee
S. McArthur, Washington University
A. McCann, McGill University
M. McCutcheon, McGill University
P. Moriarty, Galway-Mayo Institute of Technology
R. Mukherjee, Columbia University
R. A. Ong, University of California - Los Angeles
A. N. Otte, University of California - Santa Cruz
D. Pandel, University of Iowa
J. S. Perkins, Harvard-Smithsonian Center for Astrophysics
A. Pichel, Instituto de Astronomia y Fisica del Espacio
M. Pohl, Platanenallee
J. Quinn, University College Dublin
K. Ragan, McGill University
P. T. Reynolds, University of Chicago
E. Roache, Harvard-Smithsonian Center for Astrophysics
H. J. Rose, University of Leeds
M. Schroedter, Iowa State University
G. H. Sembroski, Purdue University
G. D. Senturk, Columbia University
A. W. Smith, Argonne National Laboratory
D. Steele, Adler Planetarium and Astronomy Museum
S. P. Swordy, University of Chicago
G. Tešić, McGill University
M. Theiling, Harvard-Smithsonian Center for Astrophysics
S. Thibadeau, Washington University
A. Varlotta, Purdue University
V. V. Vassiliev, University of California - Los Angeles
S. Vincent, University of Utah
S. P. Wakely, University of Chicago
J. E. Ward, University College Dublin
T. C. Weekes, Harvard-Smithsonian Center for Astrophysics
A. Weinstein, University of California - Los Angeles
T. Weisgarber, University of Chicago
D. A. Williams, University of California - Santa Cruz
S. Wissel, University of Chicago
M. Wood, University of California - Los Angeles
M. Villata, Osservatorio Astronomico di Torino
C. M. Raiteri, Osservatorio Astronomico di Torino
M. A. Gurwell, Harvard-Smithsonian Center for Astrophysics
V. M. Larionov, St. Petersburg State University
O. M. Kurtanidze, Abastumani Observatory
M. F. Aller, University of Michigan
A. Lähteenmäki, Helsinki University of Technology TKK
W. P. Chen, National Central University
A. Berduygin, University of Turku
I. Agudo, Instituto de Astrofısica de Andalucıa
H. D. Aller, University of Michigan
A. A. Arkharov, Pulkovo Observatory
U. Bach, Max-Planck-Institut fur Radioastronomie
R. Bachev, Bulgarian Academy of Sciences
P. Beltrame, Circolo Astrofili Talmassons
E. Benitez, Universidad Nacional Autonoma de Mexico
C. S. Buemi, Osservatorio Astrofisico di Catania
J. Dashti, Ohio University
P. Calcidese, Osservatorio Astronomico della Regione Autonoma Valle d’Aosta
D. Capezzali, Armenzano Astronomical Observatory
D. Carosati, Armenzano Astronomical Observatory
D. Da Rio, Circolo Astrofili Talmassons
A. Di Paola, Osservatorio Astronomico di Roma
C. Diltz, Ohio University
M. Dolci, Osservatorio Astronomico di Collurania Teramo
D. Dultzin, Universidad Nacional Autonoma de Mexico
E. Forne, Agrupaci´o Astronomica de Sabadell
J. L. Gómez, Instituto de Astrofısica de Andalucıa
V. A. Hagen-Thorn, St. Petersburg State University
A. Halkola, University of Turku
J. Heidt, Landessternwarte Heidelberg
D. Hiriart, Universidad Nacional Autonoma de Mexico
T. Hovatta, Helsinki University of Technology TKK
H.-Y. Hsiao, National Central University
S. G. Jorstad, Boston University
G. N. Kimeridze, Abastumani Observatory
T. S. Konstantinova, St. Petersburg State University
E. N. Kopatskaya, St. Petersburg State University
E. Koptelova, National Central University
P. Leto, Osservatorio Astrofisico di Catania
R. Ligustri, Circolo Astrofili Talmassons
E. Lindfors, University of Turku
J. M. Lopez, Universidad Nacional Autonoma de Mexico
A. P. Marscher, Boston University
M. Mommert, Landessternwarte Heidelberg
R. Mujica, INAOE
M. G. Nikolashvili, Abastumani Observatory
K. Nilsson, University of Turku
N. Palma, Ohio University
M. Pasanen, University of Turku
M. Roca-Sogorb, Instituto de Astrofısica de Andalucıa
J. A. Ros, Agrupacio Astronomica de Sabadell
P. Roustazadeh, Ohio University
A. C. Sadun, University of Colorado Denver
J. Saino, University of Turku
L. A. Sigua, Abastumani Observatory
A. Sillanää, University of Turku
M. Sorcia, Universidad Nacional Autonoma de Mexico
L. O. Takalo, University of Turku
M. Tornikoski, Helsinki University of Technology TKK
C. Trigilio, Osservatorio Astrofisico di Catania
R. Turchetti, Circolo Astrofili Talmassons
G. Umana, Osservatorio Astrofisico di Catania
T. Belloni, INAF-Osservatorio Astronomico di Brera
C. H. Blake, Princeton University
J. S. Bloom, University of California - Berkeley
E. Angelakis, Max-Planck-Institut fur Radioastronomie
M. Fumagalli, University of California - Santa Cruz
M. Hauser, Universitat Heidelberg
J. X. Prochaska, University of California - Santa Cruz
D. Riquelme, Institut de Radio Astronomie Millimetrique
A. Sievers, Institut de Radio Astronomie Millimetrique
D. L. Starr, University of California - Berkeley
G. Tagliaferri, INAF-Osservatorio Astronomico di Brera
H. Ungerechts, Institut de Radio Astronomie Millim´etrique
S. Wagner, Universitat Heidelberg
J. A. Zensus, Max-Planck-Institut fur Radioastronomie

Abstract

The BL Lacertae object 3C 66A was detected in a flaring state by the Fermi Large Area Telescope (LAT) and VERITAS in 2008 October. In addition to these gamma-ray observations, F-GAMMA, GASP-WEBT, PAIRITEL, MDM, ATOM, Swift, and Chandra provided radio to X-ray coverage. The available light curves show variability and, in particular, correlated flares are observed in the optical and Fermi-LAT gamma-ray band. The resulting spectral energy distribution can be well fitted using standard leptonic models with and without an external radiation field for inverse Compton scattering. It is found, however, that only the model with an external radiation field can accommodate the intra-night variability observed at optical wavelengths.

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URL: http://digitalcommons.calpoly.edu/phy_fac/370