MULTI-WAVELENGTH OBSERVATIONS OF THE FLARING GAMMA-RAY BLAZAR 3C 66A IN 2008 OCTOBER

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題名:	MULTI-WAVELENGTH OBSERVATIONS OF THE FLARING GAMMA-RAY BLAZAR 3C 66A IN 2008 OCTOBER
作者:	Abdo,AA;Ackermann,M;Ajello,M;Baldini,L;Ballet,J;Barbiellini,G;Bastieri,D;Bechtol,K;Bellazzini,R;Berenji,B;Blandford,RD;Bonamente,E;Borgland,AW;Bouvier,A;Bregeon,J;Brez,A;Brigida,M;Bruel,P;Buehler,R;Buson,S;Caliandro,GA;Cameron,RA;Caraveo,PA;Carrigan,S;Casandjian,JM;Cavazzuti,E;Cecchi,C;Celik,O;Charles,E;Chekhtman,A;Cheung,CC;Chiang,J;Ciprini,S;Claus,R;Cohen-Tanugi,J;Conrad,J;Costamante,L;Cutini,S;Davis,DS;Dermer,CD;de Palma,F;Digel,SW;Silva,EDE;Drell,PS;Dubois,R;Dumora,D;Favuzzi,C;Fegan,SJ;Fortin,P;Frailis,M;Fuhrmann,L;Fukazawa,Y;Funk,S;Fusco,P;Giroletti,M;Glanzman,T;Godfrey,G;Grenier,IA;Grove,JE;Guillemot,L;Guiriec,S;Hadasch,D;Hayashida,M;Hays,E;Horan,D;Hughes,RE;Itoh,R;Johannesson,G;Johnson,AS;Johnson,TJ;Johnson,WN;Kamae,T;Katagiri,H;Kataoka,J;Knodlseder,J;Kuss,M;Lande,J;Latronico,L;Lee,SH;Longo,F;Loparco,F;Lott,B;Lovellette,MN;Lubrano,P;Makeev,A;Mazziotta,MN;McEnery,JE;Mehault,J;Michelson,PF;Mizuno,T;Moiseev,AA;Monte,C;Monzani,ME;Morselli,A;Moskalenko,IV;Murgia,S;Nakamori,T;Naumann-Godo,M;Nestoras,I;Nolan,PL;Norris,JP;Nuss,E;Ohsugi,T;Okumura,A;Omodei,N;Orlando,E;Ormes,JF;Ozaki,M;Paneque,D;Panetta,JH;Parent,D;Pelassa,V;Pepe,M;Pesce-Rollins,M;Piron,F;Porter,TA;Raino,S;Rando,R;Razzano,M;Reimer,A;Reimer,O;Reyes,LC;Ripken,J;Ritz,S;Romani,RW;Roth,M;Sadrozinski,HFW;Sanchez,D;Sander,A;Scargle,JD;Sgro,C;Shaw,MS;Smith,PD;Spandre,G;Spinelli,P;Strickman,MS;Suson,DJ;Takahashi,H;Tanaka,T;Thayer,JB;Thayer,JG;Thompson,DJ;Tibaldo,L;Torres,DF;Tosti,G;Tramacere,A;Usher,TL;Vandenbroucke,J;Vasileiou,V;Vilchez,N;Vitale,V;Waite,AP;Wang,P;Winer,BL;Wood,KS;Yang,Z;Ylinen,T;Ziegler,M;Acciari,VA;Aliu,E;Arlen,T;Aune,T;Beilicke,M;Benbow,W;Bottcher,M;Boltuch,D;Bradbury,SM;Buckley,JH;Bugaev,V;Byrum,K;Cannon,A;Cesarini,A;Christiansen,JL;Ciupik,L;Cui,W;Perez,ID;Dickherber,R;Errando,M;Falcone,A;Finley,JP;Finnegan,G;Fortson,L;Furniss,A;Galante,N;Gall,D;Gillanders,GH;Godambe,S;Grube,J;Guenette,R;Gyuk,G;Hanna,D;Holder,J;Hui,CM;Humensky,TB;Imran,A;Kaaret,P;Karlsson,N;Kertzman,M;Kieda,D;Konopelko,A;Krawczynski,H;Krennrich,F;Lang,MJ;LeBohec,S;Maier,G;McArthur,S;McCann,A;McCutcheon,M;Moriarty,P;Mukherjee,R;Ong,RA;Otte,AN;Pandel,D;Perkins,JS;Pichel,A;Pohl,M;Quinn,J;Ragan,K;Reynolds,PT;Roache,E;Rose,HJ;Schroedter,M;Sembroski,GH;Senturk,GD;Smith,AW;Steele,D;Swordy,SP;Tesic,G;Theiling,M;Thibadeau,S;Varlotta,A;Vassiliev,VV;Vincent,S;Wakely,SP;Ward,JE;Weekes,TC;Weinstein,A;Weisgarber,T;Williams,DA;Wissel,S;Wood,M;Villata,M;Raiteri,CM;Gurwell,MA;Larionov,VM;Kurtanidze,OM;Aller,MF;Lahteenmaki,A;Chen,WP;Berduygin,A;Agudo,I;Aller,HD;Arkharov,AA;Bach,U;Bachev,R;Beltrame,P;Benitez,E;Buemi,CS;Dashti,J;Calcidese,P;Capezzali,D;Carosati,D;Da Rio,D;Di Paola,A;Diltz,C;Dolci,M;Dultzin,D;Forne,E;Gomez,JL;Hagen-Thorn,VA;Halkola,A;Heidt,J;Hiriart,D;Hovatta,T;Hsiao,HY;Jorstad,SG;Kimeridze,GN;Konstantinova,TS;Kopatskaya,EN;Koptelova,E;Leto,P;Ligustri,R;Lindfors,E;Lopez,JM;Marscher,AP;Mommert,M;Mujica,R;Nikolashvili,MG;Nilsson,K;Palma,N;Pasanen,M;Roca-Sogorb,M;Mommert,M;Mujica,R;Nikolashvili,MG;Nilsson,K;Palma,N;Pasanen,M;Roca-Sogorb,M;Ros,JA;Roustazadeh,P;Sadun,AC;Saino,J;Sigua,LA;Sillanaa,A;Sorcia,M;Takalo,LO;Tornikoski,M;Trigilio,C;Turchetti,R;Umana,G;Belloni,T;Blake,CH;Bloom,JS;Angelakis,E;Fumagalli,M;Hauser,M;Prochaska,JX;Riquelme,D;Sievers,A;Starr,DL;Tagliaferri,G;Ungerechts,H;Wagner,S;Zensus,JA
貢獻者:	天文研究所
關鍵詞:	BL LACERTAE OBJECTS;ACTIVE GALACTIC NUCLEI;LARGE-AREA TELESCOPE;SPECTRAL ENERGY-DISTRIBUTION;EPOCH VLBI SURVEY;BRIGHT BLAZARS;TEV BLAZARS;BACKGROUND-RADIATION;VERITAS OBSERVATIONS;RADIO-SOURCES
日期:	2011
上傳時間:	2012-03-27 18:12:19 (UTC+8)
出版者:	國立中央大學
摘要:	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.
關聯:	ASTROPHYSICAL JOURNAL
顯示於類別:	[天文研究所] 期刊論文

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