THE JUNE 2008 FLARE OF MARKARIAN 421 FROM OPTICAL TO TeV ENERGIES

Donnarumma, I.; Vittorini, V.; Vercellone, S.; Del Monte, E.; Feroci, M.; D'Ammando, F.; Pacciani, L.; Chen, A.; Tavani, M.; Bulgarelli, A.; Giuliani, A.; Longo, F.; Pucella, G.; Argan, A.; Barbiellini, G.; Boffelli, F.; Caraveo, P.; Cattaneo, P.; Cocco, V.; Costa, E.; De Paris, G.; Di Cocco, G.; Evangelista, Y.; Fiorini, M.; Froysland, T.; Frutti, M.; Fuschino, F.; Galli, M.; Gianotti, F.; Labanti, C.; Lapshov, I.; Lazzarotto, F.; Lipari, P.; Marisaldi, M.; Mastropietro, M.; Mereghetti, S.; Morelli, E.; Morselli, A.; Pellizzoni, A.; Perotti, F.; Picozza, P.; Porrovecchio, G.; Prest, M.; Rapisarda, M.; Rappoldi, A.; Rubini, A.; Soffitta, P.; Trifoglio, M.; Trois, A.; Vallazza, E.; Zambra, A.; Zanello, D.; Pittori, C.; Santolamazza, P.; Verrecchia, F.; Giommi, P.; Colafrancesco, S.; Salotti, L.; Villata, M.; Raiteri, C.; Chen, W.; Efimova, N.; Jordan, B.; Konstantinova, T.; Koptelova, E.; Kurtanidze, O.; Larionov, V.; Ros, J.; Sadun, A.; Anderhub, H.; Antonelli, L.; Antoranz, P.; Backes, M.; Baixeras, C.; Balestra, S.; Barrio, J.; Bartko, H.; Bastieri, D.; Becerra Gonzalez, J.; Becker, J.; Bednarek, W.; Berger, K.; Bernardini, E.; Biland, A.; Bock, R.; Bonnoli, G.; Bordas, P.; Tridon, D.; Bosch-Ramon, V.; Bretz, T.; Britvitch, I.; Camara, M.; Carmona, E.; Chilingarian, A.; Commichau, S.; Contreras, J.; Cortina, J.; Costado, M.; Covino, S.; Curtef, V.; Dazzi, F.; De Angelis, A.; De Cea Del Pozo, E.; Reyes, R.; De Lotto, B.; De Maria, M.; De Sabata, F.; Delgado Mendez, C.; Dominguez, A.; Dorner, D.; Doro, M.; Elsaesser, D.; Errando, M.; Ferenc, D.; Fernandez, E.; Firpo, R.; Fonseca, M.; Font, L.; Galante, N.; Garcia Lopez, R.; Garczarczyk, M.; Gaug, M.; Goebel, F.; Hadasch, D.; Hayashida, M.; Herrero, A.; Hoehne-Moench, D.; Hose, J.; Hsu, C.; Huber, S.; Jogler, T.; Kranich, D.; La Barbera, A.; Laille, A.; Leonardo, E.; Lindfors, E.; Lombardi, S.; Lopez, M.; Lorenz, E.; Majumdar, P.; Maneva, G.; Mankuzhiyil, N.; Mannheim, K.; Maraschi, L.; Mariotti, M.; Martinez, M.; Mazin, D.; Meucci, M.; Meyer, M.; Miranda, J.; Mirzoyan, R.; Moldon, J.; Moles, M.; Moralejo, A.; Nieto, D.; Nilsson, K.; Ninkovic, J.; Oya, I.; Paoletti, R.; Paredes, J.; Pasanen, M.; Pascoli, D.; Pauss, F.; Pegna, R.; Perez-Torres, M.; Persic, M.; Peruzzo, L.; Prada, F.; Prandini, E.; Puchades, N.; Raymers, A.; Rhode, W.; Ribo, M.; Rico, J.; Rissi, M.; Robert, A.; Ruegamer, S.; Saggion, A.; Saito, T.; Salvati, M.; Sanchez-Conde, M.; Sartori, P.; Satalecka, K.; Scalzotto, V.; Scapin, V.; Schweizer, T.; Shayduk, M.; Shinozaki, K.; Shore, S.; Sidro, N.; Sierpowska-Bartosik, A.; Sillanpaa, A.; Sitarek, J.; Sobczynska, D.; Spanier, F.; Stamerra, A.; Stark, L.; Takalo, L.; Tavecchio, F.; Temnikov, P.; Tescaro, D.; Teshima, M.; Tluczykont, M.; Torres, D.; Turini, N.; Vankov, H.; Venturini, A.; Vitale, V.; Wagner, R.; Wittek, W.; Zabalza, V.; Zandanel, F.; Zanin, R.; Zapatero, J.; Acciari, V.; Aliu, E.; Arlen, T.; Beilicke, M.; Benbow, W.; Bradbury, S.; Buckley, J.; Bugaev, V.; Butt, Y.; Byrum, K.; Cannon, A.; Cesarini, A.; Chow, Y.; Ciupik, L.; Cogan, P.; Colin, P.; Cui, W.; Daniel, M.; Dickherber, R.; Duke, C.; Ergin, TÜLÜN; Fegan, S.; Finley, J.; Finnegan, G.; Fortin, P.; Furniss, A.; Gall, D.; Gillanders, G.; Guenette, R.; Gyuk, G.; Grube, J.; Hanna, D.; Holder, J.; Horan, D.; Hui, C.; Humensky, T.; Imran, A.; Kaaret, P.; Karlsson, N.; Kertzman, M.; Kieda, D.; Kildea, J.; Konopelko, A.; Krawczynski, H.; Krennrich, F.; Lang, M.; LeBohec, S.; Maier, G.; McCann, A.; McCutcheon, M.; Milovanovic, A.; Moriarty, P.; Nagai, T.; Ong, R.; Otte, A.; Pandel, D.; Perkins, J.; Pichel, A.; Pohl, M.; Ragan, K.; Reyes, L.; Reynolds, P.; Roache, E.; Rose, H.; Schroedter, M.; Sembroski, G.; Smith, A.; Steele, D.; Swordy, S.; Theiling, M.; Toner, J.; Valcarcel, L.; Varlotta, A.; Wakely, S.; Ward, J.; Weekes, T.; Weinstein, A.; Williams, D.; Wissel, S.; Wood, M.; Zitzer, B.

doi:10.1088/0004-637x/691/1/l13

THE JUNE 2008 FLARE OF MARKARIAN 421 FROM OPTICAL TO TeV ENERGIES

Atıf İçin Kopyala

Donnarumma I., Vittorini V., Vercellone S., Del Monte E., Feroci M., D'Ammando F., ...Daha Fazla

ASTROPHYSICAL JOURNAL LETTERS, cilt.691, sa.1, 2009 (SCI-Expanded)

Yayın Türü: Makale / Tam Makale
Cilt numarası: 691 Sayı: 1
Basım Tarihi: 2009
Doi Numarası: 10.1088/0004-637x/691/1/l13
Dergi Adı: ASTROPHYSICAL JOURNAL LETTERS
Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
Anahtar Kelimeler: BL Lacertae objects: individual (Mrk 421), gamma rays: observations, galaxies: jets, radiation mechanisms: non-thermal, X-rays: galaxies, BL-LAC OBJECTS, X-RAY-SPECTRA, GAMMA-RAYS, XMM-NEWTON, 3C 454.3, WEBT, OUTBURST, DISTRIBUTIONS, ACCELERATION, EMISSION
Orta Doğu Teknik Üniversitesi Adresli: Hayır

Özet

We present optical, X-ray, high-energy ((sic) 30 GeV) and very high energy ((sic) 100 GeV; VHE) observations of the high-frequency peaked blazar Mrk 421 taken between 2008 May 24 and June 23. A high-energy gamma-ray signal was detected by AGILE with root TS = 4.5 between June 9 and 15, with F(E > 100 MeV) = 42(-12)(+14) x 10(-8) photons cm(-2) s(-1). This flaring state is brighter than the average flux observed by EGRET by a factor of similar to 3, but still consistent with the highest EGRET flux. In hard X-rays (20-60 keV) SuperAGILE resolved a five-day flare (June 9-15) peaking at similar to 55 mCrab. SuperAGILE, RXTE/ASM and Swift/BAT data show a correlated flaring structure between soft and hard X-rays. Hints of the same flaring behavior are also detected in the simultaneous optical data provided by the GASP-WEBT. A Swift/XRT observation near the flaring maximum revealed the highest 2-10 keV flux ever observed from this source, of 2.6 x 10(-9) erg cm(-2) s(-1) (i.e. > 100 mCrab). A peak synchrotron energy of similar to 3 keV was derived, higher than typical values of similar to 0.5-1 keV. VHE observations with MAGIC and VERITAS between June 6 and 8 showed the flux peaking in a bright state, well correlated with the X-rays. This extraordinary set of simultaneous data, covering a 12-decade spectral range, allowed for a deep analysis of the spectral energy distribution as well as of correlated light curves. The gamma-ray flare can be interpreted within the framework of the synchrotron self-Compton model in terms of a rapid acceleration of leptons in the jet.