Authors
Max L Ahnen, Stefano Ansoldi, Lucio Angelo Antonelli, Cornelia Arcaro, Ana Babić, B Banerjee, Priyadarshini Bangale, U Barresde Almeida, Juan A Barrio, J Becerragonzález, Włodzimierz Bednarek, Elisa Bernardini, Alessio Berti, Wrijupan Bhattacharyya, Oscar Blanch, Giacomo Bonnoli, Roberto Carosi, Alessandro Carosi, Arghya Chatterjee, SM Colak, P Colin, E Colombo, JL Contreras, J Cortina, Stefano Covino, P Cumani, P Da Vela, F Dazzi, A De Angelis, B De Lotto, M Delfino, J Delgado, M Doert, A Domínguez, D Dominis Prester, M Doro, M Engelkemeier, V Fallah Ramazani, A Fernández-Barral, D Fidalgo, MV Fonseca, L Font, C Fruck, D Galindo, RJ García López, M Garczarczyk, M Gaug, P Giammaria, N Godinović, D Gora, D Guberman, D Hadasch, A Hahn, T Hassan, M Hayashida, J Herrera, J Hose, D Hrupec, K Ishio, Y Konno, H Kubo, J Kushida, D Kuveždić, D Lelas, E Lindfors, S Lombardi, F Longo, M López, C Maggio, P Majumdar, M Makariev, G Maneva, M Manganaro, L Maraschi, M Mariotti, M Martínez, D Mazin, U Menzel, M Minev, JM Miranda, R Mirzoyan, A Moralejo, V Moreno, E Moretti, T Nagayoshi, V Neustroev, A Niedzwiecki, M Nievas Rosillo, C Nigro, K Nilsson, D Ninci, K Nishijima, K Noda, L Nogués, S Paiano, J Palacio, D Paneque, R Paoletti, JM Paredes, G Pedaletti, M Peresano, L Perri, M Persic, PG Prada Moroni, E Prandini, I Puljak, JR Garcia, I Reichardt, M Ribó, J Rico, C Righi, A Rugliancich, T Saito, K Satalecka, S Schroeder, T Schweizer, SN Shore, J Sitarek, I Šnidarić, D Sobczynska, A Stamerra, M Strzys, T Surić, L Takalo, F Tavecchio, P Temnikov, T Terzić, M Teshima, N Torres-Albà, A Treves, S Tsujimoto, G Vanzo, M Vazquez Acosta, I Vovk, JE Ward, M Will, D Zarić, A Arbet-Engels, D Baack, M Balbo, A Biland, M Blank, T Bretz, K Bruegge, M Bulinski, J Buss, A Dmytriiev, D Dorner, S Einecke, D Elsaesser
Publication date
2018/12/1
Journal
Astronomy & astrophysics
Volume
620
Pages
A181
Publisher
EDP Sciences
Description
Aims
We aim to characterize the multiwavelength emission from Markarian 501 (Mrk 501), quantify the energy-dependent variability, study the potential multiband correlations, and describe the temporal evolution of the broadband emission within leptonic theoretical scenarios.
Methods
We organized a multiwavelength campaign to take place between March and July of 2012. Excellent temporal coverage was obtained with more than 25 instruments, including the MAGIC, FACT and VERITAS Cherenkov telescopes, the instruments on board the Swift and Fermi spacecraft, and the telescopes operated by the GASP-WEBT collaboration.
Results
Mrk 501 showed a very high energy (VHE) gamma-ray flux above 0.2 TeV of ∼0.5 times the Crab Nebula flux (CU) for most of the campaign. The highest activity occurred on 2012 June 9, when the VHE flux was ∼3 CU, and the peak of the high-energy spectral component was …
Scholar articles
ML Ahnen, S Ansoldi, LA Antonelli, C Arcaro, A Babić… - Astronomy & astrophysics, 2018