H.E.S.S. discovery of very high energy γ-ray emission from PKS 0625−354

H Abdalla, A Abramowski, F Aharonian, F Ait Benkhali, A G Akhperjanian, T Andersson, E O Angüner, M Arrieta, P Aubert, M Backes, A Balzer,M Barnard, Y Becherini, J Becker Tjus, D Berge, S Bernhard, K Bernlöhr, R Blackwell, M Böttcher, C Boisson, J Bolmont, P Bordas, J Bregeon, F Brun, P Brun, M Bryan, T Bulik, M Capasso, J Carr, S Casanova, M Cerruti, N Chakraborty, R Chalme-Calvet, R C G Chaves, A Chen, J Chevalier, M Chrétien, S Colafrancesco, G Cologna, B Condon, J Conrad, Y Cui,I D Davids, J Decock, B Degrange, C Deil, J Devin, P deWilt, L Dirson, A Djannati-Ataï, W Domainko, A Donath, L O'C Drury, G Dubus, K Dutson, J Dyks, M Dyrda, T Edwards, K Egberts, P Eger, J-P Ernenwein, S Eschbach, C Farnier, S Fegan, M V Fernandes, A Fiasson, G Fontaine, A Förster, S Funk, M Füßling, S Gabici, M Gajdus, Y A Gallant, T Garrigoux, G Giavitto, B Giebels, J F Glicenstein, D Gottschall, A Goyal, M-H Grondin, D Hadasch, J Hahn, M Haupt, J Hawkes, G Heinzelmann, G Henri, G Hermann, O Hervet, J A Hinton, W Hofmann, C Hoischen, M Holler, D Horns, A Ivascenko, A Jacholkowska, M Jamrozy, M Janiak, D Jankowsky, F Jankowsky, M Jingo, T Jogler, L Jouvin, I Jung-Richardt, M A Kastendieck, K Katarzyński, U Katz, D Kerszberg, B Khélifi, M Kieffer, J King, S Klepser, D Klochkov, W Kluźniak, D Kolitzus, Nu Komin, K Kosack, S Krakau, M Kraus, F Krayzel, P P Krüger, H Laffon, G Lamanna, J Lau, J-P Lees, J Lefaucheur, V Lefranc, A Lemière, M Lemoine-Goumard, J-P Lenain, E Leser, T Lohse, M Lorentz, R Liu, R López-Coto, I Lypova, V Marandon, A Marcowith, C Mariaud, R Marx, G Maurin, N Maxted, M Mayer, P J Meintjes, M Meyer, A M W Mitchell, R Moderski, M Mohamed, L Mohrmann, K Morå, E Moulin, T Murach, M de Naurois, F Niederwanger, J Niemiec, L Oakes, P O'Brien, H Odaka, S Öttl, S Ohm, M Ostrowski, I Oya, M Padovani, M Panter, R D Parsons,N W Pekeur, G Pelletier, C Perennes, P-O Petrucci, B Peyaud, Q Piel, S Pita, H Poon, D Prokhorov, H Prokoph, G Pühlhofer, M Punch, A Quirrenbach, S Raab, A Reimer, O Reimer, M Renaud, R de los Reyes, F Rieger, C Romoli, S Rosier-Lees, G Rowell, B Rudak, C B Rulten, V Sahakian, D Salek, D A Sanchez, A Santangelo, M Sasaki, R Schlickeiser, F Schüssler, A Schulz, U Schwanke, S Schwemmer, M Settimo,A S Seyffert, N Shafi, I Shilon, R Simoni, H Sol,F Spanier, G Spengler, F Spies, Ł Stawarz, R Steenkamp, C Stegmann, F Stinzing, K Stycz,I Sushch, J-P Tavernet, T Tavernier, A M Taylor, R Terrier, L Tibaldo, D Tiziani, M Tluczykont, C Trichard, R Tuffs, Y Uchiyama,D J van der Walt, C van Eldik,C van Rensburg, B van Soelen, G Vasileiadis, J Veh, C Venter, A Viana, P Vincent, J Vink, F Voisin, H J Völk, T Vuillaume,Z Wadiasingh, S J Wagner, P Wagner, R M Wagner, R White, A Wierzcholska, P Willmann, A Wörnlein, D Wouters, R Yang, V Zabalza, D Zaborov, M Zacharias, R Zanin, A A Zdziarski, A Zech, F Zefi, A Ziegler, N Żywucka

Monthly Notices of the Royal Astronomical Society（2018）

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摘要

PKS 0625-354 (z = 0.055) was observed with the four High Energy Stereoscopic System (H.E.S.S.) telescopes in 2012 during 5.5 h. The source was detected above an energy threshold of 200 GeV at a sig ...

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