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
user-5fe1a78c4c775e6ec07359f9(2018)
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Abstract
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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emission
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