학술논문

Very high energy gamma-ray emission from two blazars of unknown redshift and upper limits on their distance
Document Type
Author
Abdalla, H.Adam, R.Aharonian, F.Benkhali, F. AitAnguner, E. O.Arakawa, M.Arcaro, C.Armand, C.Armstrong, T.Ashkar, H.Backes, M.Baghmanyan, VMartins, V. BarbosaBarnacka, A.Barnard, M.Becherini, YvonneBerge, D.Bernloehr, K.Bottcher, M.Boisson, C.Bolmont, J.Bonnefoy, S.Bregeon, J.Breuhaus, M.Brun, F.Brun, P.Bryan, M.Buechele, M.Bulik, T.Bylund, TomasCaroff, S.Carosi, A.Casanova, S.Chand, T.Chandra, S.Chen, A.Cotter, G.Curylo, M.Davids, I. D.Davies, J.Deil, C.Devin, J.deWilt, P.Dirson, L.Djannati-Atai, A.Dmytriiev, A.Donath, A.Doroshenko, VDyks, J.Egberts, K.Eichhorn, F.Emery, G.Ernenwein, J-PFeijen, K.Fegan, S.Fiasson, A.Fontaine, G.Funk, S.Fuessling, M.Gabici, S.Gallant, Y. A.Giavitto, G.Giunti, L.Glawion, D.Glicenstein, J. F.Gottschall, D.Grondin, M-HHahn, J.Haupt, M.Hermann, G.Hinton, J. A.Hofmann, W.Hoischen, C.Holch, T. L.Holler, M.Hoerbe, M.Horns, D.Huber, D.Iwasaki, H.Jamrozy, M.Jankowsky, D.Jankowsky, F.Jardin-Blicq, A.Joshi, VJung-Richardt, IKastendieck, M. A.Katarzyski, K.Katsuragawa, M.Katz, U.Khangulyan, D.Khelifi, B.Klepser, S.Kluzniak, W.Komin, NuKonno, R.Kosack, K.Kostunin, D.Kreter, M.Lamanna, G.Lemiere, A.Lemoine-Goumard, M.Lenain, J-PLeser, E.Levy, C.Lohse, T.Lypova, IMackey, J.Majumdar, J.Malyshev, D.Marandon, VMarchegiani, P.Marcowith, A.Mares, A.Marti-Devesa, G.Marx, R.Maurin, G.Meintjes, P. J.Moderski, R.Mohamed, M.Mohrmann, L.Moore, C.Morris, P.Moulin, E.Muller, J.Murach, T.Nakashima, S.Nakashima, K.de Naurois, M.Ndiyavala, H.Niederwanger, F.Niemiec, J.Oakes, L.O'Brien, P.Odaka, H.Ohm, S.Wilhelmi, E. de OnaOstrowski, M.Panter, M.Parsons, R. D.Peyaud, B.Piel, Q.Pita, S.Poireau, VNoel, A. P.Prokhorov, D. A.Prokoph, H.Puehlhofer, G.Punch, MichaelQuirrenbach, A.Raab, S.Rauth, R.Reimer, A.Reimer, O.Remy, Q.Renaud, M.Rieger, F.Rinchiuso, L.Romoli, C.Rowell, G.Rudak, B.Ruiz-Velasco, E.Sahakian, VSailer, S.Saito, S.Sanchez, D. A.Santangelo, A.Sasaki, M.Scalici, M.Schussler, F.Schutte, H. M.Schwanke, U.Schwemmer, S.Seglar-Arroyo, M.Senniappan, MohanrajSeyffert, A. S.Shafi, N.Shiningayamwe, K.Simoni, R.Sinha, A.Sol, H.Specovius, A.Spencer, S.Spir-Jacob, M.Stawarz, L.Steenkamp, R.Stegmann, C.Steppa, C.Takahashi, T.Tavernier, T.Taylor, A. M.Terrier, R.Tiziani, D.Tluczykont, M.Tomankova, L.Trichard, C.Tsirou, M.Tsuji, N.Tuffs, R.Uchiyama, Y.van der Walt, D. J.van Eldik, C.van Rensburg, C.van Soelen, B.Vasileiadis, G.Veh, J.Venter, C.Vincent, P.Vink, J.Voelk, H. J.Vuillaume, T.Wadiasingh, Z.Wagner, S. J.Watson, J.Werner, F.White, R.Wierzcholska, A.Yang, R.Yoneda, H.Zacharias, M.Zanin, R.Zargaryan, D.Zdziarski, A. A.Zech, A.Zhu, S. J.Zorn, J.Zywucka, N.Cerruti, M.
Source
Monthly notices of the Royal Astronomical Society. 494(4):5590-5602
Subject
BL Lacertae objects: individual
galaxies: high-redshift
gamma-rays: general
Resolved and unresolved sources as a function of wavelength
Astroparticle Physics
Astropartikelfysik
Language
English
ISSN
0035-8711
1365-2966
Abstract
We report on the detection of very high energy (VHE; E > 100 GeV) gamma-ray emission from the BL Lac objects KUV 00311-1938 and PKS 1440-389 with the High Energy Stereoscopic System (H.E.S.S.). H.E.S.S. observations were accompanied or preceded by multiwavelength observations with Fermi/LAT, XRT and UVOT onboard the Swift satellite, and ATOM. Based on an extrapolation of the Fermi/LAT spectrum towards the VHE gamma-ray regime, we deduce a 95 per cent confidence level upper limit on the unknown redshift of KUV 00311-1938 of z < 0.98 and of PKS 1440-389 of z < 0.53. When combined with previous spectroscopy results, the redshift of KUV 00311-1938 is constrained to 0.51 <= z < 0.98 and of PKS 1440-389 to 0.14 (sic) z < 0.53.