학술논문

Very high energy $\gamma$-ray emission from two blazars of unknown redshift and upper limits on their distance
Document Type
Working Paper
Author
Collaboration, H. E. S. S.Abdalla, H.Adam, R.Aharonian, F.Benkhali, F. AitAngüner, E. O.Arakawa, M.Arcaro, C.Armand, C.Armstrong, T.Ashkar, H.Backes, M.Baghmanyan, V.Martins, V. BarbosaBarnacka, A.Barnard, M.Becherini, Y.Berge, D.Bernlöhr, K.Böttcher, M.Boisson, C.Bolmont, J.Bonnefoy, S.Bregeon, J.Breuhaus, M.Brun, F.Brun, P.Bryan, M.Büchele, M.Bulik, T.Bylund, T.Caroff, S.Carosi, A.Casanova, S.Chand, T.Chandra, S.Chen, A.Cotter, G.Curyło, M.Davids, I. D.Davies, J.Deil, C.Devin, J.deWilt, P.Dirson, L.Djannati-Ataï, A.Dmytriiev, A.Donath, A.Doroshenko, V.Dyks, J.Egberts, K.Eichhorn, F.Emery, G.Ernenwein, J. -P.Feijen, K.Fegan, S.Fiasson, A.Fontaine, G.Funk, S.Füßling, M.Gabici, S.Gallant, Y. A.Giavitto, G.Giunti, L.Glawion, D.Glicenstein, J. F.Gottschall, D.Grondin, M. -H.Hahn, J.Haupt, M.Hermann, G.Hinton, J. A.Hofmann, W.Hoischen, C.Holch, T. L.Holler, M.H{\"}orbe, M.; Horns, D.Huber, D.Iwasaki, H.Jamrozy, M.Jankowsky, D.Jankowsky, F.Jardin-Blicq, A.Joshi, V.Jung-Richardt, I.Kastendieck, M. A.Katarzynski, K.Katsuragawa, M.Katz, U.Khangulyan, D.Khélifi, B.Klepser, S.Kluzniak, W.Komin, Nu.Konno, R.Kosack, K.Kostunin, D.Kreter, M.Lamanna, G.Lemière, A.Lemoine-Goumard, M.Lenain, J. -P.Leser, E.Levy, C.Lohse, T.Lypova, I.Mackey, J.Majumdar, J.Malyshev, D.Marandon, V.Marchegiani, P.Marcowith, A.Mares, A.Martí-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, V.Noel, A. PriyanaProkhorov, D. A.Prokoph, H.Pühlhofer, G.Punch, M.Quirrenbach, 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, V.Sailer, S.Saito, S.Sanchez, D. A.Santangelo, A.Sasaki, M.Scalici, M.Schüssler, F.Schutte, H. M.Schwanke, U.Schwemmer, S.Seglar-Arroyo, M.Senniappan, M.Seyffert, A. S.Shafi, N.Shiningayamwe, K.Simoni, R.Sinha, A.Sol, H.Specovius, A.Spencer, S.Spir-Jacob, M.Stawarz, Ł.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.Völk, 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.Żywucka, N.Cerruti, M.
Source
Subject
Astrophysics - High Energy Astrophysical Phenomena
Language
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 multi-wavelength observations with Fermi/LAT, XRT and UVOT on board the Swift satellite, and ATOM. Based on an extrapolation of the Fermi/LAT spectrum towards the VHE $\gamma$-ray regime, we deduce a 95% 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 $0.51 \leq z < 0.98$ and for PKS 1440-389 to $0.14 \lessapprox z < 0.53$.
Comment: Accepted for publication in MNRAS. 13 pages, 4 figures