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Very high energy $��$-ray emission from two blazars of unknown redshift and upper limits on their distance

Authors :
Collaboration, H. E. S. S.
Abdalla, H.
Adam, R.
Aharonian, F.
Benkhali, F. Ait
Ang��ner, E. O.
Arakawa, M.
Arcaro, C.
Armand, C.
Armstrong, T.
Ashkar, H.
Backes, M.
Baghmanyan, V.
Martins, V. Barbosa
Barnacka, A.
Barnard, M.
Becherini, Y.
Berge, D.
Bernl��hr, K.
B��ttcher, M.
Boisson, C.
Bolmont, J.
Bonnefoy, S.
Bregeon, J.
Breuhaus, M.
Brun, F.
Brun, P.
Bryan, M.
B��chele, M.
Bulik, T.
Bylund, T.
Caroff, S.
Carosi, A.
Casanova, S.
Chand, T.
Chandra, S.
Chen, A.
Cotter, G.
Cury��o, M.
Davids, I. D.
Davies, J.
Deil, C.
Devin, J.
deWilt, P.
Dirson, L.
Djannati-Ata��, 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.
F����ling, 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.
Kh��lifi, B.
Klepser, S.
Kluzniak, W.
Komin, Nu.
Konno, R.
Kosack, K.
Kostunin, D.
Kreter, M.
Lamanna, G.
Lemi��re, 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.
Mart��-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 Ona
Ostrowski, M.
Panter, M.
Parsons, R. D.
Peyaud, B.
Piel, Q.
Pita, S.
Poireau, V.
Noel, A. Priyana
Prokhorov, D. A.
Prokoph, H.
P��hlhofer, 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.
Sch��ssler, 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, ��.
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.
V��lk, 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.
��ywucka, N.
Cerruti, M.
Publication Year :
2020
Publisher :
arXiv, 2020.

Abstract

We report on the detection of very-high-energy (VHE; $E > 100$ GeV) $��$-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 $��$-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 $0.14 \lessapprox z < 0.53$.<br />Accepted for publication in MNRAS. 13 pages, 4 figures

Details

ISSN :
03111938
Database :
OpenAIRE
Accession number :
edsair.doi...........269c96f79d3111cf331866f50d5c6f82
Full Text :
https://doi.org/10.48550/arxiv.2004.03306