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@ARTICLE{Collaboration:193032,
author = {: and Abramowski, A. and Aharonian, F. and Benkhali, F. Ait
and Akhperjanian, A. G. and Angüner, E. and Anton, G. and
Balenderan, S. and Balzer, A. and Barnacka, A. and
Becherini, Y. and Tjus, J. Becker and Bernlöhr, K. and
Birsin, E. and Bissaldi, E. and Biteau, J. and Boettcher,
Mathias and Boisson, C. and Bolmont, J. and Bordas, P. and
Brucker, J. and Brun, F. and Brun, P. and Bulik, T. and
Carrigan, S. and Casanova, S. and Cerruti, M. and Chadwick,
P. M. and Chalme-Calvet, R. and Chaves, R. C. G. and
Cheesebrough, A. and Chrétien, M. and Colafrancesco, S. and
Cologna, G. and Conrad, J. and Couturier, C. and Cui, Y. and
Dalton, M. and Daniel, M. K. and Davids, I. D. and Degrange,
B. and Deil, C. and deWilt, P. and Dickinson, H. J. and
Djannati-Ataï, A. and Domainko, W. and Drury, L. O'C. and
Dubus, G. and Dutson, K. and Dyks, J. and Dyrda, M. and
Edwards, T. and Egberts, K. and Eger, P. and Espigat, P. and
Farnier, C. and Fegan, S. and Feinstein, F. and Fernandes,
M. V. and Fernandez, D. and Fiasson, A. and Fontaine, G. and
Förster, A. and Füßling, M. and Gajdus, M. and Gallant,
Y. A. and Garrigoux, T. and Giavitto, G. and Giebels, B. and
Glicenstein, J. F. and Grondin, M. -H. and Grudzińska, M.
and Häffner, S. and Hahn, J. and Harris, J. and
Heinzelmann, G. and Henri, G. and Hermann, G. and Hervet, O.
and Hillert, A. and Hinton, J. A. and Hofmann, W. and
Hofverberg, P. and Holler, M. and Horns, D. and
Jacholkowska, A. and Jahn, C. and Jamrozy, M. and Janiak, M.
and Jankowsky, F. and Jung, I. and Kastendieck, Max and
Katarzyński, K. and Katz, U. and Kaufmann, S. and Khélifi,
B. and Kieffer, M. and Klepser, S. and Klochkov, D. and
Kluźniak, W. and Kneiske, T. and Kolitzus, D. and Komin,
Nu. and Kosack, K. and Krakau, S. and Krayzel, F. and
Krüger, P. P. and Laffon, H. and Lamanna, G. and
Lefaucheur, J. and Lemière, A. and Lemoine-Goumard, M. and
Lenain, J. -P. and Lennarz, D. and Lohse, T. and Lopatin, A.
and Lu, C. -C. and Marandon, V. and Marcowith, A. and Marx,
R. and Maurin, G. and Maxted, N. and Mayer, Michael and
McComb, T. J. L. and Méhault, J. and Meintjes, P. J. and
Menzler, U. and Meyer, M. and Moderski, R. and Mohamed, M.
and Moulin, E. and Murach, T. and Naumann, C. L. and de
Naurois, M. and Niemiec, J. and Nolan, S. J. and Oakes, L.
and Ohm, S. and Wilhelmi, E. de O na and Opitz, B. and
Ostrowski, M. and Oya, I. and Panter, M. and Parsons, R. D.
and Arribas, M. Paz and Pekeur, N. W. and Pelletier, G. and
Perez, J. and Petrucci, P. -O. and Peyaud, B. and Pita, S.
and Poon, H. and Pühlhofer, G. and Punch, M. and
Quirrenbach, A. and Raab, S. and Raue, M. and Reimer, A. and
Reimer, O. and Renaud, M. and Reyes, R. de los and Rieger,
F. and Rob, L. and Romoli, C. and Rosier-Lees, S. and
Rowell, G. and Rudak, B. and Rulten, C. B. and Sahakian, V.
and Sanchez, Daniel and Santangelo, A. and Schlickeiser, R.
and Schüssler, F. and Schulz, A. and Schwanke, U. and
Schwarzburg, S. and Schwemmer, S. and Sol, H. and Spengler,
G. and Spies, F. and Stawarz, L. and Steenkamp, R. and
Stegmann, C. and Stinzing, F. and Stycz, K. and Sushch, I.
and Szostek, A. and Tavernet, J. -P. and Tavernier, T. and
Taylor, A. M. and Terrier, R. and Tluczykont, M. and
Trichard, C. and Valerius, K. and van Eldik, C. and van
Soelen, B. and Vasileiadis, G. and Venter, C. and Viana, A.
and Vincent, P. and Völk, H. J. and Volpe, F. and Vorster,
M. and Vuillaume, T. and Wagner, S. J. and Wagner, P. and
Ward, M. and Weidinger, M. and Weitzel, Q. and White, R. and
Wierzcholska, A. and Willmann, P. and Wörnlein, A. and
Wouters, D. and Zabalza, V. and Zacharias, M. and Zajczyk,
A. and Zdziarski, A. A. and Zech, A. and Zechlin,
Hannes-Sebastian},
collaboration = {H.E.S.S.{ Collaboration}},
title = {{D}iscovery of the {VHE} gamma-ray source {HESS}
{J}1832-093 in the vicinity of {SNR} {G}22.7-0.2},
reportid = {PUBDB-2014-04479, arXiv:1411.0572},
pages = {2-6},
year = {2014},
note = {OA},
abstract = {The region around the supernova remnant (SNR) W41 contains
several TeV sources and has prompted the H.E.S.S.
Collaboration to perform deep observations of this field of
view. This resulted in the discovery of the new very high
energy (VHE) source HESS J1832-093, at the position $\rm
RA=18^h 32^m 50^s \pm 3^s_{stat} \pm 2^s_{syst}, \rm
Dec=-9^\circ 22' 36'' \pm 32''_{stat} \pm 20''_{syst}
(J2000)$, spatially coincident with a part of the radio
shell of the neighboring remnant G22.7-0.2. The photon
spectrum is well described by a power-law of index $\Gamma =
2.6 \pm 0.3_{\rm stat} \pm 0.1_{\rm syst}$ and a
normalization at 1 TeV of $\Phi_0=(4.8 \pm 0.8_{\rm stat}\pm
1.0_{\rm syst})\,\times\,10^{-13}\,\rm{cm}
^{-2}\,s^{-1}\,TeV^{-1}$. The location of the gamma-ray
emission on the edge of the SNR rim first suggested a
signature of escaping cosmic-rays illuminating a nearby
molecular cloud. Then a dedicated XMM-Newton observation led
to the discovery of a new X-ray point source spatially
coincident with the TeV excess. Two other scenarios were
hence proposed to identify the nature of HESS J1832-093.
Gamma-rays from inverse Compton radiation in the framework
of a pulsar wind nebula scenario or the possibility of
gamma-ray production within a binary system are therefore
also considered. Deeper multi-wavelength observations will
help to shed new light on this intriguing VHE source.},
cin = {ZEU-EXP/AT},
cid = {$I:(DE-H253)ZEU-EXP_AT-20120731$},
pnm = {523 - High-energy gamma ray astronomy (POF2-523)},
pid = {G:(DE-HGF)POF2-523},
experiment = {EXP:(DE-MLZ)NOSPEC-20140101},
typ = {PUB:(DE-HGF)25 / PUB:(DE-HGF)15},
eprint = {1411.0572},
howpublished = {arXiv:1411.0572},
archivePrefix = {arXiv},
SLACcitation = {$\%\%CITATION$ = $arXiv:1411.0572;\%\%$},
url = {https://bib-pubdb1.desy.de/record/193032},
}
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