H.E.S.S. reveals a lack of TeV emission from the supernova remnant Puppis A

2015
journal article
article
14
cris.lastimport.wos2024-04-09T19:07:06Z
dc.abstract.enContext. Puppis A is an interesting ~4 kyr-old supernova remnant (SNR) that shows strong evidence of interaction between the forward shock and a molecular cloud. It has been studied in detail from radio frequencies to high-energy (HE, 0.1−100 GeV) γ-rays. An analysis of the Fermi-LAT data has shown extended HE $\gamma$-ray emission with a 0.2−100 GeV spectrum exhibiting no significant deviation from a power law, unlike most of the GeV-emitting SNRs known to be interacting with molecular clouds. This makes it a promising target for imaging atmospheric Cherenkov telescopes (IACTs) to probe the $\gamma$-ray emission above 100 GeV. Aims. Very-high-energy (VHE, E ≥ 0.1 TeV) $\gamma$-ray emission from Puppis A has been, for the first time, searched for with the High Energy Stereoscopic System (H.E.S.S.). Methods. Stereoscopic imaging of Cherenkov radiation from extensive air showers is used to reconstruct the direction and energy of the incident γ-rays in order to produce sky images and source spectra. The profile likelihood method is applied to find constraints on the existence of a potential break or cutoff in the photon spectrum. Results. The analysis of the H.E.S.S. data does not reveal any significant emission towards Puppis A. The derived upper limits on the differential photon flux imply that its broadband $\gamma$-ray spectrum must exhibit a spectral break or cutoff. By combining Fermi-LAT and H.E.S.S. measurements, the 99% confidence-level upper limits on such a cutoff are found to be 450 and 280 GeV, assuming a power law with a simple exponential and a sub-exponential cutoff, respectively. It is concluded that none of the standard limitations (age, size, radiative losses) on the particle acceleration mechanism, assumed to be continuing at present, can explain the lack of VHE signal. The scenario in which particle acceleration has ceased some time ago is considered as an alternative explanation. The HE/VHE spectrum of Puppis A could then exhibit a break of non-radiative origin (as observed in several other interacting SNRs, albeit at somewhat higher energies), owing to the interaction with dense and neutral material, in particular towards the NE region.pl
dc.affiliationWydział Fizyki, Astronomii i Informatyki Stosowanej : Instytut – Obserwatorium Astronomicznepl
dc.contributor.authorAbramowski, A.pl
dc.contributor.authorAharonian, F.pl
dc.contributor.authorAit Benkhali, F.pl
dc.contributor.authorAkhperjanian, A. G.pl
dc.contributor.authorAngüner, E. O.pl
dc.contributor.authorBackes, M.pl
dc.contributor.authorBalenderan, S.pl
dc.contributor.authorBalzer, A.pl
dc.contributor.authorBarnacka, Anna - 241952 pl
dc.contributor.authorBecherini, Y.pl
dc.contributor.authorBecker Tjus, J.pl
dc.contributor.authorBerge, D.pl
dc.contributor.authorBernhard, S.pl
dc.contributor.authorBernlöhr, K.pl
dc.contributor.authorBirsin, E.pl
dc.contributor.authorBiteau, J.pl
dc.contributor.authorBöttcher, M.pl
dc.contributor.authorBoisson, C.pl
dc.contributor.authorBolmont, J.pl
dc.contributor.authorBordas, P.pl
dc.contributor.authorBregeon, J.pl
dc.contributor.authorBrun, F.pl
dc.contributor.authorBrun, P.pl
dc.contributor.authorBryan, M.pl
dc.contributor.authorBulik, T.pl
dc.contributor.authorCarrigan, S.pl
dc.contributor.authorCasanova, S.pl
dc.contributor.authorChadwick, P. M.pl
dc.contributor.authorChakraborty, N.pl
dc.contributor.authorChalme-Calvet, R.pl
dc.contributor.authorChaves, R. C. G.pl
dc.contributor.authorChrétien, M.pl
dc.contributor.authorColafrancesco, S.pl
dc.contributor.authorCologna, G.pl
dc.contributor.authorConrad, J.pl
dc.contributor.authorCouturier, C.pl
dc.contributor.authorCui, Y.pl
dc.contributor.authorDavids, I. D.pl
dc.contributor.authorDegrange, B.pl
dc.contributor.authorDeil, C.pl
dc.contributor.authordeWilt, P.pl
dc.contributor.authorDjannati-Ataï, A.pl
dc.contributor.authorDomainko, W.pl
dc.contributor.authorDonath, A.pl
dc.contributor.authorDrury, L. O’C.pl
dc.contributor.authorDubus, G.pl
dc.contributor.authorDutson, K.pl
dc.contributor.authorDyks, J.pl
dc.contributor.authorDyrda, M.pl
dc.contributor.authorEdwards, T.pl
dc.contributor.authorEgberts, K.pl
dc.contributor.authorEger, P.pl
dc.contributor.authorEspigat, P.pl
dc.contributor.authorFarnier, C.pl
dc.contributor.authorFegan, S.pl
dc.contributor.authorFeinstein, F.pl
dc.contributor.authorFernandes, M. V.pl
dc.contributor.authorFernandez, D.pl
dc.contributor.authorFiasson, A.pl
dc.contributor.authorFontaine, G.pl
dc.contributor.authorFörster, A.pl
dc.contributor.authorFüßling, M.pl
dc.contributor.authorGabici, S.pl
dc.contributor.authorGajdus, M.pl
dc.contributor.authorGallant, Y. A.pl
dc.contributor.authorGarrigoux, T.pl
dc.contributor.authorGiavitto, G.pl
dc.contributor.authorGiebels, B.pl
dc.contributor.authorGlicenstein, J. F.pl
dc.contributor.authorGottschall, D.pl
dc.contributor.authorGrondin, M.-H.pl
dc.contributor.authorGrudzińska, M.pl
dc.contributor.authorHadasch, D.pl
dc.contributor.authorHäffner, S.pl
dc.contributor.authorHahn, J.pl
dc.contributor.authorHarris, J.pl
dc.contributor.authorHeinzelmann, G.pl
dc.contributor.authorHenri, G.pl
dc.contributor.authorHermann, G.pl
dc.contributor.authorHervet, O.pl
dc.contributor.authorHillert, A.pl
dc.contributor.authorHinton, J. A.pl
dc.contributor.authorHofmann, W.pl
dc.contributor.authorHofverberg, P.pl
dc.contributor.authorHoller, M.pl
dc.contributor.authorHorns, D.pl
dc.contributor.authorIvascenko, A.pl
dc.contributor.authorJacholkowska, A.pl
dc.contributor.authorJahn, C.pl
dc.contributor.authorJamrozy, Marek - 128434 pl
dc.contributor.authorJaniak, M.pl
dc.contributor.authorJankowsky, F.pl
dc.contributor.authorJung-Richardt, I.pl
dc.contributor.authorKastendieck, M. A.pl
dc.contributor.authorKatarzyński, K.pl
dc.contributor.authorKatz, U.pl
dc.contributor.authorKaufmann, S.pl
dc.contributor.authorKhélifi, B.pl
dc.contributor.authorKieffer, M.pl
dc.contributor.authorKlepser, S.pl
dc.contributor.authorKlochkov, D.pl
dc.contributor.authorKluźniak, W.pl
dc.contributor.authorKolitzus, D.pl
dc.contributor.authorKomin, Nu.pl
dc.contributor.authorKosack, K.pl
dc.contributor.authorKrakau, S.pl
dc.contributor.authorKrayzel, F.pl
dc.contributor.authorKrüger, P. P.pl
dc.contributor.authorLaffon, H.pl
dc.contributor.authorLamanna, G.pl
dc.contributor.authorLefaucheur, J.pl
dc.contributor.authorLefranc, V.pl
dc.contributor.authorLemière, A.pl
dc.contributor.authorLemoine-Goumard, M.pl
dc.contributor.authorLenain, J.-P.pl
dc.contributor.authorLohse, T.pl
dc.contributor.authorLopatin, A.pl
dc.contributor.authorLu, C.-C.pl
dc.contributor.authorMarandon, V.pl
dc.contributor.authorMarcowith, A.pl
dc.contributor.authorMarx, R.pl
dc.contributor.authorMaurin, G.pl
dc.contributor.authorMaxted, N.pl
dc.contributor.authorMayer, M.pl
dc.contributor.authorMcComb, T. J. L.pl
dc.contributor.authorMéhault, J.pl
dc.contributor.authorMeintjes, P. J.pl
dc.contributor.authorMenzler, U.pl
dc.contributor.authorMeyer, M.pl
dc.contributor.authorMitchell, A. M. W.pl
dc.contributor.authorModerski, R.pl
dc.contributor.authorMohamed, M.pl
dc.contributor.authorMorå, K.pl
dc.contributor.authorMoulin, E.pl
dc.contributor.authorMurach, T.pl
dc.contributor.authorde Naurois, M.pl
dc.contributor.authorNiemiec, J.pl
dc.contributor.authorNolan, S. J.pl
dc.contributor.authorOakes, L.pl
dc.contributor.authorOdaka, H.pl
dc.contributor.authorOhm, S.pl
dc.contributor.authorOpitz, B.pl
dc.contributor.authorOstrowski, Michał - 100042 pl
dc.contributor.authorOya, I.pl
dc.contributor.authorPanter, M.pl
dc.contributor.authorParsons, R. D.pl
dc.contributor.authorPaz Arribas, M.pl
dc.contributor.authorPekeur, N. W.pl
dc.contributor.authorPelletier, G.pl
dc.contributor.authorPetrucci, P.-O.pl
dc.contributor.authorPeyaud, B.pl
dc.contributor.authorPita, S.pl
dc.contributor.authorPoon, H.pl
dc.contributor.authorPühlhofer, G.pl
dc.contributor.authorPunch, M.pl
dc.contributor.authorQuirrenbach, A.pl
dc.contributor.authorRaab, S.pl
dc.contributor.authorReichardt, I.pl
dc.contributor.authorReimer, A.pl
dc.contributor.authorReimer, O.pl
dc.contributor.authorRenaud, M.pl
dc.contributor.authorde los Reyes, R.pl
dc.contributor.authorRieger, F.pl
dc.contributor.authorRomoli, C.pl
dc.contributor.authorRosier-Lees, S.pl
dc.contributor.authorRowell, G.pl
dc.contributor.authorRudak, B.pl
dc.contributor.authorRulten, C. B.pl
dc.contributor.authorSahakian, V.pl
dc.contributor.authorSalek, D.pl
dc.contributor.authorSanchez, D. A.pl
dc.contributor.authorSantangelo, A.pl
dc.contributor.authorSchlickeiser, R.pl
dc.contributor.authorSchüssler, F.pl
dc.contributor.authorSchulz, A.pl
dc.contributor.authorSchwanke, U.pl
dc.contributor.authorSchwarzburg, S.pl
dc.contributor.authorSchwemmer, S.pl
dc.contributor.authorSol, H.pl
dc.contributor.authorSpanier, F.pl
dc.contributor.authorSpengler, G.pl
dc.contributor.authorSpies, F.pl
dc.contributor.authorStawarz, Łukasz - 132081 pl
dc.contributor.authorSteenkamp, R.pl
dc.contributor.authorStegmann, C.pl
dc.contributor.authorStinzing, F.pl
dc.contributor.authorStycz, K.pl
dc.contributor.authorSushch, I.pl
dc.contributor.authorTavernet, J.-P.pl
dc.contributor.authorTavernier, T.pl
dc.contributor.authorTaylor, A. M.pl
dc.contributor.authorTerrier, R.pl
dc.contributor.authorTluczykont, M.pl
dc.contributor.authorTrichard, C.pl
dc.contributor.authorValerius, K.pl
dc.contributor.authorvan Eldik, C.pl
dc.contributor.authorvan Soelen, B.pl
dc.contributor.authorVasileiadis, G.pl
dc.contributor.authorVeh, J.pl
dc.contributor.authorVenter, C.pl
dc.contributor.authorViana, A.pl
dc.contributor.authorVincent, P.pl
dc.contributor.authorVink, J.pl
dc.contributor.authorVölk, H. J.pl
dc.contributor.authorVolpe, F.pl
dc.contributor.authorVorster, M.pl
dc.contributor.authorVuillaume, T.pl
dc.contributor.authorWagner, S. J.pl
dc.contributor.authorWagner, P.pl
dc.contributor.authorWagner, R. M.pl
dc.contributor.authorWard, M.pl
dc.contributor.authorWeidinger, M.pl
dc.contributor.authorWeitzel, Q.pl
dc.contributor.authorWhite, R.pl
dc.contributor.authorWierzcholska, Alicja - 113652 pl
dc.contributor.authorWillmann, P.pl
dc.contributor.authorWörnlein, A.pl
dc.contributor.authorWouters, D.pl
dc.contributor.authorYang, R.pl
dc.contributor.authorZabalza, V.pl
dc.contributor.authorZaborov, D.pl
dc.contributor.authorZacharias, M.pl
dc.contributor.authorZdziarski, A. A.pl
dc.contributor.authorZech, A.pl
dc.contributor.authorZechlin, H.-S.pl
dc.contributor.institutionH.E.S.S. Collaborationpl
dc.date.accessioned2015-07-13T16:54:00Z
dc.date.available2015-07-13T16:54:00Z
dc.date.issued2015pl
dc.date.openaccess12
dc.description.accesstimepo opublikowaniu
dc.description.additionalReproduced with permission from Astronomy & Astrophysics, © ESOpl
dc.description.admin[AU] Wierzcholska, Alicja [USOS30589]
dc.description.versionostateczna wersja wydawcy
dc.description.volume575pl
dc.identifier.articleidA81pl
dc.identifier.doi10.1051/0004-6361/201424805pl
dc.identifier.eissn1432-0746pl
dc.identifier.issn0004-6361pl
dc.identifier.projectROD UJ / Ppl
dc.identifier.urihttp://ruj.uj.edu.pl/xmlui/handle/item/12657
dc.languageengpl
dc.language.containerengpl
dc.rightsUdzielam licencji. Uznanie autorstwa - Użycie niekomercyjne - Na tych samych warunkach 4.0 Międzynarodowa*
dc.rights.licenceOTHER
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/4.0/legalcode.pl*
dc.share.typeotwarte czasopismo
dc.subject.engamma rays: ISMpl
dc.subject.enISM: individual objects: Puppis Apl
dc.subject.enradiation mechanisms: non-thermalpl
dc.subject.encosmic rayspl
dc.subject.enacceleration of particlespl
dc.subtypeArticlepl
dc.titleH.E.S.S. reveals a lack of TeV emission from the supernova remnant Puppis Apl
dc.title.journalAstronomy & Astrophysicspl
dc.typeJournalArticlepl
dspace.entity.typePublication
cris.lastimport.wos
2024-04-09T19:07:06Z
dc.abstract.enpl
Context. Puppis A is an interesting ~4 kyr-old supernova remnant (SNR) that shows strong evidence of interaction between the forward shock and a molecular cloud. It has been studied in detail from radio frequencies to high-energy (HE, 0.1−100 GeV) γ-rays. An analysis of the Fermi-LAT data has shown extended HE $\gamma$-ray emission with a 0.2−100 GeV spectrum exhibiting no significant deviation from a power law, unlike most of the GeV-emitting SNRs known to be interacting with molecular clouds. This makes it a promising target for imaging atmospheric Cherenkov telescopes (IACTs) to probe the $\gamma$-ray emission above 100 GeV. Aims. Very-high-energy (VHE, E ≥ 0.1 TeV) $\gamma$-ray emission from Puppis A has been, for the first time, searched for with the High Energy Stereoscopic System (H.E.S.S.). Methods. Stereoscopic imaging of Cherenkov radiation from extensive air showers is used to reconstruct the direction and energy of the incident γ-rays in order to produce sky images and source spectra. The profile likelihood method is applied to find constraints on the existence of a potential break or cutoff in the photon spectrum. Results. The analysis of the H.E.S.S. data does not reveal any significant emission towards Puppis A. The derived upper limits on the differential photon flux imply that its broadband $\gamma$-ray spectrum must exhibit a spectral break or cutoff. By combining Fermi-LAT and H.E.S.S. measurements, the 99% confidence-level upper limits on such a cutoff are found to be 450 and 280 GeV, assuming a power law with a simple exponential and a sub-exponential cutoff, respectively. It is concluded that none of the standard limitations (age, size, radiative losses) on the particle acceleration mechanism, assumed to be continuing at present, can explain the lack of VHE signal. The scenario in which particle acceleration has ceased some time ago is considered as an alternative explanation. The HE/VHE spectrum of Puppis A could then exhibit a break of non-radiative origin (as observed in several other interacting SNRs, albeit at somewhat higher energies), owing to the interaction with dense and neutral material, in particular towards the NE region.
dc.affiliationpl
Wydział Fizyki, Astronomii i Informatyki Stosowanej : Instytut – Obserwatorium Astronomiczne
dc.contributor.authorpl
Abramowski, A.
dc.contributor.authorpl
Aharonian, F.
dc.contributor.authorpl
Ait Benkhali, F.
dc.contributor.authorpl
Akhperjanian, A. G.
dc.contributor.authorpl
Angüner, E. O.
dc.contributor.authorpl
Backes, M.
dc.contributor.authorpl
Balenderan, S.
dc.contributor.authorpl
Balzer, A.
dc.contributor.authorpl
Barnacka, Anna - 241952
dc.contributor.authorpl
Becherini, Y.
dc.contributor.authorpl
Becker Tjus, J.
dc.contributor.authorpl
Berge, D.
dc.contributor.authorpl
Bernhard, S.
dc.contributor.authorpl
Bernlöhr, K.
dc.contributor.authorpl
Birsin, E.
dc.contributor.authorpl
Biteau, J.
dc.contributor.authorpl
Böttcher, M.
dc.contributor.authorpl
Boisson, C.
dc.contributor.authorpl
Bolmont, J.
dc.contributor.authorpl
Bordas, P.
dc.contributor.authorpl
Bregeon, J.
dc.contributor.authorpl
Brun, F.
dc.contributor.authorpl
Brun, P.
dc.contributor.authorpl
Bryan, M.
dc.contributor.authorpl
Bulik, T.
dc.contributor.authorpl
Carrigan, S.
dc.contributor.authorpl
Casanova, S.
dc.contributor.authorpl
Chadwick, P. M.
dc.contributor.authorpl
Chakraborty, N.
dc.contributor.authorpl
Chalme-Calvet, R.
dc.contributor.authorpl
Chaves, R. C. G.
dc.contributor.authorpl
Chrétien, M.
dc.contributor.authorpl
Colafrancesco, S.
dc.contributor.authorpl
Cologna, G.
dc.contributor.authorpl
Conrad, J.
dc.contributor.authorpl
Couturier, C.
dc.contributor.authorpl
Cui, Y.
dc.contributor.authorpl
Davids, I. D.
dc.contributor.authorpl
Degrange, B.
dc.contributor.authorpl
Deil, C.
dc.contributor.authorpl
deWilt, P.
dc.contributor.authorpl
Djannati-Ataï, A.
dc.contributor.authorpl
Domainko, W.
dc.contributor.authorpl
Donath, A.
dc.contributor.authorpl
Drury, L. O’C.
dc.contributor.authorpl
Dubus, G.
dc.contributor.authorpl
Dutson, K.
dc.contributor.authorpl
Dyks, J.
dc.contributor.authorpl
Dyrda, M.
dc.contributor.authorpl
Edwards, T.
dc.contributor.authorpl
Egberts, K.
dc.contributor.authorpl
Eger, P.
dc.contributor.authorpl
Espigat, P.
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Farnier, C.
dc.contributor.authorpl
Fegan, S.
dc.contributor.authorpl
Feinstein, F.
dc.contributor.authorpl
Fernandes, M. V.
dc.contributor.authorpl
Fernandez, D.
dc.contributor.authorpl
Fiasson, A.
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Fontaine, G.
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Förster, A.
dc.contributor.authorpl
Füßling, M.
dc.contributor.authorpl
Gabici, S.
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Gajdus, M.
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Gallant, Y. A.
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Garrigoux, T.
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Giavitto, G.
dc.contributor.authorpl
Giebels, B.
dc.contributor.authorpl
Glicenstein, J. F.
dc.contributor.authorpl
Gottschall, D.
dc.contributor.authorpl
Grondin, M.-H.
dc.contributor.authorpl
Grudzińska, M.
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Hadasch, D.
dc.contributor.authorpl
Häffner, S.
dc.contributor.authorpl
Hahn, J.
dc.contributor.authorpl
Harris, J.
dc.contributor.authorpl
Heinzelmann, G.
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Henri, G.
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Hermann, G.
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Hervet, O.
dc.contributor.authorpl
Hillert, A.
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Hinton, J. A.
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Hofmann, W.
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Hofverberg, P.
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Holler, M.
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Horns, D.
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Ivascenko, A.
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Jacholkowska, A.
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Jahn, C.
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Jamrozy, Marek - 128434
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Janiak, M.
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Jankowsky, F.
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Jung-Richardt, I.
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Kastendieck, M. A.
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Katarzyński, K.
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Katz, U.
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Kaufmann, S.
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Khélifi, B.
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Kieffer, M.
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Klepser, S.
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Klochkov, D.
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Kluźniak, W.
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Kolitzus, D.
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Komin, Nu.
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Kosack, K.
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Krakau, S.
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Krayzel, F.
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Krüger, P. P.
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Laffon, H.
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Lamanna, G.
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Lefaucheur, J.
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Lefranc, V.
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Lemière, A.
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Lemoine-Goumard, M.
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Lenain, J.-P.
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Lohse, T.
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Lopatin, A.
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Lu, C.-C.
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Marandon, V.
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Marcowith, A.
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Marx, R.
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Maurin, G.
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Maxted, N.
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Mayer, M.
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McComb, T. J. L.
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Méhault, J.
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Meintjes, P. J.
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Menzler, U.
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Meyer, M.
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Mitchell, A. M. W.
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Moderski, R.
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Mohamed, M.
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Morå, K.
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Moulin, E.
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Murach, T.
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de Naurois, M.
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Niemiec, J.
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Nolan, S. J.
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Oakes, L.
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Odaka, H.
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Ohm, S.
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Opitz, B.
dc.contributor.authorpl
Ostrowski, Michał - 100042
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Oya, I.
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Panter, M.
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Parsons, R. D.
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Paz Arribas, M.
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Pekeur, N. W.
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Pelletier, G.
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Petrucci, P.-O.
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Peyaud, B.
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Pita, S.
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Poon, H.
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Pühlhofer, G.
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Punch, M.
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Quirrenbach, A.
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Raab, S.
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Reichardt, I.
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Reimer, A.
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Reimer, O.
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Renaud, M.
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de los Reyes, R.
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Rieger, F.
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Romoli, C.
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Rosier-Lees, S.
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Rowell, G.
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Rudak, B.
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Rulten, C. B.
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Sahakian, V.
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Salek, D.
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Sanchez, D. A.
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Santangelo, A.
dc.contributor.authorpl
Schlickeiser, R.
dc.contributor.authorpl
Schüssler, F.
dc.contributor.authorpl
Schulz, A.
dc.contributor.authorpl
Schwanke, U.
dc.contributor.authorpl
Schwarzburg, S.
dc.contributor.authorpl
Schwemmer, S.
dc.contributor.authorpl
Sol, H.
dc.contributor.authorpl
Spanier, F.
dc.contributor.authorpl
Spengler, G.
dc.contributor.authorpl
Spies, F.
dc.contributor.authorpl
Stawarz, Łukasz - 132081
dc.contributor.authorpl
Steenkamp, R.
dc.contributor.authorpl
Stegmann, C.
dc.contributor.authorpl
Stinzing, F.
dc.contributor.authorpl
Stycz, K.
dc.contributor.authorpl
Sushch, I.
dc.contributor.authorpl
Tavernet, J.-P.
dc.contributor.authorpl
Tavernier, T.
dc.contributor.authorpl
Taylor, A. M.
dc.contributor.authorpl
Terrier, R.
dc.contributor.authorpl
Tluczykont, M.
dc.contributor.authorpl
Trichard, C.
dc.contributor.authorpl
Valerius, K.
dc.contributor.authorpl
van Eldik, C.
dc.contributor.authorpl
van Soelen, B.
dc.contributor.authorpl
Vasileiadis, G.
dc.contributor.authorpl
Veh, J.
dc.contributor.authorpl
Venter, C.
dc.contributor.authorpl
Viana, A.
dc.contributor.authorpl
Vincent, P.
dc.contributor.authorpl
Vink, J.
dc.contributor.authorpl
Völk, H. J.
dc.contributor.authorpl
Volpe, F.
dc.contributor.authorpl
Vorster, M.
dc.contributor.authorpl
Vuillaume, T.
dc.contributor.authorpl
Wagner, S. J.
dc.contributor.authorpl
Wagner, P.
dc.contributor.authorpl
Wagner, R. M.
dc.contributor.authorpl
Ward, M.
dc.contributor.authorpl
Weidinger, M.
dc.contributor.authorpl
Weitzel, Q.
dc.contributor.authorpl
White, R.
dc.contributor.authorpl
Wierzcholska, Alicja - 113652
dc.contributor.authorpl
Willmann, P.
dc.contributor.authorpl
Wörnlein, A.
dc.contributor.authorpl
Wouters, D.
dc.contributor.authorpl
Yang, R.
dc.contributor.authorpl
Zabalza, V.
dc.contributor.authorpl
Zaborov, D.
dc.contributor.authorpl
Zacharias, M.
dc.contributor.authorpl
Zdziarski, A. A.
dc.contributor.authorpl
Zech, A.
dc.contributor.authorpl
Zechlin, H.-S.
dc.contributor.institutionpl
H.E.S.S. Collaboration
dc.date.accessioned
2015-07-13T16:54:00Z
dc.date.available
2015-07-13T16:54:00Z
dc.date.issuedpl
2015
dc.date.openaccess
12
dc.description.accesstime
po opublikowaniu
dc.description.additionalpl
Reproduced with permission from Astronomy & Astrophysics, © ESO
dc.description.admin
[AU] Wierzcholska, Alicja [USOS30589]
dc.description.version
ostateczna wersja wydawcy
dc.description.volumepl
575
dc.identifier.articleidpl
A81
dc.identifier.doipl
10.1051/0004-6361/201424805
dc.identifier.eissnpl
1432-0746
dc.identifier.issnpl
0004-6361
dc.identifier.projectpl
ROD UJ / P
dc.identifier.uri
http://ruj.uj.edu.pl/xmlui/handle/item/12657
dc.languagepl
eng
dc.language.containerpl
eng
dc.rights*
Udzielam licencji. Uznanie autorstwa - Użycie niekomercyjne - Na tych samych warunkach 4.0 Międzynarodowa
dc.rights.licence
OTHER
dc.rights.uri*
http://creativecommons.org/licenses/by-nc-sa/4.0/legalcode.pl
dc.share.type
otwarte czasopismo
dc.subject.enpl
gamma rays: ISM
dc.subject.enpl
ISM: individual objects: Puppis A
dc.subject.enpl
radiation mechanisms: non-thermal
dc.subject.enpl
cosmic rays
dc.subject.enpl
acceleration of particles
dc.subtypepl
Article
dc.titlepl
H.E.S.S. reveals a lack of TeV emission from the supernova remnant Puppis A
dc.title.journalpl
Astronomy & Astrophysics
dc.typepl
JournalArticle
dspace.entity.type
Publication

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