J/A+A/542/A94ivo://CDS.VizieR/J/A+A/542/A94doi:10.26093/cds/vizier.35420094CDSH.E.S.S. CollaborationAbramowski A.Acero F.Aharonian F.,Akhperjanian A.G.Anton G.Balzer A.Barnacka A.Becherini Y.,Becker J.Bernlohr K.Birsin E.Biteau J.Bochow A.Boisson C.,Bolmont J.Bordas P.Brucker J.Brun F.Brun P.Bulik T.Busching I.,Carrigan S.Casanova S.P.M. ChadwickCharbonnier A.Chaves R.C.G.,Cheesebrough A.Cologna G.Conrad J.Cerruti M.Dalton M.Daniel M.K.,Davids I.D.Degrange B.Deil C.Dickinson H.J.Djannati-Atai A.,Domainko W.Drury L.O'C.Dubus G.Dutson K.Dyks J.Dyrda M.,Egberts K.Eger P.Espigat P.Fallon L.Fegan S.Feinstein F.,Fernandes M.V.Fiasson A.Fontaine G.Forster A.Fussling M.Gast H.,Gerard L.Gerbig D.Giebels B.Glicenstein J.F.Gluck B.Goring D.,Haffner S.Gallant Y.A.Hague J.D.Hahn J.Hampf D.Harris J.,Hauser M.Heinz S.Heinzelmann G.Henri G.Hermann G.Hillert A.,Hinton J.A.Hofmann W.Hofverberg P.Holler M.Horns D.,Jacholkowska A.de Jager O.C.Jahn C.Jamrozy M.Jung I.,Kastendieck M.A.Katarzynski K.Katz U.Kaufmann S.Keogh D.,Klochkov D.Kluzniak W.Kneiske T.Komin Nu.Kosack K.Kossakowski R.,Krayzel F.Khelifi B.Laffon H.Lamanna G.Lenain J.-P.Lennarz D.,Lohse T.Lopatin A.Lu C.-C.Marandon V.Marcowith A.Masbou J.,Maxted N.Mayer M.McComb T.J.L.Medina M.C.Mehault J.Moderski R.,Mohamed M.Moulin E.Naumann C.L.Naumann-Godo M.de Naurois M.,Nedbal D.Nekrassov D.Nguyen N.Nicholas B.Niemiec J.Nolan S.J.,Ohm S.de Ona Wilhelmi E.Opitz B.Ostrowski M.Panter M.,Paz Arribas M.Pekeur N.W.Pelletier G.Perez J.Petrucci P.-O.,Peyaud B.Pita S.Oya I.Puhlhofer G.Punch M.Quirrenbach A.Raue M.,Rayner S.M.Reimer A.Reimer O.Renaud M.de los Reyes R.Rieger F.,Ripken J.Rob L.Rosier-Lees S.Rowell G.Rudak B.Rulten C.B.,Sahakian V.Sanchez D.A.Santangelo A.Schlickeiser R.Schulz A.,Schwanke U.Schwarzburg S.Schwemmer S.Sheidaei F.Skilton J.L.,Sol H.Spengler G.Stawarz L.Steenkamp R.Stegmann C.Stinzing F.,Stycz K.Sushch I.Szostek A.Tavernet J.-P.Terrier R.,Tluczykont M.Valerius K.van Eldik C.Vasileiadis G.Venter C.,Viana A.Vincent P.Volk H.J.Volpe F.Vorobiov S.Vorster M.,Wagner S.J.Ward M.White R.Wierzcholska A.Zacharias M.Zajczyk A.,Zdziarski A.A.Zech A.Zechlin H.-S.2017-07-03T14:26:58Z2012-06-14T08:13:36ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.fractive-galactic-nucleibl-lacertae-objectsgamma-ray-astronomy1RXS J101015.9-311909 is a galaxy located at a redshift of z=0.14 hosting an active nucleus (called AGN) belonging to the class of bright BL Lac objects. Observations at high (HE, E>100MeV) and very high (VHE, E>100GeV) energies provide insights into the origin of very energetic particles present in such sources and the radiation processes at work. We report on results from VHE observations performed between 2006 and 2010 with the H.E.S.S. instrument, an array of four imaging atmospheric Cherenkov telescopes. H.E.S.S. data have been analysed with enhanced analysis methods, making the detection of faint sources more significant.2012A&A...542A..94Hhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/542/A94CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/542/A94https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/542/A94http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/542/A94https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/542/A94https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/542/A94http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/542/A94GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapGamma-raydefaultJ/A+A/542/A94/hessspH.E.S.S. spectral points (Fig. 4 left)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintEEnergy in TeVTeVphys.energydoubledNdETime-averaged differential H.E.S.S. spectrumcm**-2.s**-1.TeV**-1phot.flux.density;em.gamma.harddoublee_dNdENegative error on the time-averaged differential H.E.S.S. spectrumcm**-2.s**-1.TeV**-1stat.errordoubleE_dNdEPositive error on the time-averaged differential H.E.S.S. spectrumcm**-2.s**-1.TeV**-1stat.error;stat.maxdoubleJ/A+A/542/A94/fermispFermi spectral points (Fig. 7)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintEEnergy in MeVMeVphys.energydoublee_ENegative error on energy in MeVMeVstat.errordoubleE_EPositive error on energy in MeVMeVstat.error;stat.maxdoublenuFnuTime-averaged differential VHE gamma-ray spectrummW.m**-2phot.flux.density;em.gamma.harddoublee_nuFnuNegative error on the time-averaged differential Fermi/LAT spectrummW.m**-2stat.errordoubleE_nuFnuPositive error on the time-averaged differential Fermi/LAT spectrummW.m**-2stat.error;stat.maxdoubleJ/A+A/542/A94/swiftcaSwift/XRT spectrum (Fig. 6, case A)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintEEnergy in MeVMeVphys.energydoublee_ENegative error on energy in MeVMeVstat.errorfloatE_EPositive error on energy in MeVMeVstat.error;stat.maxfloatnuFnuTime-averaged differential Swift/XRT spectrummW.m**-2phot.flux.density;em.gamma.harddoublee_nuFnuNegative error on the time-averaged differential Swift/XRT spectrummW.m**-2stat.errordoubleE_nuFnuPositive error on the time-averaged differential Swift/XRT spectrummW.m**-2stat.error;stat.maxdoubleJ/A+A/542/A94/swiftcbSwift/XRT spectrum (Fig. 6, case B)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintEEnergy in MeVMeVphys.energydoublee_ENegative error on energy in MeVMeVstat.errorfloatE_EPositive error on energy in MeVMeVstat.error;stat.maxfloatnuFnuTime-averaged differential Swift/XRT spectrummW.m**-2phot.flux.density;em.gamma.harddoublee_nuFnuNegative error on the time-averaged differential Swift/XRT spectrummW.m**-2stat.errordoubleE_nuFnuPositive error on the time-averaged differential Swift/XRT spectrummW.m**-2stat.error;stat.maxdoubleJ/A+A/542/A94/hesslcH.E.S.S. light curve (Fig. 5 upper panel)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintMJDModified Julian Datedtime.epochdoubleFluxFlux above E>0.2TeV1e-12cm**-2.s**-1phot.flux.density;em.gamma.harddoublee_FluxError on given flux1e-12cm**-2.s**-1stat.error;phot.fluxdoubleFluxUp? Upper limit on flux (if flux negative)1e-12cm**-2.s**-1phot.flux.density;em.gamma.harddoublenullableJ/A+A/542/A94/fermilc1Fermi/LAT light curve for E>300MeV (Fig.5 middle panel)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintMJDModified Julian Datedtime.epochfloatFluxFlux above E>300MeV1e-09cm**-2.s**-1phot.flux.density;em.gamma.harddoublee_FluxError on given flux1e-09cm**-2.s**-1stat.error;phot.fluxdoubleJ/A+A/542/A94/fermilc2Fermi/LAT light curve for E>1GeV (Fig.5 middle panel)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintMJDModified Julian Datedtime.epochfloatFluxFlux above E>300MeV1e-09cm**-2.s**-1phot.flux.density;em.gamma.harddoublee_FluxError on given flux1e-09cm**-2.s**-1stat.error;phot.fluxdoubleJ/A+A/542/A94/atomlc1ATOM B-band (Fig. 5 bottom panel)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintMJDModified Julian Datedtime.epochdoubleFluxATOM flux (in R filter for atomlc1, B filter for atomlc2) filter (1)1e-17W.m**-2.nm**-1phot.flux.density;em.gamma.harddoublee_FluxATOM error on the given flux (1)1e-17W.m**-2.nm**-1stat.error;phot.fluxdoubleJ/A+A/542/A94/atomlc2ATOM R-band (Fig. 5 bottom panel)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintMJDModified Julian Datedtime.epochdoubleFluxATOM flux (in R filter for atomlc1, B filter for atomlc2) filter (1)1e-17W.m**-2.nm**-1phot.flux.density;em.gamma.harddoublee_FluxATOM error on the given flux (1)1e-17W.m**-2.nm**-1stat.error;phot.fluxdouble