J/A+A/556/A71ivo://CDS.VizieR/J/A+A/556/A71doi:10.26093/cds/vizier.35560071CDSAkyuz A.Thompson D.J.Donato D.Perkins J.S.Fuhrmann L.Angelakis E.,Zensus J.A.Larsson S.Sokolovsky K.Kurtanidze O.2017-06-01T08:52:47Z2015-02-20T14:15:19ZCDS support team

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

cds-question@unistra.frquasarsgamma-ray-astronomyThe observation of gamma-ray flares from blazar 0836+710 in 2011, following a period of quiescence, offered an opportunity to study correlated activity at different wavelengths for a high-redshift (z=2.218) active galactic nucleus. Optical and radio monitoring, plus Fermi-LAT gamma-ray monitoring provided 2008-2012 coverage, while Swift offered auxiliary optical, ultraviolet, and X-ray information. Other contemporaneous observations were used to construct a broad-band spectral energy distribution.2013A&A...556A..71Ahttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/556/A71CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+A/545/A65 : S5 0836+710 image at 1.6GHz (Perucho+, 2012)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/556/A71https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/556/A71http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/556/A71https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/556/A71https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/556/A71http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/556/A71GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapGamma-raydefaultJ/A+A/556/A71/fig1Fermi-LAT light curve for 0836+710 during the quiescent period, MJD 54682-55621 (2008/Aug/4-2011/Mar/01) 7-day time binningrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintMJD[54721/55954] Modified Julian Datedtime.epochdoubleFluxFlux (E>100MeV) (in 10^-7^ph/cm^2^/s)ph.m**-2.ks**-1phot.count;em.gamma.harddoublee_Fluxrms uncertainty on Fluxph.m**-2.ks**-1stat.error;phot.fluxdoubleJ/A+A/556/A71/fig3Fermi-LAT light curve for 0836+710 during the active period, MJD 55621-55957 (2011/Mar/01-2012/Jan/03) 1-day time binningrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintMJD[54721/55954] Modified Julian Datedtime.epochdoubleFluxFlux (E>100MeV) (in 10^-7^ph/cm^2^/s)ph.m**-2.ks**-1phot.count;em.gamma.harddoublee_Fluxrms uncertainty on Fluxph.m**-2.ks**-1stat.error;phot.fluxdoubleJ/A+A/556/A71/fig5Energy spectrum of 0836+710 during the full active period (2011 March through 2012 January)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintE[0.1/12] EnergyGeVem.energyfloatb_E[0.1/10] Lower value of energy intervalGeVphys.energy;stat.minfloatB_E[0.1/15] Upper value of energy intervalGeVphys.energy;stat.maxfloatnuFnuFlux density {nu}F_{nu}_ (erg/cm^2^/s)mW.m**-2phot.flux.density;em.gamma.harddoublee_nuFnurms uncertainty on nuFnumW.m**-2stat.errordoubleJ/A+A/556/A71/fig2Fermi-LAT light curve for 0836+710 during the active period, MJD 55621-55957 (2011/Mar/01-2012/Jan/03) 7-day time binningrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintMJD[54721/55954] Modified Julian Datedtime.epochdoubleFluxFlux (E>100MeV) (in 10^-7^ph/cm^2^/s)ph.m**-2.ks**-1phot.count;em.gamma.harddoublee_Fluxrms uncertainty on Fluxph.m**-2.ks**-1stat.error;phot.fluxdoubleJ/A+A/556/A71/fig6Energy spectrum of 0836+710 during the flarerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintE[0.1/12] EnergyGeVem.energyfloatb_E[0.1/10] Lower value of energy intervalGeVphys.energy;stat.minfloatB_E[0.1/15] Upper value of energy intervalGeVphys.energy;stat.maxfloatnuFnuFlux density {nu}F_{nu}_ (erg/cm^2^/s)mW.m**-2phot.flux.density;em.gamma.harddoublee_nuFnurms uncertainty on nuFnumW.m**-2stat.errordoubleJ/A+A/556/A71/fig4Energy spectrum of 0836+710 during the quiescent periodE[0.1/12] EnergyGeVem.energyfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintb_E[0.1/10] Lower value of energy intervalGeVphys.energy;stat.minfloatB_E[0.1/15] Upper value of energy intervalGeVphys.energy;stat.maxfloatnuFnuFlux density {nu}F_{nu}_ (erg/cm^2^/s)mW.m**-2phot.flux.density;em.gamma.harddoublee_nuFnurms uncertainty on nuFnumW.m**-2stat.errordouble