J/A+A/573/A50ivo://CDS.VizieR/J/A+A/573/A50doi:10.26093/cds/vizier.35730050CDSAleksic J.Ansoldi S.Antonelli L.A.Antoranz P.Babic A.Bangale P.,Barres de Almeida U.Barrio J.A.Becerra Gonzalez J.Bednarek W.,Berger K.Bernardini E.Biland A.Blanch O.Bock R.K.Bonnefoy S.,Bonnoli G.Borracci F.Bretz T.Carmona E.Carosi A.,Carreto Fidalgo D.Collin P.Colombo E.Contreras J.L.Cortina J.,Covino S.Da Vela P.Dazzi F.De Angelis A.De Caneva G.De Lotto B.,Delgado Mendez C.Doert M.Dominguez A.Dominis Prester D.Dorner D.,Doro M.Einecke S.Eisenacher D.Elsaesser D.Farina E.Ferenc D.,Fonseca M.V.Font L.Frantzen K.Fruck C.Garcia Lopez R.J.,Garczarcyk M.Garrido Terrats D.Gaug M.Giavitto G.Godinovic N.,Gonzalez Munoz A.Gozzini S.R.Hadamek A.Hadash D.Herrero A.,Hilderbrand D.Hose J.Hrupec D.Idec W.Kadenius V.Kellermann H.,Knoetig M.L.Krause J.Kushida J.La Barbera A.Lelas D.,Lawandowska N.Linfors E.Lombardi S.Lopez M.Lopez-Coto R.,Lopez-Oramas A.Lorentz E.Lozano I.Makariev M.Mallot K.Maneva G.,Mankuzhiyil N.Mannheim K.Marachi L.Marcote B.Mariotti M.,Marinez M.Mazin D.Menzel U.Meucci M.Miranda J.M.Mirzoyan R.,Moralejo A.Munar-Adrover P.Nakajima D.Niedzwiecki A.Nilsson K.,Nowak N.Orito R.Overkemping A.Paiano S.Palatiello M.Paneque D.,Paoletti R.Parades J.M.Parades-Frotuny X.Partini S.Persic M.,Prada F.Prada Moroni P.G.Prandini E.Preziuso S.Puljak I.,Reinthal R.Rhode W.Ribo M.Rico J.Rodriguez Garcia J.Rugamer S.,Saggion A.Saito T.Saito K.Salvati M.Spanier F.Stamatescu V.,Stamerra A.Steinbring T.Storz J.Sun S.Suric T.Takalo L.,Tavacchio F.Temnikov P.Terzic T.Tescaro D.Teshima M.Thaele J.,Tibolla O.Torres D.F.Toyoma T.Treves A.Uellenbeck M.Vogler P.,Wagner R.M.Zandanel F.Zanin R.(The MAGIC collaboration),Behera B.Beilicke M.Benbow W.Berger K.Bird R.Bouvier A.,Bugaev V.Cerruti M.Chen X.Ciupik L.Collins-Hughes E.Cui W.,Duke C.Dumm J.Falcone A.Federici S.Feng Q.Finley J.P.Fortson L.,Furniss A.Galante N.Gillanders G.H.Griffin S.Griffiths S.T.,Grube J.Gyuk G.Hanna D.Holder J.Johnson C.A.Kaaret P.,Kertzman M.Kieda D.Krawczynski H.Lang M.J.S Madhavan A.Maier G.,Majumdar P.Meagher K.Moriarty P.Mukherjee R.Nieto D.,O'Faolain de Bhroithe A.Ong R.A.Otte A.N.Pichel A.Pohl M.,Popkow A.Prokoph H.Quinn J.Rajotte J.Ratliff G.Reyes L.C.,Reynolds P.T.Richards G.T.Roache E.Sembroski G.H.Shahinyan K.,Sheidaei F.Smith A.W.Staszak D.Telezhinsky I.Theiling M.Tyler J.,Varlotta A.Vincent S.Wakely S.P.Weekes T.C.Welsing R.,Williams D.A.Zajczyk A.Zitzer B.(The VERITAS collaboration),Villata M.Raiteri C.M.Ajello M.Perri M.Aller H.D.Aller M.F.,Larionov V.M.Efimova N.V.Konstantinova T.S.Kopatskaya E.N.Chen W.P.,Koptelova E.Hsiao H.Y.Kurtanidze O.M.Nikolashvili M.G.,Kimeridze G.N.Jordan B.Leto P.Buemi C.S.Trigilio C.Umana G.,Lahteenmaki A.Nieppola E.Tornikoski M.Sainio J.Kadenius V.,Giroletti M.Cesarini A.Fuhrmann L.Kovalev Yu.A.Kovalev Y.Y.2017-06-27T06:38:37Z2014-12-17T08:56:59ZCDS support team

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

cds-question@unistra.fractive-galactic-nucleigamma-ray-astronomyspectral-energy-distributionBlazars are variable sources on various timescales over a broad energy range spanning from radio to very high energy (>100GeV, hereafter VHE). Mrk 501 is one of the brightest blazars at TeV energies and has been extensively studied since its first VHE detection in 1996. However, most of the {gamma}-ray studies performed on Mrk 501 during the past years relate to flaring activity, when the source detection and characterization with the available {gamma}-ray instrumentation was easier to perform. Our goal is to characterize in detail the source {gamma}-ray emission, together with the radio-to-X-ray emission, during the non-flaring (low) activity, which is less often studied than the occasional flaring (high) activity. We organized a multiwavelength (MW) campaign on Mrk 501 between March and May 2008. This multi-instrument effort included the most sensitive VHE {gamma}-ray instruments in the northern hemisphere, namely the imaging atmospheric Cherenkov telescopesMAGIC and VERITAS, as well as Swift, RXTE, the F-GAMMA, GASP-WEBT, and other collaborations and instruments. This provided extensive energy and temporal coverage of Mrk 501 throughout the entire campaign.2015A&A...573A..50Ahttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/573/A50CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+A/495/691 : Multifrequency catalogue of blazars Roma-BZCAT (Massaro+ 2009)J/ApJ/709/1407 : SED of the Fermi blazars (Li+, 2010)J/ApJ/716/30 : SED of Fermi bright blazars (Abdo+, 2010)J/A+A/539/A149 : Multiwavelength view of blazar PKS 2155-304 (Abramowski+ 2012)J/A+A/545/A68 : Optical spectrum of the blazar PKS 0447-439 (Fumagalli+, 2012)J/A+A/559/A75 : 43GHz observation of the blazar Mrk 421 (Blasi+, 2013)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/573/A50https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/573/A50http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/573/A50https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/573/A50https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/573/A50http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/573/A50GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapGamma-raydefaultJ/A+A/573/A50/sed_1Spectral energy distributions for Mrk 501 in the period MJD 54545-54560 (2008-03-20/2008-04-03)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintnu[9.e8/1.e+27] FrequencyHzem.freqdoublenuFnuEnergy Flux (in erg/cm^2^/s)mW.m**-2phot.fluxdoublee_nuFnu1-{sigma} statistical uncertainty in energy flux (in erg/cm^2^/s)mW.m**-2stat.errordoubleJ/A+A/573/A50/sed_2Spectral energy distributions for Mrk 501 in the period MJD 54561-54574 (2008-04-05/2008-04-17)nu[9.e8/1.e+27] FrequencyHzem.freqdoublenuFnuEnergy Flux (in erg/cm^2^/s)mW.m**-2phot.fluxdoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordinte_nuFnu1-{sigma} statistical uncertainty in energy flux (in erg/cm^2^/s)mW.m**-2stat.errordoubleJ/A+A/573/A50/sed_3Spectral energy distributions for Mrk 501 in the period MJD 54579-54604 (2008-04-23/2008-05-19)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintnu[9.e8/1.e+27] FrequencyHzem.freqdoublenuFnuEnergy Flux (in erg/cm^2^/s)mW.m**-2phot.fluxdoublee_nuFnu1-{sigma} statistical uncertainty in energy flux (in erg/cm^2^/s)mW.m**-2stat.errordouble