J/A+A/576/A126ivo://CDS.VizieR/J/A+A/576/A126doi:10.26093/cds/vizier.35760126CDSAleksic 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.Colin 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.,Garczarczyk M.Garrido Terrats D.Gaug M.Giavitto G.Godinovi N.,Gonzalez Munoz A.Gozzini S.R.Hadamek A.Hadasch D.Herrero A.,Hildebrand D.Hose J.Hrupec D.Idec W.Kadenius V.Kellermann H.,Knoetig M.L.Krause J.Kushida J.La Barbera A.Lelas D.,Lewandowska N.Lindfors E.Longo F.Lombardi S.Lopez M.,Lopez-Coto R.Lopez-Oramas A.Lorenz E.Lozano I.Makariev M.,Mallot K.Maneva G.Mankuzhiyil N.Mannheim K.Maraschi L.,Marcote B.Mariotti M.Martinez 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.Paredes J.M.Paredes-Fortuny 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 K.Salvati M.,Satalecka K.Scalzotto V.Scapin V.Schultz C.Schweizer T.,Shore S.N.Sillanpaa A.Sitarek J.Snidaric I.Sobczynska D.,Spanier F.Stamatescu V.Stamerra A.Steinbring T.Storz J.Sun S.,Suri T.Takalo L.Tavecchio F.Temnikov P.Terzi T.Tescaro D.,Teshima M.Thaele J.Tibolla O.Torres D.F.Toyama T.Treves A.,Uellenbeck M.Vogler P.Wagner R.M.Zandanel F.Zanin R.,(The MAGIC collaboration)Archambault S.Behera B.Beilicke M.,Benbow W.Bird R.Buckley J.H.Bugaev V.Cerruti M.Chen X.,Ciupik L.Collins-Hughes E.Cui W.Dumm J.Eisch J.D.Falcone A.,Federici S.Feng Q.Finley J.P.Fleischhack H.Fortin P.Fortson L.,Furniss A.Griffin S.Griffiths S.T.Grube J.Gyuk G.Hanna D.,Holder J.Hughes G.Humensky T.B.Johnson C.A.Kaaret P.Kertzman M.,Khassen Y.Kieda D.Krawczynski H.Krennrich F.Kumar S.Lang M.J.,Maier G.McArthur S.Meagher K.Moriarty P.Mukherjee R.Ong R.A.,Otte A.N.Park N.Pichel A.Pohl M.Popkow A.Prokoph H.Quinn J.,Ragan K.Rajotte J.Reynolds P.T.Richards G.T.Roache E.Rovero A.C.,Sembroski G.H.Shahinyan K.Staszak D.Telezhinsky I.Theiling M.,Tucci J.V.Tyler J.Varlotta A.Wakely S.P.Weekes T.C.Weinstein A.,Welsing R.Wilhelm A.Williams D.A.Zitzer B.,(The VERITAS collaboration)Villata M.Raiteri C.Aller H.D.,Aller M.F.Chen W.P.Jordan B.Koptelova E.Kurtanidze O.M.,Lahteenmaki A.McBreen B.Larionov V.M.Lin C.S.Nikolashvili M.G.,Angelakis E.Capalbi M.Carraminana A.Carrasco L.Cassaro P.,Cesarini A.Fuhrmann L.Giroletti M.Hovatta T.Krichbaum T.P.,Krimm H.A.Max-Moerbeck W.Moody J.W.Maccaferri G.Mori Y.,Nestoras I.Orlati A.Pace C.Pearson R.Perri M.Readhead A.C.S.,Richards J.L.Sadun A.C.Sakamoto T.Tammi J.Tornikoski M.Yatsu Y.,Zook A.2015-08-10T16:27:04Z2015-04-17T08:19:19ZCDS support team

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

cds-question@unistra.frbl-lacertae-objectsmarkarian-galaxiesWe perform an extensive characterization of the broadband emission of Mrk 421, as well as its temporal evolution, during the non-flaring (low) state. The high brightness and nearby location (z=0.031) of Mrk 421 make it an excellent laboratory to study blazar emission. The goal is to learn about the physical processes responsible for the typical emission of Mrk 421, which might also be extended to other blazars that are located farther away and hence are more difficult to study. We performed a 4.5-month multi-instrument campaign on Mrk 421 between January 2009 and June 2009, which included VLBA, F- GAMMA, GASP-WEBT, Swift, RXTE, Fermi-LAT, MAGIC, and Whipple, among other instruments and collaborations. This extensive radio to very-high-energy (VHE; E>100GeV) gamma-ray dataset provides excellent temporal and energy coverage, which allows detailed studies of the evolution of the broadband spectral energy distribution.2015A&A...576A.126Ahttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/576/A126CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+A/545/A117 : Monitoring of Mrk 421 at 15 and 24GHz (Lico+, 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/576/A126https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/576/A126http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/576/A126https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/576/A126https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/576/A126http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/576/A126GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/A+A/576/A126/table1Lightcurves of Mrk 421 from radio to VHE from MJD54850 (2009-01-09) to MJD54983 (2009-06-01)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintInstInstrumentmeta.id;instrcharBandBand / energy rangeinstr.bandpasscharbFreqband frequency, lower boundaryHzem.freq;stat.mindoubleBFreqband frequency, upper boundaryHzem.freq;stat.maxdoubleMJDStModified Julian Date, observation (time bin) startdtime.epochdoubleMJDEndModified Julian Date, observation (time bin) enddtime.epochdoublex_FluxFlux unitmeta.unit;phot.fluxcharFluxFluxphot.count;em.optdoublee_FluxFlux errorstat.error;phot.fluxdoubleHFlux? Host galaxy flux (1)phot.count;em.optdoublenullablee_HFlux? Host galaxy flux error (1)stat.errordoublenullable