학술논문

X-ray Polarization of the BL Lac Type Blazar 1ES 0229+200
Document Type
Working Paper
Author
Ehlert, Steven R.Liodakis, IoannisMiddei, RiccardoMarscher, Alan P.Tavecchio, FabrizioAgudo, IvánKouch, Pouya M.Lindfors, ElinaNilsson, KariMyserlis, IoannisGurwell, MarkRao, RamprasadAceituno, Francisco JoseBonnoli, GiacomoCasanova, VictorAgiz-Gonzalez, BeatrizEscudero, JuanSantos, Jorge OteroSota, AlfredoAngelakis, EmmanouilKraus, AlexanderKeating, Garrett K.Antonelli, Lucio A.Bachetti, MatteoBaldini, LucaBaumgartner, Wayne H.Bellazzini, RonaldoBianchi, StefanoBongiorno, Stephen D.Bonino, RaffaellaBrez, AlessandroBucciantini, NiccolòCapitanio, FiammaCastellano, SimoneCavazzuti, ElisabettaChen, Chien-TingCiprini, StefanoCosta, EnricoDe Rosa, AlessandraDel Monte, EttoreDi Gesu, LauraDi Lalla, NiccolòDi Marco, AlessandroDonnarumma, ImmacolataDoroshenko, VictorDovčiak, MichalEnoto, TeruakiEvangelista, YuriFabiani, SergioFerrazzoli, RiccardoGarcia, Javier A.Gunji, ShuichiHayashida, KiyoshiHeyl, JeremyIwakiri, WataruJorstad, Svetlana G.Kaaret, PhilipKaras, VladimirKislat, FabianKitaguchi, TakaoKolodziejczak, Jeffery J.Krawczynski, HenricLa Monaca, FabioLatronico, LucaMaldera, SimoneManfreda, AlbertoMarin, FrédéricMarinucci, AndreaMarshall, Herman L.Massaro, FrancescoMatt, GiorgioMitsuishi, IkuyukiMizuno, TsunefumiMuleri, FabioNegro, MichelaNg, C. -Y.O'Dell, Stephen L.Omodei, NicolaOppedisano, ChiaraPapitto, AlessandroPavlov, George G.Peirson, Abel L.Perri, MatteoPesce-Rollins, MelissaPetrucci, Pierre-OlivierPilia, MauraPossenti, AndreaPoutanen, JuriPuccetti, SimonettaRamsey, Brian D.Rankin, JohnRatheesh, AjayRoberts, Oliver J.Romani, Roger W.Sgro, CarmeloSlane, PatrickSoffitta, PaoloSpandre, GloriaSwartz, Douglas A.Tamagawa, ToruTaverna, RobertoTawara, YuzuruTennant, Allyn F.Thomas, Nicholas E.Tombesi, FrancescoTrois, AlessioTsygankov, Sergey S.Turolla, RobertoVink, JaccoWeisskopf, Martin C.Wu, KinwahXie, FeiZane, Silvia
Source
Subject
Astrophysics - High Energy Astrophysical Phenomena
Language
Abstract
We present polarization measurements in the $2-8 \thinspace \mathrm{keV}$ band from blazar 1ES 0229+200, the first extreme high synchrotron peaked source to be observed by the Imaging X-ray Polarimetry Explorer (IXPE). Combining two exposures separated by about two weeks, we find the degree of polarization to be $\Pi_{X} = 17.9 \pm 2.8 \%$ at an electric-vector position angle $\psi_X = 25.0 \pm 4.6^{\circ}$ using a spectropolarimetric fit from joint IXPE and XMM-Newton observations. There is no evidence for the polarization degree or angle varying significantly with energy or time on both short time scales (hours) or longer time scales (days). The contemporaneous polarization degree at optical wavelengths was $>$7$\times$ lower, making 1ES 0229+200 the most strongly chromatic blazar yet observed. This high X-ray polarization compared to the optical provides further support that X-ray emission in high-peaked blazars originates in shock-accelerated, energy-stratified electron populations, but is in tension with many recent modeling efforts attempting to reproduce the spectral energy distribution of 1ES 0229+200 which attribute the extremely high energy synchrotron and Compton peaks to Fermi acceleration in the vicinity of strongly turbulent magnetic fields.
Comment: 17 Pages, 6 Figures, Resubmitted to ApJ after addressing referee comments