Limits on X-Ray Polarization at the Core of Centaurus A as Observed with the Imaging X-Ray Polarimetry Explorer

Ehlert, Steven R.Steven R.EhlertFERRAZZOLI, RiccardoRiccardoFERRAZZOLIMarinucci, AndreaAndreaMarinucciMarshall, Herman L.Herman L.MarshallMIDDEI, RiccardoRiccardoMIDDEIPACCIANI, LUIGILUIGIPACCIANIPERRI, MatteoMatteoPERRIPetrucci, Pierre-OlivierPierre-OlivierPetrucciPuccetti, SimonettaSimonettaPuccettiBarnouin, ThibaultThibaultBarnouinBianchi, StefanoStefanoBianchiLiodakis, IoannisIoannisLiodakisMadejski, GrzegorzGrzegorzMadejskiMarin, FrédéricFrédéricMarinMarscher, Alan P.Alan P.MarscherMatt, GiorgioGiorgioMattPoutanen, JuriJuriPoutanenWu, KinwahKinwahWuAgudo, IvánIvánAgudoANTONELLI, Lucio AngeloLucio AngeloANTONELLIBACHETTI, MatteoMatteoBACHETTIBaldini, LucaLucaBaldiniBaumgartner, Wayne H.Wayne H.BaumgartnerBellazzini, RonaldoRonaldoBellazziniBongiorno, Stephen D.Stephen D.BongiornoBonino, RaffaellaRaffaellaBoninoBrez, AlessandroAlessandroBrezBUCCIANTINI, Niccolo'Niccolo'BUCCIANTINICAPITANIO, FIAMMAFIAMMACAPITANIOCastellano, SimoneSimoneCastellanoCavazzuti, ElisabettaElisabettaCavazzutiCiprini, StefanoStefanoCipriniCOSTA, ENRICOENRICOCOSTADE ROSA, AlessandraAlessandraDE ROSADEL MONTE, EttoreEttoreDEL MONTEDi Gesu, LauraLauraDi GesuDi Lalla, NiccolóNiccolóDi LallaDI MARCO, AlessandroAlessandroDI MARCODonnarumma, ImmacolataImmacolataDonnarummaDoroshenko, VictorVictorDoroshenkoDovčiak, MichalMichalDovčiakEnoto, TeruakiTeruakiEnotoEVANGELISTA, YURIYURIEVANGELISTAFABIANI, SergioSergioFABIANIGarcia, Javier A.Javier A.GarciaGunji, ShuichiShuichiGunjiHayashida, KiyoshiKiyoshiHayashidaHeyl, JeremyJeremyHeylIwakiri, WataruWataruIwakiriJorstad, Svetlana G.Svetlana G.JorstadKaras, VladimirVladimirKarasKitaguchi, TakaoTakaoKitaguchiKolodziejczak, Jeffery J.Jeffery J.KolodziejczakKrawczynski, HenricHenricKrawczynskiLA MONACA, FabioFabioLA MONACALatronico, LucaLucaLatronicoMaldera, SimoneSimoneMalderaManfreda, AlbertoAlbertoManfredaMASSARO, FrancescoFrancescoMASSAROMitsuishi, IkuyukiIkuyukiMitsuishiMizuno, TsunefumiTsunefumiMizunoMULERI, FABIOFABIOMULERINegro, MichelaMichelaNegroNg, C. -Y.C. -Y.NgO'Dell, Stephen L.Stephen L.O'DellOmodei, NicolaNicolaOmodeiOppedisano, ChiaraChiaraOppedisanoPAPITTO, ALESSANDROALESSANDROPAPITTOPavlov, George G.George G.PavlovPeirson, Abel L.Abel L.PeirsonPesce-Rollins, MelissaMelissaPesce-RollinsPILIA, MauraMauraPILIAPOSSENTI, ANDREAANDREAPOSSENTIRamsey, Brian D.Brian D.RamseyRANKIN, JohnJohnRANKINRATHEESH, AJAYAJAYRATHEESHRomani, Roger W.Roger W.RomaniSgrò, CarmeloCarmeloSgròSlane, PatrickPatrickSlaneSOFFITTA, PAOLOPAOLOSOFFITTASpandre, GloriaGloriaSpandreTamagawa, ToruToruTamagawaTAVECCHIO, FabrizioFabrizioTAVECCHIOTaverna, RobertoRobertoTavernaTawara, YuzuruYuzuruTawaraTennant, Allyn F.Allyn F.TennantThomas, Nicholas E.Nicholas E.ThomasTOMBESI, FrancescoFrancescoTOMBESITROIS, ALESSIOALESSIOTROISTsygankov, SergeySergeyTsygankovTurolla, RobertoRobertoTurollaVink, JaccoJaccoVinkWeisskopf, Martin C.Martin C.WeisskopfXIE, FEIFEIXIEZane, SilviaSilviaZaneIXPE CollaborationRODI, James CraigJames CraigRODIJourdain, ElisabethElisabethJourdainRoques, Jean-PierreJean-PierreRoques2025-02-282025-02-2820220004-637Xhttp://hdl.handle.net/20.500.12386/36306We present measurements of the polarization of X-rays in the 2-8 keV band from the nucleus of the radio galaxy Centaurus A (Cen A), using a 100 ks observation from the Imaging X-ray Polarimetry Explorer (IXPE). Nearly simultaneous observations of Cen A were also taken with the Swift, NuSTAR, and INTEGRAL observatories. No statistically significant degree of polarization is detected with IXPE. These observations have a minimum detectable polarization at 99% confidence (MDP99) of 6.5% using a weighted, spectral model-independent calculation in the 2-8 keV band. The polarization angle ψ is consequently unconstrained. Spectral fitting across three orders of magnitude in X-ray energy (0.3-400 keV) demonstrates that the SED of Cen A is well described by a simple power law with moderate intrinsic absorption (N H ~ 1023 cm-2) and a Fe Kα emission line, although a second unabsorbed power law is required to account for the observed spectrum at energies below 2 keV. This spectrum suggests that the reprocessing material responsible for this emission line is optically thin and distant from the central black hole. Our upper limits on the X-ray polarization are consistent with the predictions of Compton scattering, although the specific seed photon population responsible for the production of the X-rays cannot be identified. The low polarization degree, variability in the core emission, and the relative lack of variability in the Fe Kα emission line support a picture where electrons are accelerated in a region of highly disordered magnetic fields surrounding the innermost jet....STAMPAenLimits on X-Ray Polarization at the Core of Centaurus A as Observed with the Imaging X-Ray Polarimetry ExplorerArticle10.3847/1538-4357/ac80562-s2.0-85138196662https://api.elsevier.com/content/abstract/scopus_id/85138196662https://iopscience.iop.org/article/10.3847/1538-4357/ac8056FIS/05 - ASTRONOMIA E ASTROFISICAERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation