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Article: Detection of X-Ray Polarization from the Blazar 1ES 1959+650 with the Imaging X-Ray Polarimetry Explorer

TitleDetection of X-Ray Polarization from the Blazar 1ES 1959+650 with the Imaging X-Ray Polarimetry Explorer
Authors
Errando, MLiodakis, IMarscher, APMarshall, HLMiddei, RNegro, MPeirson, ALPerri, MPuccetti, SRabinowitz, PLAgudo, IJorstad, SGSavchenko, SSBlinov, DBourbah, IGKiehlmann, SKontopodis, EMandarakas, NRomanopoulos, SSkalidis, RVervelaki, AAceituno, FJBernardos, MIBonnoli, GCasanova, VAgís-González, BHusillos, CMarchini, ASota, AKouch, PMLindfors, ECasadio, CEscudero, JMyserlis, IImazawa, RSasada, MFukazawa, YKawabata, KSUemura, MMizuno, TNakaoka, TAkitaya, HGurwell, MKeating, GKRao, RIngram, AMassaro, FAntonelli, LABonino, RCavazzuti, EChen, CTCibrario, NCiprini, SDe Rosa, ADi Gesu, LDi Pierro, FDonnarumma, IEhlert, SRFenu, FGau, EKaras, VKim, DEKrawczynski, HLaurenti, MLisalda, LLopez-Coto, RMadejski, GMarin, FMarinucci, AIkuyuki, MMuleri, FPacciani, LPaggi, APetrucci, POCavero, NRRomani, RWTavecchio, FTugliani, SWu, KBachetti, MBaldini, LBaumgartner, WHBellazzini, RBianchi, SBongiorno, SDBrez, ABucciantini, NCapitanio, FCastellano, SCosta, EDel Monte, EDi Lalla, NDi Marco, ADoroshenko, VDovciak, MEnoto, TEvangelista, YFabiani, SFerrazzoli, RGarcia, JAGunji, SHayashida, KHeyl, JIwakiri, WKaaret, PKislat, FKitaguchi, TKolodziejczak, JJLa Monaca, FLatronico, LMaldera, SManfreda, AMatt, GNg, CYO'Dell, SLOmodei, NOppedisano, CPapitto, APavlov, GGPesce-Rollins, MPilia, MPossenti, APoutanen, JRamsey, BDRankin, JRatheesh, ARoberts, OJSgro, CSlane, PSoffitta, PSpandre, GSwartz, DATamagawa, TTaverna, RTawara, YTennant, AFThomas, NETombesi, FTrois, ATsygankov, SSTurolla, RVink, JWeisskopf, MCXie, FZane, S
Issue Date1-Mar-2024
PublisherAmerican Astronomical Society
Citation
Astrophysical Journal, 2024, v. 963, n. 1, p. 1-13 How to Cite?
Abstract

Observations of linear polarization in the 2–8 keV energy range with the Imaging X-ray Polarimetry Explorer (IXPE) explore the magnetic field geometry and dynamics of the regions generating nonthermal radiation in relativistic jets of blazars. These jets, particularly in blazars whose spectral energy distribution peaks at X-ray energies, emit X-rays via synchrotron radiation from high-energy particles within the jet. IXPE observations of the X-ray-selected BL Lac–type blazar 1ES 1959+650 on 2022 May 3–4 showed a significant linear polarization degree of Πx = 8.0% ± 2.3% at an electric-vector position angle ψx = 123° ± 8°. However, on 2022 June 9–12, only an upper limit of Πx ≤ 5.1% could be derived (at the 99% confidence level). The degree of optical polarization at that time, ΠO ∼ 5%, is comparable to the X-ray measurement. We investigate possible scenarios for these findings, including temporal and geometrical depolarization effects. Unlike some other X-ray-selected BL Lac objects, there is no significant chromatic dependence of the measured polarization in 1ES 1959+650, and its low X-ray polarization may be attributed to turbulence in the jet flow with dynamical timescales shorter than 1 day.


Persistent Identifierhttp://hdl.handle.net/10722/342799
ISSN
2023 Impact Factor: 4.8
2023 SCImago Journal Rankings: 1.905
ISI Accession Number ID

 

DC FieldValueLanguage
dc.contributor.authorErrando, M-
dc.contributor.authorLiodakis, I-
dc.contributor.authorMarscher, AP-
dc.contributor.authorMarshall, HL-
dc.contributor.authorMiddei, R-
dc.contributor.authorNegro, M-
dc.contributor.authorPeirson, AL-
dc.contributor.authorPerri, M-
dc.contributor.authorPuccetti, S-
dc.contributor.authorRabinowitz, PL-
dc.contributor.authorAgudo, I-
dc.contributor.authorJorstad, SG-
dc.contributor.authorSavchenko, SS-
dc.contributor.authorBlinov, D-
dc.contributor.authorBourbah, IG-
dc.contributor.authorKiehlmann, S-
dc.contributor.authorKontopodis, E-
dc.contributor.authorMandarakas, N-
dc.contributor.authorRomanopoulos, S-
dc.contributor.authorSkalidis, R-
dc.contributor.authorVervelaki, A-
dc.contributor.authorAceituno, FJ-
dc.contributor.authorBernardos, MI-
dc.contributor.authorBonnoli, G-
dc.contributor.authorCasanova, V-
dc.contributor.authorAgís-González, B-
dc.contributor.authorHusillos, C-
dc.contributor.authorMarchini, A-
dc.contributor.authorSota, A-
dc.contributor.authorKouch, PM-
dc.contributor.authorLindfors, E-
dc.contributor.authorCasadio, C-
dc.contributor.authorEscudero, J-
dc.contributor.authorMyserlis, I-
dc.contributor.authorImazawa, R-
dc.contributor.authorSasada, M-
dc.contributor.authorFukazawa, Y-
dc.contributor.authorKawabata, KS-
dc.contributor.authorUemura, M-
dc.contributor.authorMizuno, T-
dc.contributor.authorNakaoka, T-
dc.contributor.authorAkitaya, H-
dc.contributor.authorGurwell, M-
dc.contributor.authorKeating, GK-
dc.contributor.authorRao, R-
dc.contributor.authorIngram, A-
dc.contributor.authorMassaro, F-
dc.contributor.authorAntonelli, LA-
dc.contributor.authorBonino, R-
dc.contributor.authorCavazzuti, E-
dc.contributor.authorChen, CT-
dc.contributor.authorCibrario, N-
dc.contributor.authorCiprini, S-
dc.contributor.authorDe Rosa, A-
dc.contributor.authorDi Gesu, L-
dc.contributor.authorDi Pierro, F-
dc.contributor.authorDonnarumma, I-
dc.contributor.authorEhlert, SR-
dc.contributor.authorFenu, F-
dc.contributor.authorGau, E-
dc.contributor.authorKaras, V-
dc.contributor.authorKim, DE-
dc.contributor.authorKrawczynski, H-
dc.contributor.authorLaurenti, M-
dc.contributor.authorLisalda, L-
dc.contributor.authorLopez-Coto, R-
dc.contributor.authorMadejski, G-
dc.contributor.authorMarin, F-
dc.contributor.authorMarinucci, A-
dc.contributor.authorIkuyuki, M-
dc.contributor.authorMuleri, F-
dc.contributor.authorPacciani, L-
dc.contributor.authorPaggi, A-
dc.contributor.authorPetrucci, PO-
dc.contributor.authorCavero, NR-
dc.contributor.authorRomani, RW-
dc.contributor.authorTavecchio, F-
dc.contributor.authorTugliani, S-
dc.contributor.authorWu, K-
dc.contributor.authorBachetti, M-
dc.contributor.authorBaldini, L-
dc.contributor.authorBaumgartner, WH-
dc.contributor.authorBellazzini, R-
dc.contributor.authorBianchi, S-
dc.contributor.authorBongiorno, SD-
dc.contributor.authorBrez, A-
dc.contributor.authorBucciantini, N-
dc.contributor.authorCapitanio, F-
dc.contributor.authorCastellano, S-
dc.contributor.authorCosta, E-
dc.contributor.authorDel Monte, E-
dc.contributor.authorDi Lalla, N-
dc.contributor.authorDi Marco, A-
dc.contributor.authorDoroshenko, V-
dc.contributor.authorDovciak, M-
dc.contributor.authorEnoto, T-
dc.contributor.authorEvangelista, Y-
dc.contributor.authorFabiani, S-
dc.contributor.authorFerrazzoli, R-
dc.contributor.authorGarcia, JA-
dc.contributor.authorGunji, S-
dc.contributor.authorHayashida, K-
dc.contributor.authorHeyl, J-
dc.contributor.authorIwakiri, W-
dc.contributor.authorKaaret, P-
dc.contributor.authorKislat, F-
dc.contributor.authorKitaguchi, T-
dc.contributor.authorKolodziejczak, JJ-
dc.contributor.authorLa Monaca, F-
dc.contributor.authorLatronico, L-
dc.contributor.authorMaldera, S-
dc.contributor.authorManfreda, A-
dc.contributor.authorMatt, G-
dc.contributor.authorNg, CY-
dc.contributor.authorO'Dell, SL-
dc.contributor.authorOmodei, N-
dc.contributor.authorOppedisano, C-
dc.contributor.authorPapitto, A-
dc.contributor.authorPavlov, GG-
dc.contributor.authorPesce-Rollins, M-
dc.contributor.authorPilia, M-
dc.contributor.authorPossenti, A-
dc.contributor.authorPoutanen, J-
dc.contributor.authorRamsey, BD-
dc.contributor.authorRankin, J-
dc.contributor.authorRatheesh, A-
dc.contributor.authorRoberts, OJ-
dc.contributor.authorSgro, C-
dc.contributor.authorSlane, P-
dc.contributor.authorSoffitta, P-
dc.contributor.authorSpandre, G-
dc.contributor.authorSwartz, DA-
dc.contributor.authorTamagawa, T-
dc.contributor.authorTaverna, R-
dc.contributor.authorTawara, Y-
dc.contributor.authorTennant, AF-
dc.contributor.authorThomas, NE-
dc.contributor.authorTombesi, F-
dc.contributor.authorTrois, A-
dc.contributor.authorTsygankov, SS-
dc.contributor.authorTurolla, R-
dc.contributor.authorVink, J-
dc.contributor.authorWeisskopf, MC-
dc.contributor.authorXie, F-
dc.contributor.authorZane, S-
dc.date.accessioned2024-04-24T02:47:15Z-
dc.date.available2024-04-24T02:47:15Z-
dc.date.issued2024-03-01-
dc.identifier.citationAstrophysical Journal, 2024, v. 963, n. 1, p. 1-13-
dc.identifier.issn0004-637X-
dc.identifier.urihttp://hdl.handle.net/10722/342799-
dc.description.abstract<p>Observations of linear polarization in the 2–8 keV energy range with the Imaging X-ray Polarimetry Explorer (IXPE) explore the magnetic field geometry and dynamics of the regions generating nonthermal radiation in relativistic jets of blazars. These jets, particularly in blazars whose spectral energy distribution peaks at X-ray energies, emit X-rays via synchrotron radiation from high-energy particles within the jet. IXPE observations of the X-ray-selected BL Lac–type blazar 1ES 1959+650 on 2022 May 3–4 showed a significant linear polarization degree of Π<sub>x</sub> = 8.0% ± 2.3% at an electric-vector position angle <em>ψ</em><sub>x</sub> = 123° ± 8°. However, on 2022 June 9–12, only an upper limit of Π<sub>x</sub> ≤ 5.1% could be derived (at the 99% confidence level). The degree of optical polarization at that time, Π<sub>O</sub> ∼ 5%, is comparable to the X-ray measurement. We investigate possible scenarios for these findings, including temporal and geometrical depolarization effects. Unlike some other X-ray-selected BL Lac objects, there is no significant chromatic dependence of the measured polarization in 1ES 1959+650, and its low X-ray polarization may be attributed to turbulence in the jet flow with dynamical timescales shorter than 1 day.<br></p>-
dc.languageeng-
dc.publisherAmerican Astronomical Society-
dc.relation.ispartofAstrophysical Journal-
dc.rightsThis work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.-
dc.titleDetection of X-Ray Polarization from the Blazar 1ES 1959+650 with the Imaging X-Ray Polarimetry Explorer-
dc.typeArticle-
dc.identifier.doi10.3847/1538-4357/ad1ce4-
dc.identifier.scopuseid_2-s2.0-85185917858-
dc.identifier.volume963-
dc.identifier.issue1-
dc.identifier.spage1-
dc.identifier.epage13-
dc.identifier.eissn1538-4357-
dc.identifier.isiWOS:001183282000001-
dc.identifier.issnl0004-637X-

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