The X-ray polarization of the Seyfert 1 galaxy IC 4329A

Author:

Ingram A1ORCID,Ewing M1,Marinucci A2ORCID,Tagliacozzo D3ORCID,Rosario D J1,Veledina A45ORCID,Kim D E678ORCID,Marin F9ORCID,Bianchi S3ORCID,Poutanen J4ORCID,Matt G3,Marshall H L10,Ursini F3ORCID,De Rosa A6ORCID,Petrucci P-O11,Madejski G12,Barnouin T9,Gesu L Di2,Dovčiak M13ORCID,Gianolli V E311ORCID,Krawczynski H14,Loktev V4ORCID,Middei R615ORCID,Podgorny J91316ORCID,Puccetti S15,Ratheesh A6,Soffitta P6,Tombesi F81718,Ehlert S R19ORCID,Massaro F2021,Agudo I22,Antonelli L A1523ORCID,Bachetti M24ORCID,Baldini L2526,Baumgartner W H19,Bellazzini R25,Bongiorno S D19,Bonino R2021ORCID,Brez A25,Bucciantini N272829,Capitanio F6,Castellano S25,Cavazzuti E2,Chen C-T30ORCID,Ciprini S1517,Costa E6,Del Monte E6,Lalla N Di12,Marco A Di6ORCID,Donnarumma I2,Doroshenko V31ORCID,Enoto T32,Evangelista Y6,Fabiani S6,Ferrazzoli R6,García J A33,Gunji S34ORCID,Heyl J35ORCID,Iwakiri W36,Jorstad S G3738ORCID,Kaaret P19,Karas V13,Kislat F39,Kitaguchi T32,Kolodziejczak J J19,Monaca F La6ORCID,Latronico L20,Liodakis I40ORCID,Maldera S20,Manfreda A41,Marscher A P37,Mitsuishi I42,Mizuno T43,Muleri F6,Negro M444546,Ng C-Y47,O’Dell S L19,Omodei N12,Oppedisano C20,Papitto A23,Pavlov G G48,Peirson A L12,Perri M1523,Pesce-Rollins M25,Pilia M24,Possenti A24,Ramsey B D19,Rankin J6,Roberts O J30,Romani R W12,Sgrò C25,Slane P49,Spandre G25,Swartz D A30,Tamagawa T32,Tavecchio F50,Taverna R51,Tawara Y42,Tennant A F19,Thomas N E19,Trois A24ORCID,Tsygankov S S4,Turolla R5152,Vink J53ORCID,Weisskopf M C19,Wu K52ORCID,Xie F546,Zane S52

Affiliation:

1. School of Mathematics, Statistics, and Physics, Newcastle University , Newcastle upon Tyne NE1 7RU , UK

2. ASI – Agenzia Spaziale Italiana , Via del Politecnico Snc, I-00133 Roma , Italy

3. Dipartimento di Matematica e Fisica, Università degli Studi Roma Tre , Via della Vasca Navale 84, I-00146 Roma , Italy

4. Department of Physics and Astronomy , University of Turku, FI-20014 Turku , Finland

5. Nordita, KTH Royal Institute of Technology and Stockholm University , Hannes Alfvéns väg 12, SE-10691 Stockholm , Sweden

6. INAF Istituto di Astrofisica e Planetologia Spaziali , Via del Fosso del Cavaliere 100, I-00133 Roma , Italy

7. Dipartimento di Fisica, Università degli Studi di Roma ‘La Sapienza’ , Piazzale Aldo Moro 5, I-00185 Roma , Italy

8. Dipartimento di Fisica, Università degli Studi di Roma ‘Tor Vergata’ , Via della Ricerca Scientifica 1, I-00133 Roma , Italy

9. Université de Strasbourg, CNRS, Observatoire Astronomique de Strasbourg , UMR 7550, F-67000 Strasbourg , France

10. MIT Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology , 77 Massachusetts Avenue, Cambridge, MA 02139 , USA

11. Université Grenoble Alpes, CNRS, IPAG , F-38000 Grenoble , France

12. Department of Physics and Kavli Institute for Particle Astrophysics and Cosmology, Stanford University , Stanford, CA 94305 , USA

13. Astronomical Institute of the Czech Academy of Sciences , Boční II 1401/1, CZ-14100 Praha 4 , Czech Republic

14. Physics Department and McDonnell Center for the Space Sciences, Washington University , St Louis, MO 63130 , USA

15. Space Science Data Center, Agenzia Spaziale Italiana , Via del Politecnico Snc, I-00133 Roma , Italy

16. Astronomical Institute, Charles University , V Holešovičkách 2, CZ-18000 Prague , Czech Republic

17. Istituto Nazionale di Fisica Nucleare, Sezione di Roma ‘Tor Vergata’ , Via della Ricerca Scientifica 1, I-00133 Roma , Italy

18. Department of Astronomy, University of Maryland , College Park, Maryland 20742 , USA

19. NASA Marshall Space Flight Center , Huntsville, AL 35812 , USA

20. Istituto Nazionale di Fisica Nucleare , Sezione di Torino, Via Pietro Giuria 1, I-10125 Torino , Italy

21. Dipartimento di Fisica, Università degli Studi di Torino , Via Pietro Giuria 1, I-10125 Torino , Italy

22. Instituto de Astrofísica de Andalucía’CSIC , Glorieta de la Astronomía s/n, E-18008 Granada , Spain

23. INAF Osservatorio Astronomico di Roma , Via Frascati 33, I-00078 Monte Porzio Catone (RM) , Italy

24. INAF Osservatorio Astronomico di Cagliari , Via della Scienza 5, I-09047 Selargius (CA) , Italy

25. Istituto Nazionale di Fisica Nucleare , Sezione di Pisa, Largo B. Pontecorvo 3, I-56127 Pisa , Italy

26. Dipartimento di Fisica, Università di Pisa , Largo B. Pontecorvo 3, I-56127 Pisa , Italy

27. INAF Osservatorio Astrofisico di Arcetri , Largo Enrico Fermi 5, I-50125 Firenze , Italy

28. Dipartimento di Fisica e Astronomia, Università degli Studi di Firenze , Via Sansone 1, I-50019 Sesto Fiorentino (FI) , Italy

29. Istituto Nazionale di Fisica Nucleare , Sezione di Firenze, Via Sansone 1, I-50019 Sesto Fiorentino (FI) , Italy

30. Science and Technology Institute, Universities Space Research Association , Huntsville, AL 35805 , USA

31. Institut für Astronomie und Astrophysik, Universität Tübingen , Sand 1, I-72076 Tübingen , Germany

32. RIKEN Cluster for Pioneering Research , 2-1 Hirosawa, Wako, Saitama 351-0198 , Japan

33. California Institute of Technology , Pasadena, CA 91125 , USA

34. Yamagata University , 1-4-12 Kojirakawamachi, Yamagatashi 990-8560 , Japan

35. University of British Columbia , Vancouver, BC V6T 1Z4 , Canada

36. International Center for Hadron Astrophysics, Chiba University , Chiba 263-8522 , Japan

37. Institute for Astrophysical Research, Boston University , 725 Commonwealth Avenue, Boston, MA 02215 , USA

38. Department of Astrophysics, St Petersburg State University , Uni-versitetsky pr. 28, Petrodvoretz, 198504 St Petersburg , Russia

39. Department of Physics and Astronomy and Space Science Center, University of New Hampshire , Durham NH 03824 , USA

40. Finnish Centre for Astronomy with ESO , University of Turku, FI-20014 Turku , Finland

41. Istituto Nazionale di Fisica Nucleare , Sezione di Napoli, Strada Comunale Cinthia, I-80126 Napoli , Italy

42. Graduate School of Science, Division of Particle and Astrophysical Science, Nagoya University , Furocho, Chikusaku, Nagoya, Aichi 464-8602 , Japan

43. Hiroshima Astrophysical Science Center, Hiroshima University , 1-3-1 Kagamiyama, Higashi-Hiroshima, Hiroshima 739-8526 , Japan

44. University of Maryland , Baltimore County, Baltimore, MD 21250 , USA

45. NASA Goddard Space Flight Center , Greenbelt, MD 20771 , USA

46. Center for Research and Exploration in Space Science and Technology , NASA/GSFC, Greenbelt, MD 20771 , USA

47. Department of Physics, The University of Hong Kong , Pokfulam, Hong Kong

48. Department of Astronomy and Astrophysics, Pennsylvania State University , University Park, PA 16802 , USA

49. Center for Astrophysics | Harvard & Smithsonian , 60 Garden St, Cambridge, MA 02138 , USA

50. INAF Osservatorio Astronomico di Brera , Via E. Bianchi 46, I-23807 Merate (LC) , Italy

51. Dipartimento di Fisica e Astronomia, Università degli Studi di Padova , Via Marzolo 8, I-35131 Padova , Italy

52. Mullard Space Science Laboratory, University College London , Holmbury St Mary, Dorking, Surrey RH5 6NT , UK

53. Anton Pannekoek Institute for Astronomy & GRAPPA, University of Amsterdam , Science Park 904, NL-1098 XH Amsterdam , the Netherlands

54. Guangxi Key Laboratory for Relativistic Astrophysics, School of Physical Science and Technology, Guangxi University , Nanning 530004 , China

Abstract

ABSTRACT We present an X-ray spectro-polarimetric analysis of the bright Seyfert galaxy IC 4329A. The Imaging X-ray Polarimetry Explorer (IXPE) observed the source for ∼500 ks, supported by XMM–Newton (∼60 ks) and NuSTAR (∼80 ks) exposures. We detect polarization in the 2–8 keV band with 2.97σ confidence. We report a polarization degree of 3.3 ± 1.1 per cent and a polarization angle of 78° ± 10° (errors are 1σ confidence). The X-ray polarization is consistent with being aligned with the radio jet, albeit partially due to large uncertainties on the radio position angle. We jointly fit the spectra from the three observatories to constrain the presence of a relativistic reflection component. From this, we obtain constraints on the inclination angle to the inner disc (<39° at 99 per cent confidence) and the disc inner radius (<11 gravitational radii at 99 per cent confidence), although we note that modelling systematics in practice add to the quoted statistical error. Our spectropolarimetric modelling indicates that the 2–8 keV polarization is consistent with being dominated by emission directly observed from the X-ray corona, but the polarization of the reflection component is completely unconstrained. Our constraints on viewer inclination and polarization degree tentatively favour more asymmetric, possibly out-flowing, coronal geometries that produce more highly polarized emission, but the coronal geometry is unconstrained at the 3σ level.

Funder

CNRS

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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