Title: X-ray polarization measurement of the gold standard of radio-quiet active galactic nuclei: NGC 1068
Context.NGC 1068 is the most observed radio-quiet active galactic nucleus (AGN) in polarimetry, yet its high-energy polarization has never been probed before due to a lack of dedicated polarimeters. Aims.Using the first X-ray polarimeter sensitive enough to measure the polarization of AGNs, we want to probe the orientation and geometric arrangement of (sub)parsec-scale matter around the X-ray source. Methods.We used the Imaging X-ray Polarimetry Explorer (IXPE) satellite to measure, for the first time, the 2–8 keV polarization of NGC 1068. We pointed IXPE at the target for a net exposure time of 1.15 Ms, in addition to using twoChandrasnapshots of ∼10 ks each in order to account for the potential impact of several ultraluminous X-ray sources (ULXs) within IXPE’s field of view. Results.We measured a 2–8 keV polarization degree of 12.4% ± 3.6% and an electric vector polarization angle of 101° ± 8° at a 68% confidence level. If we exclude the spectral region containing bright Fe K lines and other soft X-ray lines where depolarization occurs, the polarization fraction rises to 21.3% ± 6.7% in the 3.5–6.0 keV band, with a similar polarization angle. The observed polarization angle is found to be perpendicular to the parsec-scale radio jet. Using a combinedChandraand IXPE analysis plus multiwavelength constraints, we estimated that the circumnuclear “torus” may sustain a half-opening angle of 50–55° (from the vertical axis of the system). Conclusions.Thanks to IXPE, we have measured the X-ray polarization of NGC 1068 and found comparable results, both in terms of the polarization angle orientation with respect to the radio jet and the torus half-opening angle, to the X-ray polarimetric measurement achieved for the other archetypal Compton-thick AGN: the Circinus galaxy. Probing the geometric arrangement of parsec-scale matter in extragalactic objects is now feasible thanks to X-ray polarimetry. more »« less
Ursini, F; Marinucci, A; Matt, G; Bianchi, S; Marin, F; Marshall, H L; Middei, R; Poutanen, J; Rogantini, D; De Rosa, A; et al
(, Monthly Notices of the Royal Astronomical Society)
ABSTRACT We report on the Imaging X-ray Polarimetry Explorer (IXPE) observation of the closest and X-ray brightest Compton-thick active galactic nucleus (AGN), the Circinus galaxy. We find the source to be significantly polarized in the 2–6 keV band. From previous studies, the X-ray spectrum is known to be dominated by reflection components, both neutral (torus) and ionized (ionization cones). Our analysis indicates that the polarization degree is 28 ± 7 per cent (at 68 per cent confidence level) for the neutral reflector, with a polarization angle of 18° ± 5°, roughly perpendicular to the radio jet. The polarization of the ionized reflection is unconstrained. A comparison with Monte Carlo simulations of the polarization expected from the torus shows that the neutral reflector is consistent with being an equatorial torus with a half-opening angle of 45°–55°. This is the first X-ray polarization detection in a Seyfert galaxy, demonstrating the power of X-ray polarimetry in probing the geometry of the circumnuclear regions of AGNs, and confirming the basic predictions of standard Unification Models.
X-ray polarimetry has been suggested as a prominent tool for investigating the geometrical and physical properties of the emissions from active galactic nuclei (AGN). The successful launch of the Imaging X-ray Polarimetry Explorer (IXPE) on 9 December 2021 has expanded the previously restricted scope of polarimetry into the X-ray domain, enabling X-ray polarimetric studies of AGN. Over a span of two years, IXPE has observed various AGN populations, including blazars and radio-quiet AGN. In this paper, we summarize the remarkable discoveries achieved thanks to the opening of the new window of X-ray polarimetry of AGN through IXPE observations. We will delve into two primary areas of interest: first, the magnetic field geometry and particle acceleration mechanisms in the jets of radio-loud AGN, such as blazars, where the relativistic acceleration process dominates the spectral energy distribution; and second, the geometry of the hot corona in radio-quiet AGN. Thus far, the IXPE results from blazars favor the energy-stratified shock acceleration model, and they provide evidence of helical magnetic fields inside the jet. Concerning the corona geometry, the IXPE results are consistent with a disk-originated slab-like or wedge-like shape, as could result from Comptonization around the accretion disk.
Gianolli, V E; Kim, D E; Bianchi, S; Agís-González, B; Madejski, G; Marin, F; Marinucci, A; Matt, G; Middei, R; Petrucci, P-O; et al
(, Monthly Notices of the Royal Astronomical Society)
ABSTRACT We present an X-ray spectropolarimetric analysis of the bright Seyfert galaxy NGC 4151. The source has been observed with the Imaging X-ray Polarimetry Explorer (IXPE) for 700 ks, complemented with simultaneous XMM–Newton (50 ks) and NuSTAR (100 ks) pointings. A polarization degree Π = 4.9 ± 1.1 per cent and angle Ψ = 86° ± 7° east of north (68 per cent confidence level) are measured in the 2–8 keV energy range. The spectropolarimetric analysis shows that the polarization could be entirely due to reflection. Given the low reflection flux in the IXPE band, this requires, however, a reflection with a very large (>38 per cent) polarization degree. Assuming more reasonable values, a polarization degree of the hot corona ranging from ∼4 to ∼8 per cent is found. The observed polarization degree excludes a ‘spherical’ lamppost geometry for the corona, suggesting instead a slab-like geometry, possibly a wedge, as determined via Monte Carlo simulations. This is further confirmed by the X-ray polarization angle, which coincides with the direction of the extended radio emission in this source, supposed to match the disc axis. NGC 4151 is the first active galactic nucleus with an X-ray polarization measure for the corona, illustrating the capabilities of X-ray polarimetry and IXPE in unveiling its geometry.
Kim, Dawoon E; Di_Gesu, Laura; Liodakis, Ioannis; Marscher, Alan P; Jorstad, Svetlana G; Middei, Riccardo; Marshall, Herman L; Pacciani, Luigi; Agudo, Iván; Tavecchio, Fabrizio; et al
(, Astronomy & Astrophysics)
Aims.We aim to probe the magnetic field geometry and particle acceleration mechanism in the relativistic jets of supermassive black holes. Methods.We conducted a polarimetry campaign from radio to X-ray wavelengths of the high-synchrotron-peak (HSP) blazar Mrk 421, including Imaging X-ray Polarimetry Explorer (IXPE) measurements from 2022 December 6–8. During the IXPE observation, we also monitored Mrk 421 usingSwift-XRT and obtained a single observation withXMM-Newtonto improve the X-ray spectral analysis. The time-averaged X-ray polarization was determined consistently using the event-by-event Stokes parameter analysis, spectropolarimetric fit, and maximum likelihood methods. We examined the polarization variability over both time and energy, the former via analysis of IXPE data obtained over a time span of 7 months. Results.We detected X-ray polarization of Mrk 421 with a degree of ΠX = 14 ± 1% and an electric-vector position angleψX = 107 ± 3° in the 2–8 keV band. From the time variability analysis, we find a significant episodic variation inψX. During the 7 months from the first IXPE pointing of Mrk 421 in 2022 May,ψXvaried in the range 0° to 180°, while ΠXremained relatively constant within ∼10–15%. Furthermore, a swing inψXin 2022 June was accompanied by simultaneous spectral variations. The results of the multiwavelength polarimetry show that ΠXwas generally ∼2–3 times greater than Π at longer wavelengths, whileψfluctuated. Additionally, based on radio, infrared, and optical polarimetry, we find that the rotation ofψoccurred in the opposite direction with respect to the rotation ofψXand over longer timescales at similar epochs. Conclusions.The polarization behavior observed across multiple wavelengths is consistent with previous IXPE findings for HSP blazars. This result favors the energy-stratified shock model developed to explain variable emission in relativistic jets. We considered two versions of the model, one with linear and the other with radial stratification geometry, to explain the rotation ofψX. The accompanying spectral variation during theψXrotation can be explained by a fluctuation in the physical conditions, for example in the energy distribution of relativistic electrons. The opposite rotation direction ofψbetween the X-ray and longer wavelength polarization accentuates the conclusion that the X-ray emitting region is spatially separated from that at longer wavelengths. Moreover, we identify a highly polarized knot of radio emission moving down the parsec-scale jet during the episode ofψXrotation, although it is unclear whether there is any connection between the two events.
Chen, Chien-Ting J; Liodakis, Ioannis; Middei, Riccardo; Kim, Dawoon E; Di_Gesu, Laura; Di_Marco, Alessandro; Ehlert, Steven R; Errando, Manel; Negro, Michela; Jorstad, Svetlana G; et al
(, The Astrophysical Journal)
Abstract We present multiwavelength polarization measurements of the luminous blazar Mrk 501 over a 14 month period. The 2–8 keV X-ray polarization was measured with the Imaging X-ray Polarimetry Explorer (IXPE) with six 100 ks observations spanning from 2022 March to 2023 April. Each IXPE observation was accompanied by simultaneous X-ray data from NuSTAR, Swift/XRT, and/or XMM-Newton. Complementary optical–infrared polarization measurements were also available in theB,V,R,I, andJbands, as were radio polarization measurements from 4.85 GHz to 225.5 GHz. Among the first five IXPE observations, we did not find significant variability in the X-ray polarization degree and angle with IXPE. However, the most recent sixth observation found an elevated polarization degree at >3σabove the average of the other five observations. The optical and radio measurements show no apparent correlations with the X-ray polarization properties. Throughout the six IXPE observations, the X-ray polarization degree remained higher than, or similar to, theR-band optical polarization degree, which remained higher than the radio value. This is consistent with the energy-stratified shock scenario proposed to explain the first two IXPE observations, in which the polarized X-ray, optical, and radio emission arises from different regions.
Marin, F, Marinucci, A, Laurenti, M, Kim, D E, Barnouin, T, Di_Marco, A, Ursini, F, Bianchi, S, Ravi, S, Marshall, H L, Matt, G, Chen, C-T, Gianolli, V E, Ingram, A, Middei, R, Maksym, W P, Panagiotou, C, Podgorny, J, Puccetti, S, Ratheesh, A, Tombesi, F, Agudo, I, Antonelli, L A, Bachetti, M, Baldini, L, Baumgartner, W, Bellazzini, R, Bongiorno, S, Bonino, R, Brez, A, Bucciantini, N, Capitanio, F, Castellano, S, Cavazzuti, E, Ciprini, S, Costa, E, De_Rosa, A, Del_Monte, E, Di_Gesu, L, Di_Lalla, N, Donnarumma, I, Doroshenko, V, Dovčiak, M, Ehlert, S, Enoto, T, Evangelista, Y, Fabiani, S, Ferrazzoli, R, Garcia, J, Gunji, S, Heyl, J, Iwakiri, W, Jorstad, S, Kaaret, P, Karas, V, Kislat, F, Kitaguchi, T, Kolodziejczak, J, Krawczynski, H, La_Monaca, F, Latronico, L, Liodakis, I, Madejski, G, Maldera, S, Manfreda, A, Marscher, A, Massaro, F, Mitsuishi, I, Mizuno, T, Muleri, F, Negro, M, Ng, S, O’Dell, S, Omodei, N, Oppedisano, C, Papitto, A, Pavlov, G, Perri, M, Pesce-Rollins, M, Petrucci, P-O, Pilia, M, Possenti, A, Poutanen, J, Ramsey, B, Rankin, J, Roberts, O, Romani, R, Sgrò, C, Slane, P, Soffitta, P, Spandre, G, Swartz, D, Tamagawa, T, Tavecchio, F, Taverna, R, Tawara, Y, Tennant, A, Thomas, N, Trois, A, Tsygankov, S, Turolla, R, Vink, J, Weisskopf, M, Wu, K, Xie, F, and Zane, S. X-ray polarization measurement of the gold standard of radio-quiet active galactic nuclei: NGC 1068. Retrieved from https://par.nsf.gov/biblio/10598221. Astronomy & Astrophysics 689. Web. doi:10.1051/0004-6361/202449760.
Marin, F, Marinucci, A, Laurenti, M, Kim, D E, Barnouin, T, Di_Marco, A, Ursini, F, Bianchi, S, Ravi, S, Marshall, H L, Matt, G, Chen, C-T, Gianolli, V E, Ingram, A, Middei, R, Maksym, W P, Panagiotou, C, Podgorny, J, Puccetti, S, Ratheesh, A, Tombesi, F, Agudo, I, Antonelli, L A, Bachetti, M, Baldini, L, Baumgartner, W, Bellazzini, R, Bongiorno, S, Bonino, R, Brez, A, Bucciantini, N, Capitanio, F, Castellano, S, Cavazzuti, E, Ciprini, S, Costa, E, De_Rosa, A, Del_Monte, E, Di_Gesu, L, Di_Lalla, N, Donnarumma, I, Doroshenko, V, Dovčiak, M, Ehlert, S, Enoto, T, Evangelista, Y, Fabiani, S, Ferrazzoli, R, Garcia, J, Gunji, S, Heyl, J, Iwakiri, W, Jorstad, S, Kaaret, P, Karas, V, Kislat, F, Kitaguchi, T, Kolodziejczak, J, Krawczynski, H, La_Monaca, F, Latronico, L, Liodakis, I, Madejski, G, Maldera, S, Manfreda, A, Marscher, A, Massaro, F, Mitsuishi, I, Mizuno, T, Muleri, F, Negro, M, Ng, S, O’Dell, S, Omodei, N, Oppedisano, C, Papitto, A, Pavlov, G, Perri, M, Pesce-Rollins, M, Petrucci, P-O, Pilia, M, Possenti, A, Poutanen, J, Ramsey, B, Rankin, J, Roberts, O, Romani, R, Sgrò, C, Slane, P, Soffitta, P, Spandre, G, Swartz, D, Tamagawa, T, Tavecchio, F, Taverna, R, Tawara, Y, Tennant, A, Thomas, N, Trois, A, Tsygankov, S, Turolla, R, Vink, J, Weisskopf, M, Wu, K, Xie, F, & Zane, S. X-ray polarization measurement of the gold standard of radio-quiet active galactic nuclei: NGC 1068. Astronomy & Astrophysics, 689 (). Retrieved from https://par.nsf.gov/biblio/10598221. https://doi.org/10.1051/0004-6361/202449760
Marin, F, Marinucci, A, Laurenti, M, Kim, D E, Barnouin, T, Di_Marco, A, Ursini, F, Bianchi, S, Ravi, S, Marshall, H L, Matt, G, Chen, C-T, Gianolli, V E, Ingram, A, Middei, R, Maksym, W P, Panagiotou, C, Podgorny, J, Puccetti, S, Ratheesh, A, Tombesi, F, Agudo, I, Antonelli, L A, Bachetti, M, Baldini, L, Baumgartner, W, Bellazzini, R, Bongiorno, S, Bonino, R, Brez, A, Bucciantini, N, Capitanio, F, Castellano, S, Cavazzuti, E, Ciprini, S, Costa, E, De_Rosa, A, Del_Monte, E, Di_Gesu, L, Di_Lalla, N, Donnarumma, I, Doroshenko, V, Dovčiak, M, Ehlert, S, Enoto, T, Evangelista, Y, Fabiani, S, Ferrazzoli, R, Garcia, J, Gunji, S, Heyl, J, Iwakiri, W, Jorstad, S, Kaaret, P, Karas, V, Kislat, F, Kitaguchi, T, Kolodziejczak, J, Krawczynski, H, La_Monaca, F, Latronico, L, Liodakis, I, Madejski, G, Maldera, S, Manfreda, A, Marscher, A, Massaro, F, Mitsuishi, I, Mizuno, T, Muleri, F, Negro, M, Ng, S, O’Dell, S, Omodei, N, Oppedisano, C, Papitto, A, Pavlov, G, Perri, M, Pesce-Rollins, M, Petrucci, P-O, Pilia, M, Possenti, A, Poutanen, J, Ramsey, B, Rankin, J, Roberts, O, Romani, R, Sgrò, C, Slane, P, Soffitta, P, Spandre, G, Swartz, D, Tamagawa, T, Tavecchio, F, Taverna, R, Tawara, Y, Tennant, A, Thomas, N, Trois, A, Tsygankov, S, Turolla, R, Vink, J, Weisskopf, M, Wu, K, Xie, F, and Zane, S.
"X-ray polarization measurement of the gold standard of radio-quiet active galactic nuclei: NGC 1068". Astronomy & Astrophysics 689 (). Country unknown/Code not available: EDP Sciences. https://doi.org/10.1051/0004-6361/202449760.https://par.nsf.gov/biblio/10598221.
@article{osti_10598221,
place = {Country unknown/Code not available},
title = {X-ray polarization measurement of the gold standard of radio-quiet active galactic nuclei: NGC 1068},
url = {https://par.nsf.gov/biblio/10598221},
DOI = {10.1051/0004-6361/202449760},
abstractNote = {Context.NGC 1068 is the most observed radio-quiet active galactic nucleus (AGN) in polarimetry, yet its high-energy polarization has never been probed before due to a lack of dedicated polarimeters. Aims.Using the first X-ray polarimeter sensitive enough to measure the polarization of AGNs, we want to probe the orientation and geometric arrangement of (sub)parsec-scale matter around the X-ray source. Methods.We used the Imaging X-ray Polarimetry Explorer (IXPE) satellite to measure, for the first time, the 2–8 keV polarization of NGC 1068. We pointed IXPE at the target for a net exposure time of 1.15 Ms, in addition to using twoChandrasnapshots of ∼10 ks each in order to account for the potential impact of several ultraluminous X-ray sources (ULXs) within IXPE’s field of view. Results.We measured a 2–8 keV polarization degree of 12.4% ± 3.6% and an electric vector polarization angle of 101° ± 8° at a 68% confidence level. If we exclude the spectral region containing bright Fe K lines and other soft X-ray lines where depolarization occurs, the polarization fraction rises to 21.3% ± 6.7% in the 3.5–6.0 keV band, with a similar polarization angle. The observed polarization angle is found to be perpendicular to the parsec-scale radio jet. Using a combinedChandraand IXPE analysis plus multiwavelength constraints, we estimated that the circumnuclear “torus” may sustain a half-opening angle of 50–55° (from the vertical axis of the system). Conclusions.Thanks to IXPE, we have measured the X-ray polarization of NGC 1068 and found comparable results, both in terms of the polarization angle orientation with respect to the radio jet and the torus half-opening angle, to the X-ray polarimetric measurement achieved for the other archetypal Compton-thick AGN: the Circinus galaxy. Probing the geometric arrangement of parsec-scale matter in extragalactic objects is now feasible thanks to X-ray polarimetry.},
journal = {Astronomy & Astrophysics},
volume = {689},
publisher = {EDP Sciences},
author = {Marin, F and Marinucci, A and Laurenti, M and Kim, D E and Barnouin, T and Di_Marco, A and Ursini, F and Bianchi, S and Ravi, S and Marshall, H L and Matt, G and Chen, C-T and Gianolli, V E and Ingram, A and Middei, R and Maksym, W P and Panagiotou, C and Podgorny, J and Puccetti, S and Ratheesh, A and Tombesi, F and Agudo, I and Antonelli, L A and Bachetti, M and Baldini, L and Baumgartner, W and Bellazzini, R and Bongiorno, S and Bonino, R and Brez, A and Bucciantini, N and Capitanio, F and Castellano, S and Cavazzuti, E and Ciprini, S and Costa, E and De_Rosa, A and Del_Monte, E and Di_Gesu, L and Di_Lalla, N and Donnarumma, I and Doroshenko, V and Dovčiak, M and Ehlert, S and Enoto, T and Evangelista, Y and Fabiani, S and Ferrazzoli, R and Garcia, J and Gunji, S and Heyl, J and Iwakiri, W and Jorstad, S and Kaaret, P and Karas, V and Kislat, F and Kitaguchi, T and Kolodziejczak, J and Krawczynski, H and La_Monaca, F and Latronico, L and Liodakis, I and Madejski, G and Maldera, S and Manfreda, A and Marscher, A and Massaro, F and Mitsuishi, I and Mizuno, T and Muleri, F and Negro, M and Ng, S and O’Dell, S and Omodei, N and Oppedisano, C and Papitto, A and Pavlov, G and Perri, M and Pesce-Rollins, M and Petrucci, P-O and Pilia, M and Possenti, A and Poutanen, J and Ramsey, B and Rankin, J and Roberts, O and Romani, R and Sgrò, C and Slane, P and Soffitta, P and Spandre, G and Swartz, D and Tamagawa, T and Tavecchio, F and Taverna, R and Tawara, Y and Tennant, A and Thomas, N and Trois, A and Tsygankov, S and Turolla, R and Vink, J and Weisskopf, M and Wu, K and Xie, F and Zane, S},
}
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