Toggle Main Menu Toggle Search

Open Access padlockePrints

The geometry of the hot corona in MCG-05-23-16 constrained by X-ray polarimetry

Lookup NU author(s): Dr Adam IngramORCiD

Downloads

Full text for this publication is not currently held within this repository. Alternative links are provided below where available.


Abstract

© 2023 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society.We report on the second observation of the radio-quiet active galactic nucleus MCG-05-23-16 performed with the Imaging X-ray Polarimetry Explorer (IXPE). The observation started on 2022 November 6 for a net observing time of 640 ks, and was partly simultaneous with NuSTAR (86 ks). After combining these data with those obtained in the first IXPE pointing on 2022 May (simultaneous with XMM-Newton and NuSTAR) we find a 2-8 keV polarization degree Π = 1.6 ± 0.7 (at 68 per cent confidence level), which corresponds to an upper limit Π = 3.2 per cent (at 99 per cent confidence level). We then compare the polarization results with Monte Carlo simulations obtained with the monk code, with which different coronal geometries have been explored (spherical lamppost, conical, slab, and wedge). Furthermore, the allowed range of inclination angles is found for each geometry. If the best-fitting inclination value from a spectroscopic analysis is considered, a cone-shaped corona along the disc axis is disfavoured.


Publication metadata

Author(s): Tagliacozzo D, Marinucci A, Ursini F, Matt G, Bianchi S, Baldini L, Barnouin T, Cavero Rodriguez N, De Rosa A, Di Gesu L, Dovciak M, Harper D, Ingram A, Karas V, Kim DE, Krawczynski H, Madejski G, Marin F, Middei R, Marshall HL, Muleri F, Panagiotou C, Petrucci P-O, Podgorny J, Poutanen J, Puccetti S, Soffitta P, Tombesi F, Veledina A, Zhang W, Agudo I, Antonelli LA, Bachetti M, Baumgartner WH, Bellazzini R, Bongiorno SD, Bonino R, Brez A, Bucciantini N, Capitanio F, Castellano S, Cavazzuti E, Chen C-T, Ciprini S, Costa E, Del Monte E, Di Lalla N, Di Marco A, Donnarumma I, Doroshenko V, Ehlert SR, Enoto T, Evangelista Y, Fabiani S, Ferrazzoli R, Garcia JA, Gunji S, Heyl J, Iwakiri W, Jorstad SG, Kaaret P, Kislat F, Kitaguchi T, Kolodziejczak JJ, La Monaca F, Latronico L, Liodakis I, Maldera S, Manfreda A, Marscher AP, Massaro F, Mitsuishi I, Mizuno T, Negro M, Ng C-Y, O'Dell SL, Omodei N, Oppedisano C, Papitto A, Pavlov GG, Peirson AL, Perri M, Pesce-Rollins M, Pilia M, Possenti A, Ramsey BD, Rankin J, Ratheesh A, Roberts OJ, Romani RW, Sgro C, Slane P, Spandre G, Swartz DA, Tamagawa T, Tavecchio F, Taverna R, Tawara Y, Tennant AF, Thomas NE, Trois A, Tsygankov SS, Turolla R, Vink J, Weisskopf MC, Wu K, Xie F, Zane S

Publication type: Article

Publication status: Published

Journal: Monthly Notices of the Royal Astronomical Society

Year: 2023

Volume: 525

Issue: 3

Pages: 4735-4743

Print publication date: 01/11/2023

Online publication date: 01/09/2023

Acceptance date: 28/07/2023

ISSN (print): 0035-8711

ISSN (electronic): 1365-2966

Publisher: Oxford University Press

URL: https://doi.org/10.1093/mnras/stad2627

DOI: 10.1093/mnras/stad2627


Altmetrics

Altmetrics provided by Altmetric


Share