A dataset provided by the European Space Agency

Name: The X-ray spectral signatures from the complex circumnuclear regions in NGC424
Published: 2010-01-10T00:00:00Z

Proposal ID	055095
Title	The X-ray spectral signatures from the complex circumnuclear regions in NGC424
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550950101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550950201
DOI	https://doi.org/10.5270/esa-zdvklha
Principal Investigator, PI	Dr Stefano Bianchi
Abstract	We propose a 100 ks observation of NGC424 to exploit the full range ofXMM-Newton capabilities (RGS+EPIC) by studying the properties of the differentmaterials found in the nucleus of this object.NGC424 is one of the brightestCompton-thick AGN,thus being one of the few sources which presently permit thiskind of analysis.The proposed 100 ks EPIC spectrum will allow us to study indetail the properties of the torus,by measuring:the iron Kalpha/Kbeta ratio andthe iron Kalpha centroid energy,to determine its ionization state and thenestimate its distance from the Black Hole;the Compton Shoulder,to check if thecold reflecting matter is indeed the inner wall of the obscuring torus.On theother hand, the RGS high resolution spectrum will allow us to take advantage of
Publications	The X-ray spectral signatures from the complex circumnuclear regions in the Compton thick AGN NGC 424 \|Marinucci A. Bianchi S. et al. \| A&A \| 526-36 \| 2011 \| 2011A&A...526A..36M \| http://ui.adsabs.harvard.edu/#abs/2011A&A...526A..36M An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities \|Henley David B. Shelton Robin L. \| ApJS \| 202-14 \| 2012 \| 2012ApJS..202...14H \| http://ui.adsabs.harvard.edu/#abs/2012ApJS..202...14H An XMM-Newton Survey of the Soft X-Ray Background. III. The Galactic Halo X-Ray Emission \|Henley David B. Shelton Robin L. \| ApJ \| 773-92 \| 2013 \| 2013ApJ...773...92H \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...773...92H CLASH-X: A Comparison of Lensing and X-Ray Techniques for Measuring the Mass Profiles of Galaxy Clusters \|Donahue Megan Voit G. Mark et al. \| ApJ \| 794-136 \| 2014 \| 2014ApJ...794..136D \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...794..136D Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov V. N. \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y The Origin of the Hot Gas in the Galactic Halo: Testing Galactic Fountain Models X-Ray Emission \|Henley David B. Shelton Robin L. et al. \| ApJ \| 800-102 \| 2015 \| 2015ApJ...800..102H \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...800..102H X-ray spectral variability of Seyfert 2 galaxies \|Hernandez-Garcia L. Masegosa J. et al. \| A&A \| 579-90 \| 2015 \| 2015A&A...579A..90H \| http://ui.adsabs.harvard.edu/#abs/2015A&A...579A..90H Compton-thick Accretion in the Local Universe \|Ricci C. Ueda Y. et al. \| ApJ \| 815-13 \| 2015 \| 2015ApJ...815L..13R \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...815L..13R Unveiling the Physics of Low-luminosity AGNs through X-Ray Variability: LINER versus Seyfert 2 \|Hernandez-Garcia L. Masegosa J. et al. \| ApJ \| 824-7 \| 2016 \| 2016ApJ...824....7H \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...824....7H The Interaction of the Fermi Bubbles with the Milky Ways Hot Gas Halo \|Miller Matthew J. Bregman Joel N. \| ApJ \| 829-9 \| 2016 \| 2016ApJ...829....9M \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...829....9M The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch Eric W. \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F The close environments of accreting massive black holes are shaped by radiative feedback \|Ricci Claudio Trakhtenbrot Benny et al. \| Natur \| 549-488 \| 2017 \| 2017Natur.549..488R \| http://ui.adsabs.harvard.edu/#abs/2017Natur.549..488R BAT AGN Spectroscopic Survey (BASS) - VI. The GammaX-L/LEdd relation \|Trakhtenbrot Benny Ricci Claudio et al. \| MNRAS \| 470-800 \| 2017 \| 2017MNRAS.470..800T \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.470..800T BAT AGN Spectroscopic Survey. V. X-Ray Properties of the Swift/BAT 70-month AGN Catalog \|Ricci C. Trakhtenbrot B. et al. \| ApJS \| 233-17 \| 2017 \| 2017ApJS..233...17R \| http://ui.adsabs.harvard.edu/#abs/2017ApJS..233...17R Compton-thick AGNs in the NuSTAR Era \|Marchesi S. Ajello M. et al. \| ApJ \| 854-49 \| 2018 \| 2018ApJ...854...49M \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...854...49M The Swift/BAT AGN Spectroscopic Survey. IX. The Clustering Environments of an Unbiased Sample of Local AGNs \|Powell M. C. Cappelluti N. et al. \| ApJ \| 858-110 \| 2018 \| 2018ApJ...858..110P \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...858..110P Hot corona properties of Swift/BAT-detected AGNs \|Wang Chan Yu Li-Ming et al. \| MNRAS \| 487-2463 \| 2019 \| 2019MNRAS.487.2463W \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.487.2463W Constraining the Milky Way Mass with Its Hot Gaseous Halo \|Guo Fulai Zhang Ruiyu \| ApJ \| 904-14 \| 2020 \| 2020ApJ...904L..14G \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...904L..14G An X-Ray- and SZ-bright Diffuse Source toward M31: A Local Hot Bridge \|Qu Zhijie Huang Rui et al. \| ApJ \| 907-14 \| 2021 \| 2021ApJ...907...14Q \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...907...14Q Classification of 4XMM-DR9 sources by machine learning \|Zhang Yanxia Zhao Yongheng \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z The Solar Cycle Temporal Variation of the Solar Wind Charge Exchange X-Ray Lines \|Qu Zhijie Koutroumpa Dimitra et al. \| ApJ \| 930-21 \| 2022 \| 2022ApJ...930...21Q \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...930...21Q NuSTAR Observations of 52 Compton-thick Active Galactic Nuclei Selected by the Swift/Burst Alert Telescope All-sky Hard X-Ray Survey \|Tanimoto Atsushi Ueda Yoshihiro et al. \| ApJS \| 260-30 \| 2022 \| 2022ApJS..260...30T \| http://ui.adsabs.harvard.edu/#abs/2022ApJS..260...30T From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez Antonio C. \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2008-12-07T19:08:11Z/2008-12-09T07:45:04Z
Version	17.56_20190403_1200
Mission Description	The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact	https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published	2010-01-10T00:00:00Z
Last Update	2025-01-27
Keywords	"complex circumnuclear region", "EPIC", "kbeta ratio", "xray spectral signatures", "obscuring torus", "epic spectrum", "xmm newton", "NGC424", "cold reflecting matter", "XMM-Newton", "inner wall", "iron kalpha", "XMM", "compton shoulder", "presently permit", "resolution spectrum", "black hole"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Stefano Bianchi, 2010, 'The X-ray spectral signatures from the complex circumnuclear regions in NGC424', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-zdvklha