A dataset provided by the European Space Agency

Name: The nature of the nuclear and extended emission in NGC 5643
Published: 2010-08-26T00:00:00Z

Proposal ID	060142
Title	The nature of the nuclear and extended emission in NGC 5643
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0601420101
DOI	https://doi.org/10.5270/esa-r2z0lnm
Principal Investigator, PI	Prof Giorgio Matt
Abstract	We propose a 50 ks XMM-Newton observation of the Seyfert 2 galaxy, NGC 5643,with the aim of answering two questions left unanswered by the previous, muchshorter (less than 10 ks) XMM-Newton observation. In particular, we want to: a)Measure the O vii triplet with sufficient signal-to-noise to unambiguouslydistinguish between photoionized and collisionally ionized matter. Contrary tomost other Seyferts, in this source collisional plasma seems to dominate, butthe previous measures are inconclusive. b) Distinguish between the twoalternative models for the hard X-ray emission, i.e. nuclear emission plusscattering component or partially absorbed Compton reflect ion. This will helpus to better understand the nature and morphology of the obscuring matter.
Publications	Comparison of Millimeter-wave and X-Ray Emission in Seyfert Galaxies \|Monje R. R. Blain A. W. \| ApJS \| 195-23 \| 2011 \| 2011ApJS..195...23M \| http://ui.adsabs.harvard.edu/#abs/2011ApJS..195...23M X-ray observations of the Compton-thick Seyfert 2 galaxy NGC 5643 \|Matt G. Bianchi S. et al. \| A&A \| 556-91 \| 2013 \| 2013A&A...556A..91M \| http://ui.adsabs.harvard.edu/#abs/2013A&A...556A..91M 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 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 Non-detection of X-ray emission from sterile neutrinos in stacked galaxy spectra \|Anderson Michael E. Churazov Eugene \| MNRAS \| 452-3905 \| 2015 \| 2015MNRAS.452.3905A \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.452.3905A NuSTAR Observations of the Compton-thick Active Galactic Nucleus and Ultraluminous X-Ray Source Candidate in NGC 5643 \|Annuar A. Gandhi P. et al. \| ApJ \| 815-36 \| 2015 \| 2015ApJ...815...36A \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...815...36A 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 The ultraluminous X-ray source NGC 5643 ULX1: a large stellar mass black hole accreting at super-Eddington rates? \|Pintore Fabio Zampieri Luca et al. \| MNRAS \| 459-455 \| 2016 \| 2016MNRAS.459..455P \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.459..455P 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 NuSTAR and XMM-Newton observations of the ultraluminous X-ray source NGC 5643 X-1 \|Krivonos Roman Sazonov Sergey \| MNRAS \| 463-756 \| 2016 \| 2016MNRAS.463..756K \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.463..756K 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 Study of Swift/Bat Selected Low-luminosity Active Galactic Nuclei Observed with Suzaku \|Kawamuro Taiki Ueda Yoshihiro et al. \| ApJ \| 831-37 \| 2016 \| 2016ApJ...831...37K \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...831...37K 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 A new clean catalogue of extragalactic non-nuclear X-ray sources in nearby galaxies \|Earnshaw H. P. Roberts T. P. et al. \| MNRAS \| 483-5554 \| 2019 \| 2019MNRAS.483.5554E \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483.5554E 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 A Broadband X-Ray Study of a Sample of AGNs with O III Measured Inclinations \|Zhao X. Marchesi S. et al. \| ApJ \| 894-71 \| 2020 \| 2020ApJ...894...71Z \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...894...71Z Spectral Properties of Heavily Obscured Seyfert Galaxies from the INTEGRAL All-Sky Survey \|Semena A. N. Sazonov S. Yu. \| AstL \| 45-490 \| 2019 \| 2019AstL...45..490S \| http://ui.adsabs.harvard.edu/#abs/2019AstL...45..490S 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 impact of precession on the observed population of ULXs \|Khan Norman Middleton Matthew J. et al. \| MNRAS \| 509-2493 \| 2022 \| 2022MNRAS.509.2493K \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.509.2493K The Redshift Evolution of Ultraluminous X-Ray Sources out to z 0.5: Comparison with X-Ray Binary Populations and Contribution to the Cosmic X-Ray Background \|Scott Barrows R. Comerford Julia M. et al. \| ApJ \| 932-27 \| 2022 \| 2022ApJ...932...27S \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...932...27S The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII O VIII and Fe L-shell Transitions \|Pan Zeyang Qu Zhijie et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P 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	2009-07-25T18:12:49Z/2009-07-26T09:21:29Z
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	2010-08-26T00:00:00Z
Last Update	2025-01-27
Keywords	"obscuring matter", "NGC 5643", "unambiguously distinguish", "hard xray emission", "ngc 5643", "xmm newton", "alternative models", "XMM-Newton", "source collisional plasma", "left unanswered", "collisionally ionized matter", "XMM", "vii triplet"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Giorgio Matt, 2010, 'The nature of the nuclear and extended emission in NGC 5643', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-r2z0lnm