A dataset provided by the European Space Agency

Name: The broad Fe line of the bright Seyfert 1 galaxy Mrk 1040
Published: 2010-03-10T00:00:00Z

Proposal ID	055499
Title	The broad Fe line of the bright Seyfert 1 galaxy Mrk 1040
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0554990101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0554990201
DOI	https://doi.org/10.5270/esa-z8aq9jc
Principal Investigator, PI	Dr Giovanni Miniutti
Abstract	We propose to observe the bright Seyfert 1 galaxy Mrk 1040 with XMM-Newton. Withan exposure of 80ks, we will be able to measure the continuum and Fe K$alpha$line parameters with much better accuracy than possible before with ASCA. Thiswill enable us to infer the location of the Fe-emitting gas. If the lineoriginates from within 6 gravitational radii from the black hole, information onthe black hole spin could be derived. Mrk 1040 is also bright enough to allow usto study Fe line variability down to a 15 ks timescale. The soft sensitivity ofXMM-Newton will be used to characterise the nature of the soft X-ray absorptionin this AGN.
Publications	The Swift Burst Alert Telescope Detected Seyfert 1 Galaxies: X-Ray Broadband Properties and Warm Absorbers \|Winter Lisa M. Veilleux Sylvain et al. \| ApJ \| 745-107 \| 2012 \| 2012ApJ...745..107W \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...745..107W X-ray Outflows in the Swift Burst Alert Detected Seyfert 1s \|Winter Lisa M. \| ApJ \| 725-126 \| 2010 \| 2010ApJ...725L.126W \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...725L.126W Soft Time Lags in the X-Ray Emission of Mrk 1040 \|Tripathi Shruti Misra Ranjeev et al. \| ApJ \| 736-37 \| 2011 \| 2011ApJ...736L..37T \| http://ui.adsabs.harvard.edu/#abs/2011ApJ...736L..37T CAIXA: a catalogue of AGN in the XMM-Newton archive. III. Excess variance analysis \|Ponti G. Papadakis I. et al. \| A&A \| 542-83 \| 2012 \| 2012A&A...542A..83P \| http://ui.adsabs.harvard.edu/#abs/2012A&A...542A..83P X-ray variability of 104 active galactic nuclei. XMM-Newton power-spectrum density profiles \|Gonzalez-Martin O. Vaughan S. \| A&A \| 544-80 \| 2012 \| 2012A&A...544A..80G \| http://ui.adsabs.harvard.edu/#abs/2012A&A...544A..80G Discovery of a relation between black hole mass and soft X-ray time lags in active galactic nuclei \|De Marco B. Ponti G. et al. \| MNRAS \| 431-2441 \| 2013 \| 2013MNRAS.431.2441D \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.431.2441D Are X-Ray Emitting Coronae around Supermassive Black Holes Outflowing? \|Liu Teng Wang Jun-Xian et al. \| ApJ \| 783-106 \| 2014 \| 2014ApJ...783..106L \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...783..106L 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 reverberation around accreting black holes \|Uttley P. Cackett E. M. et al. \| A&ARv \| 22-72 \| 2014 \| 2014A&ARv..22...72U \| http://ui.adsabs.harvard.edu/#abs/2014A&ARv..22...72U X-ray spectral parameters for a sample of 95 active galactic nuclei \|Vasylenko A. A. Zhdanov V. I. \| Ap&SS \| 360-71 \| 2015 \| 2015Ap&SS.360...71V \| http://ui.adsabs.harvard.edu/#abs/2015Ap&SS.360...71V A hard X-ray view of the soft excess in AGN \|Boissay Rozenn Ricci Claudio \| A&A \| 588-70 \| 2016 \| 2016A&A...588A..70B \| http://ui.adsabs.harvard.edu/#abs/2016A&A...588A..70B 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 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 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 A Systematic Study of the Short-term X-Ray Variability of Seyfert Galaxies. I. Diversity of the X-Ray rms Spectra \|Hu Jingwei Jin Chichuan et al. \| ApJ \| 936-105 \| 2022 \| 2022ApJ...936..105H \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...936..105H Tracing the evolving X-ray reverberation lags within an individual AGN light curve \|Nakhonthong N. Chainakun P. et al. \| MNRAS \| 530-1894 \| 2024 \| 2024MNRAS.530.1894N \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.530.1894N 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	2009-02-13T14:30:26Z/2009-02-14T18:38:53Z
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	2010-03-10T00:00:00Z
Last Update	2025-01-27
Keywords	"soft xray absorption", "galaxy mrk 1040", "gravitational radii", "xmm newton", "broad fe line", "XMM-Newton", "line parameters", "fe emitting gas", "blackhole spin", "mrk 1040", "line originates", "bright seyfert", "XMM", "fe line variability", "soft sensitivity", "black hole"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Giovanni Miniutti, 2010, 'The broad Fe line of the bright Seyfert 1 galaxy Mrk 1040', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-z8aq9jc