A dataset provided by the European Space Agency

Name: A hard X-ray view of the inner disc in Mrk 1040
Published: 2016-09-07T22:00:00Z

Proposal ID	076053
Title	A hard X-ray view of the inner disc in Mrk 1040
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0760530201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0760530301
DOI	https://doi.org/10.5270/esa-0f66iv9
Principal Investigator, PI	Dr James Reeves
Abstract	The study of the X-ray spectral components in AGN allows us in principle toinfer the properties of the accretion disk and in some cases, the black holespin. This proposal concerns the study of the nearby, X- ray bright Seyfert 1galaxy, Mrk 1040, which shows the presence of an unusually intense and highlybroadened (FWHM: 60000 km/s) Fe K line, as well as a strong hard X-ray excessabove 10 keV. Mrk 1040 is also rapidly variable and shows a tentative detectionof lags at soft X-rays. Here we request simultaneous XMM-Newton and NuSTARobservations (160 ks and 120 ks), enabling us to determine the origin of thehard X-ray excess and ultimately the spin of the central black hole. We willalso determine the presence the X-ray lags above 10 keV, as expected in disc reverberation scenarios.
Publications	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 Fundamental X-ray corona parameters of Swift/BAT AGN \|Hinkle Jason T. Mushotzky Richard \| MNRAS \| 506-4960 \| 2021 \| 2021MNRAS.506.4960H \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.506.4960H 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 Soft excess in AGN with relativistic Xu2011ray reflection \|Ezhikode Savithri H. Shyam Prakash V. P. et al. \| AN \| 344-20230042 \| 2023 \| 2023AN....34430042E \| http://ui.adsabs.harvard.edu/#abs/2023AN....34430042E Testing Physical Scenarios for the Reflection Features of Type-1 AGNs using XMM-Newton and NuSTAR Simultaneous Observations \|Victoria-Ceballos Cu00e9sar Ivan Gonzu00e1lez-Martu00edn Omaira et al. \| ApJ \| 954-96 \| 2023 \| 2023ApJ...954...96V \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...954...96V 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	2015-08-13T08:16:34Z/2015-08-16T04:56:57Z
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	2016-09-07T22:00:00Z
Last Update	2025-01-27
Keywords	"central black hole", "xmm newton", "broadened fwhm", "blackhole spin", "agn allows", "hard xray", "tentative detection", "xray lags", "mrk 1040", "hard xray excess", "inner disc", "60000 km", "accretion disk", "XMM-Newton", "NuSTAR", "soft xray", "disc reverberation scenarios", "xray spectral components", "XMM"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr James Reeves, 2016, 'A hard X-ray view of the inner disc in Mrk 1040', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-0f66iv9