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 X\\u2011ray 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, C\\u00e9sar Ivan, Gonz\\u00e1lez-Mart\\u00edn, 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
Keywords	"hard xray", "NuSTAR", "inner disc", "60000 km", "disc reverberation scenarios", "xray spectral components", "XMM-Newton", "tentative detection", "xmm newton", "accretion disk", "blackhole spin", "hard xray excess", "XMM", "soft xray", "mrk 1040", "broadened fwhm", "xray lags", "agn allows", "central black hole"
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