A dataset provided by the European Space Agency

Name: REFLECTION SPECTROSCOPY OF THE SEYFERT 1.5 AGN ESO 362-G18
Published: 2017-10-17T22:00:00Z

Proposal ID	079081
Title	REFLECTION SPECTROSCOPY OF THE SEYFERT 1.5 AGN ESO 362-G18
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0790810101
DOI	https://doi.org/10.5270/esa-sxfpnvg
Principal Investigator, PI	Dr JAVIER ADOLFO GARCIA
Abstract	We propose simultaneous 100 ks XMM-Newton and NuSTAR observations of the Seyfert1.5 galaxy ESO 362-G18 for the purpose of making a detailed study of thespectrum of radiation reflected from the inner accretion disk. Our chief aim isto constrain both the spin of the black hole and the properties of the coronathat illuminates the disk. The combination of NuSTARa??s high-sensitivity in thehard X-ray band, the soft-band coverage of XMM-Newton, and our state-of-the-artrelativistic reflection models will allow us to break degeneracies betweendifferent possible scenarios, and impose tight constraints on the accretiongeometry and black hole spin of this bright AGN.
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 The Nature of Soft Excess in ESO 362-G18 Revealed by XMM-Newton and NuSTAR Spectroscopy \|Xu, Yerong, Garc\\u00eda, Javier A., et al. \| ApJ \| 913-13 \| 2021 \| 2021ApJ...913...13X \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...913...13X 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 X-Ray Coronal Properties of Swift/BAT-selected Seyfert 1 Active Galactic Nuclei \|Kamraj, Nikita, Brightman, Murray, et al. \| ApJ \| 927-42 \| 2022 \| 2022ApJ...927...42K \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...927...42K The Origin of The Soft X-Ray Excess in the Seyfert 1.5 Galaxy ESO 362-G18 \|Zhong, Xiao-Gu, Wang, Jian-Cheng, \| RAA \| 22-35002 \| 2022 \| 2022RAA....22c5002Z \| http://ui.adsabs.harvard.edu/#abs/2022RAA....22c5002Z 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 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	2016-09-24T19:39:21Z/2016-09-26T05:12:41Z
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	2017-10-17T22:00:00Z
Keywords	"NuSTAR", "G18.", "XMM", "inner accretion disk", "xmm newton", "reflection spectroscopy", "break degeneracies", "bright agn", "soft band coverage", "accretion geometry", "XMM-Newton", "blackhole spin", "radiation reflected", "hard xray band", "impose tight constraints"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr JAVIER ADOLFO GARCIA, 2017, 'REFLECTION SPECTROSCOPY OF THE SEYFERT 1.5 AGN ESO 362-G18', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-sxfpnvg