A dataset provided by the European Space Agency

Name: Tomography of the innermost regions of NGC 985
Published: 2016-02-13T23:00:00Z

Proposal ID	074383
Title	Tomography of the innermost regions of NGC 985
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743830501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743830601
DOI	https://doi.org/10.5270/esa-z22g1tf
Principal Investigator, PI	Dr Jacobo Ebrero
Abstract	AGN mass outflows inject enormous amounts of matter and energy into theinterstellar medium of the host galaxy. Their location, structure, andimportance as contributors to cosmic feedback processes are not yet fullyunderstood. We propose to observe the Seyfert 1 galaxy NGC 985 with XMM-Newtonfor 240 ks using RGS as the prime instrument in order to accurately characterizethe different ionized phases and kinematic components of the warm absorber.Together with HST/COS we will study the connection between the X-ray and UVabsorbers and put stringent limits on the location of these winds in the contextof the unification model of AGN.
Publications	Discovery of a fast broad transient outflow in NGC 985 \|Ebrero J. Kriss G. A. et al. \| A&A \| 586-72 \| 2016 \| 2016A&A...586A..72E \| http://ui.adsabs.harvard.edu/#abs/2016A&A...586A..72E An X-ray view of central engines of low-luminosity quasars (LLQSO) in the local Universe \|Laha Sibasish Ghosh Ritesh et al. \| MNRAS \| 480-1522 \| 2018 \| 2018MNRAS.480.1522L \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.480.1522L 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 Multi-epoch properties of the warm absorber in the Seyfert 1 galaxy NGC 985 \|Ebrero J. Domu010dek V. et al. \| A&A \| 653-125 \| 2021 \| 2021A&A...653A.125E \| http://ui.adsabs.harvard.edu/#abs/2021A&A...653A.125E 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 Xu2011HESS: A large sample of highly accreting serendipitous AGN under the XMMu2011Newton microscope \|Laurenti M. Tombesi F. et al. \| AN \| 344-20230053 \| 2023 \| 2023AN....34430053L \| http://ui.adsabs.harvard.edu/#abs/2023AN....34430053L 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 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	2015-01-13T09:35:34Z/2015-01-26T18:24:16Z
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	2016-02-13T23:00:00Z
Last Update	2025-01-27
Keywords	"ionized phases", "unification model", "HST", "interstellar medium", "xmm newton", "stringent limits", "warm absorber", "XMM-Newton", "prime instrument", "kinematic components", "ngc 985", "galaxy ngc 985", "innermost region", "XMM", "uv absorbers", "NGC 985", "cosmic feedback processes"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Jacobo Ebrero, 2016, 'Tomography of the innermost regions of NGC 985', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-z22g1tf