A dataset provided by the European Space Agency

Name: Starburst-AGN relation in two nearby galaxies with low luminosity AGN
Published: 2016-12-01T23:00:00Z

Proposal ID	076350
Title	Starburst-AGN relation in two nearby galaxies with low luminosity AGN
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763500201
DOI	https://doi.org/10.5270/esa-oqzkbm3
Principal Investigator, PI	Ms Laura Tomas
Abstract	We propose to study two nearby face-on galaxies, NGC1097 and NGC1566, whichpresent circumnuclear star-forming and un-obscured AGN activity (Sy1), whoseX-ray emission can be separated with XMM-Newton. Data available in otherwavelenghts, combined with our X-ray data, will aid to characterize theAGN-starburst connection in these galaxies, which can help in disentangling bothtypes of activity in objects at farther distances. Hard X-ray emission is asignature of AGN activity, while soft X-ray emission is attributed to hot plasmaheated by mechanical energy released by stellar winds and supernovae. XMM-Newtondata are key for this, as quality spectra can be obtained for the nucleus andcircumnuclear rings and the AGN and starburst contributions can be characterized.
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 Broad-band X-ray observations of the 2018 outburst of the changing-look active galactic nucleus NGC 1566 \|Jana Arghajit Kumari Neeraj et al. \| MNRAS \| 507-687 \| 2021 \| 2021MNRAS.507..687J \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.507..687J AstroSat View of Spectral Transition in the Changing-look Active Galaxy NGC 1566 during the Declining Phase of the 2018 Outburst \|Tripathi Prakash Dewangan Gulab C. \| ApJ \| 925-101 \| 2022 \| 2022ApJ...925..101T \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...925..101T Response of the Fe Ku03b1 line emission to the X-ray continuum variability in the changing-look active galactic nucleus NGC 1566 \|Liang W. C. Shu X. W. et al. \| JHEAp \| 33-20 \| 2022 \| 2022JHEAp..33...20L \| http://ui.adsabs.harvard.edu/#abs/2022JHEAp..33...20L Coevolution of Broad Emission Lines and X-Ray Spectrum in Changing-look AGNs \|Liu Hao Wu Qingwen \| ApJ \| 930-46 \| 2022 \| 2022ApJ...930...46L \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...930...46L The changing-look AGN NGC 1566 in quiescence with XMM-Newton: a nuclear starburst and an AGN competing in power? \|Tomu00e1s L. Matzeu G. A. et al. \| MNRAS \| 514-403 \| 2022 \| 2022MNRAS.514..403T \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.514..403T 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 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 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 New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2015-11-05T01:49:16Z/2015-11-06T03:20:56Z
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	2016-12-01T23:00:00Z
Last Update	2025-08-04
Keywords	"xmm newton data", "hard xray emission", "NGC1097", "circumnuclear star forming", "mechanical energy released", "farther distances", "xray emission", "starburst agn relation", "XMM", "agn activity", "xray data", "stellar winds", "soft xray emission", "agn starburst connection", "hot plasma heated", "circumnuclear rings", "xmm newton", "quality spectra", "XMM-Newton", "starburst contributions", "low luminosity agn"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Ms Laura Tomas, 2016, 'Starburst-AGN relation in two nearby galaxies with low luminosity AGN', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-oqzkbm3