A dataset provided by the European Space Agency

Name: X-ray and FHIL emission lines as a geometry probe: The case of Mrk 359
Published: 2011-08-17T00:00:00Z

Proposal ID	065559
Title	X-ray and FHIL emission lines as a geometry probe: The case of Mrk 359
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655590201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655590501
DOI	https://doi.org/10.5270/esa-mhp4wwg
Principal Investigator, PI	Mr Rob Detmers
Abstract	We propose a multi-wavelength campaign to observe the Narrow-line Seyfert 1(NLS1) AGN Mrk 359, both with XMM-textit{Newton} RGS and VLT X-shooter toinvestigate the detailed X-ray and optical properties of a strong forbidden highionization line (FHIL hereafter) source, and probe the connection of the X-rayemission lines with the optical FHILs. With this observation we will obtainaccurate flux measurements of the emission lines as well as accurate velocityshifts. We will use these to constrain the density profile and geometry of theX-ray narrow-line region (NLR) and the optical FHIL emitting gas.
Publications	Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov V. N. \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y A hard X-ray view of the soft excess in AGN \|Boissay Rozenn Ricci Claudio \| A&A \| 588-70 \| 2016 \| 2016A&A...588A..70B \| http://ui.adsabs.harvard.edu/#abs/2016A&A...588A..70B Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function \|Vagnetti F. Middei R. et al. \| A&A \| 593-55 \| 2016 \| 2016A&A...593A..55V \| http://ui.adsabs.harvard.edu/#abs/2016A&A...593A..55V The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch Eric W. \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F Are narrow-line Seyfert 1 galaxies highly accreting low-MBH AGNs? \|Williams James K. Gliozzi Mario \| MNRAS \| 480-96 \| 2018 \| 2018MNRAS.480...96W \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.480...96W The soft X-ray excess: NLS1s versus BLS1s \|Gliozzi Mario Williams James K. \| MNRAS \| 491-532 \| 2020 \| 2020MNRAS.491..532G \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.491..532G 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 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2010-07-25T02:41:38Z/2010-07-30T15:47:17Z
Version	PPS_NOT_AVAILABLE
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	2011-08-17T00:00:00Z
Last Update	2025-01-27
Keywords	"emission lines", "geometry probe", "optical fhils", "xray emission lines", "fhil emission lines", "velocity shifts", "x ray", "vlt x shooter", "narrow line seyfert", "xmm textit", "XMM", "optical properties", "flux measurements", "density profile", "multi wavelength campaign", "mrk 359"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mr Rob Detmers, 2011, 'X-ray and FHIL emission lines as a geometry probe: The case of Mrk 359', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-mhp4wwg