A dataset provided by the European Space Agency

Name: MCG-03-58-007: a new powerful inner accretion disk wind
Published: 2016-12-22T23:00:00Z

Proposal ID	076401
Title	MCG-03-58-007: a new powerful inner accretion disk wind
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0764010101
DOI	https://doi.org/10.5270/esa-29a0x8x
Principal Investigator, PI	Dr Valentina Braito
Abstract	We request deep (130ks) simultaneous XMM-Newton and NuSTAR observations of thenew powerful disk wind detected in the Seyfert2 MCG-03-58-007 (Fxvirgul2x10^-12cgsz=0.0315). A Suzaku observation revealed a deep absorption trough at 7.5-9 keV,possibly associated with the presence of a high column density (NHvirgul4x10^23cm-2),highly ionized absorber outflowing at vvirgul0.1c, strongly resembling the case ofPDS456. We ask for a simultaneous observation with NuSTAR to perform a detailedspectral analysis and derive the location and energetics of this wind. Byexploiting the combined high-quality X-ray spectroscopic capabilities andbroad-band spectral coverage of the XMM-Newton and NuSTAR data we will constrainthe underlying continuum and thus better investigate the profile of the absorption features.
Publications	A new powerful and highly variable disc wind in an AGN-star-forming galaxy, the case of MCG-03-58-007 \|Braito, V., Reeves, J. N., et al. \| MNRAS \| 479-3592 \| 2018 \| 2018MNRAS.479.3592B \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.479.3592B Evidence for a clumpy disc-wind in the star-forming Seyfert 2 galaxy MCG-03-58-007 \|Matzeu, G. A., Braito, V., et al. \| MNRAS \| 483-2836 \| 2019 \| 2019MNRAS.483.2836M \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483.2836M The stratified disc wind of MCG-03-58-007 \|Braito, V., Reeves, J. N., et al. \| MNRAS \| 500-291 \| 2021 \| 2021MNRAS.500..291B \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.500..291B 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 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	2015-12-06T12:15:42Z/2015-12-08T01:34:02Z
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	2016-12-22T23:00:00Z
Keywords	"mcg 03", "NuSTAR", "007 fx", "XMM", "column density nh", "xmm newton", "spectral analysis", "deep 130", "ionized absorber outflowing", "XMM-Newton", "seyfert2 mcg 03", "deep absorption trough", "powerful disk wind", "nustar data", "quality xray spectroscopic", "12cgs z"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Valentina Braito, 2016, 'MCG-03-58-007: a new powerful inner accretion disk wind', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-29a0x8x