A dataset provided by the European Space Agency

Name: IRAS 18325-5926: A Seyfert 2 displaying unusual spectral characteristics
Published: 2014-10-30T00:00:00Z

Proposal ID	072482
Title	IRAS 18325-5926: A Seyfert 2 displaying unusual spectral characteristics
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724820101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724820201
DOI	https://doi.org/10.5270/esa-3egt725
Principal Investigator, PI	Mr Andrew Lobban
Abstract	IRAS 18325-5926 is a type-2 Seyfert galaxy displaying unusual spectralproperties; namely a broad Fe line perhaps originating primarily from He-likeFe, ionised warm-absorber features and a moderately low absorption column ofcold matter. It also exhibits significant and rapid X-ray variability. However,this source has been somewhat overlooked and the only existing XMM-Newtonobservation suffered from severe technical problems. Through a new 150ksexposure with XMM-Newton we aim to constrain the true nature and origin of thebroad Fe line, confirm the presence of outflowing ionised absorption, test forsoft X-ray reflection features from an ionised accretion disc and probe thevariability of the continuum, iron line and warm absorber on both short and long timescales.
Publications	X-ray time delays from the Seyfert 2 galaxy IRAS 18325-5926 \|Lobban, A. P., Alston, W. N., \| MNRAS \| 445-3229 \| 2014 \| 2014MNRAS.445.3229L \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.445.3229L 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 The Variable and Non-variable X-Ray Absorbers in Compton-thin Type II Active Galactic Nuclei \|Laha, Sibasish, Markowitz, Alex G., et al. \| ApJ \| 897-66 \| 2020 \| 2020ApJ...897...66L \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...897...66L 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 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2013-09-04T04:10:39Z/2013-10-16T22:30:03Z
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	2014-10-30T00:00:00Z
Keywords	"seyfert galaxy displaying", "rapid xray variability", "warm absorber", "XMM", "spectral characteristics", "iron line", "iras 18325 5926", "broad fe line", "existing xmm newton", "cold matter", "XMM-Newton", "soft xray reflection", "outflowing ionised absorption", "spectral properties", "ionised accretion disc", "ionised warm absorber", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mr Andrew Lobban, 2014, 'IRAS 18325-5926: A Seyfert 2 displaying unusual spectral characteristics', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-3egt725