A dataset provided by the European Space Agency

Name: SDSS J110012.38+084616.3: A Compton-thick or X-ray weak AGNquestionMark
Published: 2013-01-31T00:00:00Z

Proposal ID	067436
Title	SDSS J110012.38+084616.3: A Compton-thick or X-ray weak AGN?
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674360101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674360201
DOI	https://doi.org/10.5270/esa-kzv5s0m
Principal Investigator, PI	Dr Silvia Mateos
Abstract	The space density of the most powerful absorbed AGN (QSO2) and theircontribution to the AGN luminosity output remains uncertain. Many of theseobjects are severely attenuated, so hard X-ray surveys alone do not fully provethe bulk of the obscured QSO population in the nearby Universe. We propose a 80ksec XMM-Newton observation of an optically selected QSO2 at zvirgul0.1. Comparingits OIII and 2-10 keV luminosities the source is likely a Compton-thick AGN.However, the X-ray spectral analysis seems to indicate that it might be insteadCompton thin and X-ray weak. The proposed observations will allow us to unveilthe true nature of this source and will give us key information on whetherobjects such as this are intrinsically different to the QSO2 population detected in hard X-ray surveys.
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 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	2011-12-21T15:02:18Z/2011-12-22T16:06:53Z
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	2013-01-31T00:00:00Z
Keywords	"space density", "SDSS", "xray spectral analysis", "compton thick agn", "XMM", "compton thin", "sdss j110012", "qso2 population", "hard xray surveys", "obscured qso population", "kev luminosities", "key information", "nearby universe", "compton thick", "XMM-Newton", "agn luminosity output", "xray weak", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Silvia Mateos, 2013, 'SDSS J110012.38+084616.3: A Compton-thick or X-ray weak AGNquestionMark', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-kzv5s0m