A dataset provided by the European Space Agency

Name: Finding Compton-thick AGN Among the Faintest Swift BAT Sources
Published: 2019-04-21T22:00:00Z

Proposal ID	080283
Title	Finding Compton-thick AGN Among the Faintest Swift BAT Sources
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0802830101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0802830201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0802830301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0802830401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0802830501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0802830601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0802830801
DOI	https://doi.org/10.5270/esa-to2716x
Principal Investigator, PI	Dr Michael Koss
Abstract	We propose short XMM-Newton observations of 8 sources newly detected in thedeepest Swift-BAT 104- month stacked all-sky maps, but for which a Swift XRTobservation has detected no X-ray counterpart. Our past studies of these faintBAT sources found some of the brightest examples of reflection-dominated AGNavailable across the sky with accretion rates several times higher than typicalAGN that contribute significantly to black hole growth in the nearby universe.XMM-Newton is critical to identify these sources because of the factor of >10xhigher sensitivity than Swift XRT combined with a very large FOV (28.4arcsec) toresolve any contributing sources associated with Swift BAT detection(FWHM=22.5arcmin).
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 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	2017-04-25T08:59:50Z/2018-03-29T07:29:53Z
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	2019-04-21T22:00:00Z
Keywords	"accretion rates", "reflection dominated agn", "short xmm newton", "XMM", "blackhole growth", "swift xrt combined", "faint bat sources", "xray counterpart", "nearby universe", "sky maps", "XMM-Newton", "swift xrt", "brightest examples", "typical agn", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Michael Koss, 2019, 'Finding Compton-thick AGN Among the Faintest Swift BAT Sources', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-to2716x