A dataset provided by the European Space Agency

Name: XMM-Newton Observations of Two Possibly Compton-thick, Low Redshift ERO Sources
Published: 2010-06-02T00:00:00Z

Proposal ID	060284
Title	XMM-Newton Observations of Two Possibly Compton-thick, Low Redshift ERO Sources
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0602840101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0602840201
DOI	https://doi.org/10.5270/esa-tp4jdm5
Principal Investigator, PI	Dr Lisa Winter
Abstract	The Swift BAT (14-195 keV) X-ray survey has currently identified a sample of 250nearby (z=0.03) AGN. Among these, two sources have very unusual multi wavelengthproperties which have strong implications for understanding similar sourcesdetected in deep surveys. In the optical, NVSS 193013+341047 and IRAS 05218-1212show broad lines, while their XRT spectra suggest these sources are heavilyabsorbed and possibly Compton-thick. Further, the IR properties of these sourcesplace them among the most heavily extincted with unusual SED, comparable only tohigh redshift ERO. With 15 ks XMM EPIC observations of both unusual sources, wewill constrain the X-ray properties of these sources, trying to determine theorigin of this unusual (at high flux) behavior.
Publications	The Swift BAT Survey Detects Two Optical Broad Line X-Ray Heavily Obscured Active Galaxies: NVSS 193013+341047 and IRAS 05218-1212 \|Hogg J. Drew Winter Lisa M. et al. \| ApJ \| 752-153 \| 2012 \| 2012ApJ...752..153H \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...752..153H An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities \|Henley David B. Shelton Robin L. \| ApJS \| 202-14 \| 2012 \| 2012ApJS..202...14H \| http://ui.adsabs.harvard.edu/#abs/2012ApJS..202...14H 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 The Interaction of the Fermi Bubbles with the Milky Ways Hot Gas Halo \|Miller Matthew J. Bregman Joel N. \| ApJ \| 829-9 \| 2016 \| 2016ApJ...829....9M \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...829....9M 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 Broadband X-Ray Spectrum of the X-Ray-obscured Type 1 AGN 2MASX J193013.80+341049.5 \|Kamraj Nikita Balokoviu0107 Mislav et al. \| ApJ \| 887-255 \| 2019 \| 2019ApJ...887..255K \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...887..255K An X-Ray- and SZ-bright Diffuse Source toward M31: A Local Hot Bridge \|Qu Zhijie Huang Rui et al. \| ApJ \| 907-14 \| 2021 \| 2021ApJ...907...14Q \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...907...14Q 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 Solar Cycle Temporal Variation of the Solar Wind Charge Exchange X-Ray Lines \|Qu Zhijie Koutroumpa Dimitra et al. \| ApJ \| 930-21 \| 2022 \| 2022ApJ...930...21Q \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...930...21Q 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	2009-05-16T16:28:25Z/2009-05-16T22:42:44Z
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	2010-06-02T00:00:00Z
Last Update	2025-01-27
Keywords	"redshift ero", "broad lines", "ir properties", "xmm newton", "nvss 193013", "xmm epic", "multi wavelength properties", "03 agn", "EPIC", "swift bat", "XMM-Newton", "xray properties", "deep surveys", "heavily extincted", "xrt spectra", "compton thick", "heavily absorbed", "iras 05218 1212", "XMM", "nearby z"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Lisa Winter, 2010, 'XMM-Newton Observations of Two Possibly Compton-thick, Low Redshift ERO Sources', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-tp4jdm5