A dataset provided by the European Space Agency

Name: Obscured AGN beyond the local Universe
Published: 2009-06-10T00:00:00Z

Proposal ID	050206
Title	Obscured AGN beyond the local Universe
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502060101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502060201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502060301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502060401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502060901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502061001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502061101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502061601
DOI	https://doi.org/10.5270/esa-mge3rfg
Principal Investigator, PI	Dr Alessandra Lamastra
Abstract	We propose to observe with XMM-Newton, for a total of 310 ks, the Bian et al.(2006) subsample of type 2 AGN at zvirgul0.3-0.4 for which they could estimatelambda=L_{bol}/L_{Edd}, with the aim to: a) Confirm, by means of a more directestimate of L_{bol} based on X-rays rather than on LO III, as Bian et al. did,that the sources have mostly lambdavirgul1, and check whether the super-Eddingtonsources did really exist or are an artifact due to the uncertainties in the LOIII-L_{bol} relationship. b) Determine the fraction of Compton-thick AGN atzvirgul0.3-0.4, high Eddington ratios, and high luminosities, to be compared withmeasurements based on local, low luminosities samples to search for correlationbetween obscuration and both the Eddington ratio and the luminosity.
Publications	X-ray Emission from Optically Selected Radio-intermediate and Radio-loud Quasars \|Miller, B. P., Brandt, W. N., et al. \| ApJ \| 726-20 \| 2011 \| 2011ApJ...726...20M \| http://ui.adsabs.harvard.edu/#abs/2011ApJ...726...20M The XMM Cluster Survey: optical analysis methodology and the first data release \|Mehrtens, Nicola, Romer, A. Kathy, et al. \| MNRAS \| 423-1024 \| 2012 \| 2012MNRAS.423.1024M \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.1024M The bolometric luminosity of type 2 AGN from extinction-corrected OIII. No evidence of Eddington-limited sources \|Lamastra, A., Bianchi, S., et al. \| A&A \| 504-73 \| 2009 \| 2009A&A...504...73L \| http://ui.adsabs.harvard.edu/#abs/2009A&A...504...73L The XMM Cluster Survey: X-ray analysis methodology \|Lloyd-Davies, E. J., Romer, A. Kathy, et al. \| MNRAS \| 418-14 \| 2011 \| 2011MNRAS.418...14L \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.418...14L Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog \|Lin, Dacheng, Webb, Natalie A., \| ApJ \| 756-27 \| 2012 \| 2012ApJ...756...27L \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...756...27L 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 Ensemble X-ray variability of active galactic nuclei from serendipitous source catalogues \|Vagnetti, F., Turriziani, S., \| A&A \| 536-84 \| 2011 \| 2011A&A...536A..84V \| http://ui.adsabs.harvard.edu/#abs/2011A&A...536A..84V An Archival Chandra and XMM-Newton Survey of Type 2 Quasars \|Jia, Jianjun, Ptak, Andrew, et al. \| ApJ \| 777-27 \| 2013 \| 2013ApJ...777...27J \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...777...27J The XMM-Newton view of the radio-loud narrow-line Seyfert 1 galaxy PMN J0948+0022 \|Bhattacharyya, Subir, Bhatt, Himali, et al. \| MNRAS \| 440-106 \| 2014 \| 2014MNRAS.440..106B \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.440..106B The 2XMMi/SDSS Galaxy Cluster Survey. III. Clusters associated with spectroscopically targeted luminous red galaxies in SDSS-DR10 \|Takey, A., Schwope, A., \| A&A \| 564-54 \| 2014 \| 2014A&A...564A..54T \| http://ui.adsabs.harvard.edu/#abs/2014A&A...564A..54T Delving Into X-ray Obscuration of Type 2 AGN, Near and Far \|LaMassa, Stephanie M., Yaqoob, Tahir, et al. \| ApJ \| 787-61 \| 2014 \| 2014ApJ...787...61L \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...787...61L The diversity of quasars unified by accretion and orientation \|Shen, Yue, Ho, Luis C., \| Natur \| 513-210 \| 2014 \| 2014Natur.513..210S \| http://ui.adsabs.harvard.edu/#abs/2014Natur.513..210S 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 Properties of flat-spectrum radio-loud narrow-line Seyfert 1 galaxies \|Foschini, L., Berton, M., et al. \| A&A \| 575-13 \| 2015 \| 2015A&A...575A..13F \| http://ui.adsabs.harvard.edu/#abs/2015A&A...575A..13F Sunyaev-Zel.dovich effect or not? Detecting the main foreground effect of most galaxy clusters \|Xiao, Weike, Chen, Chen, et al. \| MNRAS \| 432-41 \| 2013 \| 2013MNRAS.432L..41X \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.432L..41X NuSTAR Reveals Extreme Absorption in z < 0.5 Type 2 Quasars \|Lansbury, G. B., Gandhi, P., et al. \| ApJ \| 809-115 \| 2015 \| 2015ApJ...809..115L \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...809..115L XMM-Newton publication statistics \|Ness, J.-U., Parmar, A. N., et al. \| AN \| 335-210 \| 2014 \| 2014AN....335..210N \| http://ui.adsabs.harvard.edu/#abs/2014AN....335..210N The Tight Relation between X-Ray and Ultraviolet Luminosity of Quasars \|Lusso, E., Risaliti, G., \| ApJ \| 819-154 \| 2016 \| 2016ApJ...819..154L \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...819..154L Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function \|Vagnetti, F., Middei, R., et al. \| A&A \| 593-55 \| 2016 \| 2016A&A...593A..55V \| http://ui.adsabs.harvard.edu/#abs/2016A&A...593A..55V The Interaction of the Fermi Bubbles with the Milky Way.s 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 A new sample of X-ray selected narrow emission-line galaxies. II. Looking for True Seyfert 2 \|Pons, E., Watson, M. G., \| A&A \| 594-72 \| 2016 \| 2016A&A...594A..72P \| http://ui.adsabs.harvard.edu/#abs/2016A&A...594A..72P Dependence of the broad Fe Kalpha line on the physical parameters of AGN \|Liu, Zhu, Yuan, Weimin, et al. \| MNRAS \| 463-684 \| 2016 \| 2016MNRAS.463..684L \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.463..684L AGN spectral states from simultaneous UV and X-ray observations by XMM-Newton \|Svoboda, J., Guainazzi, M., \| A&A \| 603-127 \| 2017 \| 2017A&A...603A.127S \| http://ui.adsabs.harvard.edu/#abs/2017A&A...603A.127S Anisotropy of the galaxy cluster X-ray luminosity-temperature relation \|Migkas, Konstantinos, Reiprich, Thomas H., \| A&A \| 611-50 \| 2018 \| 2018A&A...611A..50M \| http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..50M The XMM Cluster Survey: Present status and latest results \|Viana, P. T. P., Mehrtens, N., et al. \| AN \| 334-462 \| 2013 \| 2013AN....334..462V \| http://ui.adsabs.harvard.edu/#abs/2013AN....334..462V Obscured Active Galactic Nuclei \|Hickox, Ryan C., Alexander, David M., \| ARA&A \| 56-625 \| 2018 \| 2018ARA&A..56..625H \| http://ui.adsabs.harvard.edu/#abs/2018ARA&A..56..625H Testing emergent gravity on galaxy cluster scales \|Tamosiunas, Andrius, Bacon, David, et al. \| JCAP \| 5-53 \| 2019 \| 2019JCAP...05..053T \| http://ui.adsabs.harvard.edu/#abs/2019JCAP...05..053T Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline \|Hollowood, Devon L., Jeltema, Tesla, et al. \| ApJS \| 244-22 \| 2019 \| 2019ApJS..244...22H \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..244...22H Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters \|Palmese, A., Annis, J., et al. \| MNRAS \| 493-4591 \| 2020 \| 2020MNRAS.493.4591P \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.4591P 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 A Luminous X-Ray Transient in SDSS J143359.16+400636.0: A Likely Tidal Disruption Event \|Brightman, Murray, Ward, Charlotte, et al. \| ApJ \| 909-102 \| 2021 \| 2021ApJ...909..102B \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...909..102B The composite X-ray spectra of radio-loud and radio-quiet SDSS quasars \|Zhou, Min-Hua, Gu, Min-Feng, \| RAA \| 21-4 \| 2021 \| 2021RAA....21....4Z \| http://ui.adsabs.harvard.edu/#abs/2021RAA....21....4Z 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 X-ray emission from a rapidly accreting narrow-line Seyfert 1 galaxy at z = 6.56 \|Wolf, J., Nandra, K., et al. \| A&A \| 669-127 \| 2023 \| 2023A&A...669A.127W \| http://ui.adsabs.harvard.edu/#abs/2023A&A...669A.127W Probing the Origin of Changing-look Quasar Transitions with Chandra \|Yang, Qian, Green, Paul J., et al. \| ApJ \| 953-61 \| 2023 \| 2023ApJ...953...61Y \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...953...61Y 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	2007-07-11T06:24:11Z/2008-04-30T00:09:01Z
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	2009-06-10T00:00:00Z
Keywords	"", "eddington ratio", "obscured agn", "low luminosities samples", "compton thick agn", "XMM", "local universe", "bol }/ l_", "iii ]", "eddington ratios", "edd }", "XMM-Newton", "2006 subsample", "super eddington sources", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Alessandra Lamastra, 2009, 'Obscured AGN beyond the local Universe', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-mge3rfg