A dataset provided by the European Space Agency

Name: Understanding the X-ray source population through an XMM survey of ELAIS fields
Published: 2005-01-01T00:00:00Z

Proposal ID	005975
Title	Understanding the X-ray source population through an XMM survey of ELAIS fields
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0059750101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0059750201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0059750301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0059750401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0059750501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0059751801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0059752001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0059752301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0059752401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0059752501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0059752601 ... https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0059752801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0059753001
DOI	https://doi.org/10.5270/esa-5f255cw
Principal Investigator, PI	Dr Robert Mann
Abstract	We request 450ks, to survey with EPIC 3 sq. deg. we mapped with ISO at 7, 15,90 and 175 microns, and followed up in the optical, near-IR and radio, to give:(i) a sample of virgul1000 X-ray galaxies, allowing selection of statisticallyrepresentative subsamples of galaxies by activity Seyfert 1, Seyfert 2,starburst, by X-ray luminosity and by degree of obscuration;(ii) X-ray spectral information for a large sample of galaxies for which there is excellent multi-wavelength data from the radio to the UV;(iii) the best opportunity of resolving, through direct IR to X-ray comparisons,the issue of dust extinction in AGN, and of determining the contributions ofstarbursts and dust-obscured AGN to the cosmic far-infrared background.
Publications	The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue \|Watson, M. G., Schroder, A. C., et al. \| A&A \| 493-339 \| 2009 \| 2009A&A...493..339W \| http://ui.adsabs.harvard.edu/#abs/2009A&A...493..339W Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras \|Mateos, S., Saxton, R. D., et al. \| A&A \| 496-879 \| 2009 \| 2009A&A...496..879M \| http://ui.adsabs.harvard.edu/#abs/2009A&A...496..879M 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 XMM-Newton spectroscopy of high-redshift quasars \|Page, K. L., Reeves, J. N., et al. \| MNRAS \| 364-195 \| 2005 \| 2005MNRAS.364..195P \| http://ui.adsabs.harvard.edu/#abs/2005MNRAS.364..195P The X-Ray Properties of Active Galactic Nuclei with Double-peaked Balmer Lines \|Strateva, Iskra V., Brandt, W. N., et al. \| ApJ \| 651-749 \| 2006 \| 2006ApJ...651..749S \| http://ui.adsabs.harvard.edu/#abs/2006ApJ...651..749S Exploratory Study of the X-Ray Properties of Quasars with Intrinsic Narrow Absorption Lines \|Misawa, Toru, Eracleous, Michael, et al. \| ApJ \| 677-863 \| 2008 \| 2008ApJ...677..863M \| http://ui.adsabs.harvard.edu/#abs/2008ApJ...677..863M A serendipitous XMM survey of the SDSS: the evolution of the colour-magnitude diagram of X-ray AGN from z= 0.8 to 0.1 \|Georgakakis, Antonis, Nandra, K., \| MNRAS \| 414-992 \| 2011 \| 2011MNRAS.414..992G \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.414..992G An All-Sky Atlas of Radio/X-ray Associations \|Flesch, E., \| PASA \| 27-283 \| 2010 \| 2010PASA...27..283F \| http://ui.adsabs.harvard.edu/#abs/2010PASA...27..283F 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 The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive \|Clerc, N., Sadibekova, T., et al. \| MNRAS \| 423-3561 \| 2012 \| 2012MNRAS.423.3561C \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.3561C The XMM-Newton serendipitous ultraviolet source survey catalogue \|Page, M. J., Brindle, C., et al. \| MNRAS \| 426-903 \| 2012 \| 2012MNRAS.426..903P \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.426..903P Cross-correlation of the 2XMMi catalogue with Data Release 7 of the Sloan Digital Sky Survey \|Pineau, F.-X., Motch, C., et al. \| A&A \| 527-126 \| 2011 \| 2011A&A...527A.126P \| http://ui.adsabs.harvard.edu/#abs/2011A&A...527A.126P Exploring X-ray and radio emission of type 1 AGN up to z virgul 2.3 \|Ballo, L., Heras, F. J. H., et al. \| A&A \| 545-66 \| 2012 \| 2012A&A...545A..66B \| http://ui.adsabs.harvard.edu/#abs/2012A&A...545A..66B 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 Obscuration-dependent Evolution of Active Galactic Nuclei \|Buchner, Johannes, Georgakakis, Antonis, et al. \| ApJ \| 802-89 \| 2015 \| 2015ApJ...802...89B \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...802...89B 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 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 XMM Cluster Survey: evolution of the velocity dispersion-temperature relation over half a Hubble time \|Wilson, Susan, Hilton, Matt, et al. \| MNRAS \| 463-413 \| 2016 \| 2016MNRAS.463..413W \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.463..413W SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV \|Clerc, N., Merloni, A., et al. \| MNRAS \| 463-4490 \| 2016 \| 2016MNRAS.463.4490C \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.463.4490C 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 M Dwarf Activity in the Pan-STARRS1 Medium-Deep Survey: First Catalog and Rotation Periods \|Kado-Fong, E., Williams, P. K. G., et al. \| ApJ \| 833-281 \| 2016 \| 2016ApJ...833..281K \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...833..281K Searching for gamma-ray signature in WHSP blazars. Fermi-LAT detection of 150 excess signal in the 0.3-500 GeV band \|Arsioli, B., Chang, Y.-L., \| A&A \| 598-134 \| 2017 \| 2017A&A...598A.134A \| http://ui.adsabs.harvard.edu/#abs/2017A&A...598A.134A 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 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 X-ray properties of high-richness CAMIRA clusters in the Hyper Suprime-Cam Subaru Strategic Program field \|Ota, Naomi, Mitsuishi, Ikuyuki, et al. \| PASJ \| 72-1 \| 2020 \| 2020PASJ...72....1O \| http://ui.adsabs.harvard.edu/#abs/2020PASJ...72....1O X-ray properties of the X-CLASS-redMaPPer galaxy cluster sample: the luminosity-temperature relation \|Molham, Mona, Clerc, Nicolas, et al. \| MNRAS \| 494-161 \| 2020 \| 2020MNRAS.494..161M \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494..161M A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies \|Ojha, Vineet, Chand, Hum, et al. \| ApJ \| 896-95 \| 2020 \| 2020ApJ...896...95O \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...896...95O Multiwavelength classification of X-ray selected galaxy cluster candidates using convolutional neural networks \|Kosiba, Matej, Lieu, Maggie, et al. \| MNRAS \| 496-4141 \| 2020 \| 2020MNRAS.496.4141K \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.496.4141K SPIDERS: overview of the X-ray galaxy cluster follow-up and the final spectroscopic data release \|Clerc, N., Kirkpatrick, C. C., et al. \| MNRAS \| 497-3976 \| 2020 \| 2020MNRAS.497.3976C \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497.3976C 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 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	2002-04-11T18:47:07Z/2002-10-28T14:26:24Z
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	2005-01-01T00:00:00Z
Keywords	"", "xray luminosity", "infrared background", "XMM", "xmm survey", "multi wavelength data", "dust obscured agn", "dust extinction", "elais fields", "xray galaxy", "175 microns", "EPIC", "xray comparisons", "starburst ]", "xray source population"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Robert Mann, 2005, 'Understanding the X-ray source population through an XMM survey of ELAIS fields', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-5f255cw