A dataset provided by the European Space Agency

Name 020336
Title EVOLUTION OF AGN IN THE COSMIC WEB: THE HST+VIMOS+SWIRE COSMOS FIELD
URL

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DOI 10.5270/esa-o7ynu4m
Author Prof GUENTHER HASINGER
Description We propose a mosaic of medium-deep XMM pointings to homogeneously cover a large (2 deg**2) and contiguous area of the COSMOS-VIMOS field. This field is (1) part of a breakthrough spectroscopic survey carried out using the French-Italian VIMOS consortium.s 70 nights of guaranteed VLT time, to provide redshifts for all the objects with I_AB<24, and (2) target of the Cosmos HST-ACS treasury program, carried out using 640 HST orbits, to understand the interplay between Large Scale Structure, evolution and the formation of galaxies, Dark Matter - Energy and AGN. The main scientific objectives are the study of the formation and evolution of supermassive black holes, the cosmic evolution of their spatial distribution and the correlation with galaxy morphology and evolution.
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Studying the X-ray-UV Variability of Active Galactic Nuclei with data from Swift and XMM archives . Turriziani, Sara, . JPhCS . 280-12005 . 2011 . ...,
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Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras . Mateos, S., Saxton, R. D., et all. . A&A . 496-879 . 2009 . 2009A&A...496..879M ,
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Fe K emission from active galaxies in the COSMOS field . Iwasawa, K., Mainieri, V., et all. . A&A . 537-86 . 2012 . 2012A&A...537A..86I ,
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High-Redshift Quasars in the COSMOS Survey: The Space Density of z > 3 X-Ray Selected QSOs . Brusa, M., Comastri, A., et all. . ApJ . 693-8 . 2009 . 2009ApJ...693....8B ,
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Photometric Redshift and Classification for the XMM-COSMOS Sources . Salvato, M., Hasinger, G., et all. . ApJ . 690-1250 . 2009 . 2009ApJ...690.1250S ,
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The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive . Clerc, N., Sadibekova, T., et all. . MNRAS . 423-3561 . 2012 . 2012MNRAS.423.3561C ,
Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog . Lin, Dacheng, Webb, Natalie A., . ApJ . 756-27 . 2012 . 2012ApJ...756...27L ,
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The X-ray luminous galaxies optically classified as star forming are mostly narrow line Seyfert 1 s . Castello-Mor, N., Barcons, X., et all. . A&A . 544-48 . 2012 . 2012A&A...544A..48C ,
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Using the Bright Ultrahard XMM-Newton survey to define an IR selection of luminous AGN based on WISE colours . Mateos, S., Alonso-Herrero, A., et all. . MNRAS . 426-3271 . 2012 . 2012MNRAS.426.3271M ,
Black hole accretion and host galaxies of obscured quasars in XMM-COSMOS . Mainieri, V., Bongiorno, A., et all. . A&A . 535-80 . 2011 . 2011A&A...535A..80M ,
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A systematic cross-search for radio-infrared counterparts of XMM- Newton sources . Combi, J. A., Albacete Colombo, J. F., et all. . Ap&SS . 331-53 . 2011 . 2011Ap&SS.331...53C ,
Exploring X-ray and radio emission of type 1 AGN up to z ~ 2.3 . Ballo, L., Heras, F. J. H., et all. . A&A . 545-66 . 2012 . 2012A&A...545A..66B ,
The HETDEX Pilot Survey. I. Survey Design, Performance, and Catalog of Emission-line Galaxies . Adams, Joshua J., Blanc, Guillermo A., et all. . ApJS . 192-5 . 2011 . 2011ApJS..192....5A ,
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Uncovering obscured luminous AGN with WISE . Mateos, S., Alonso-Herrero, A., et all. . MNRAS . 434-941 . 2013 . 2013MNRAS.434..941M ,
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AGN host galaxy mass function in COSMOS. Is AGN feedback responsible for the mass-quenching of galaxies? . Bongiorno, A., Schulze, A., et all. . A&A . 588-78 . 2016 . 2016A&A...588A..78B ,
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The 2QDES Pilot: the luminosity and redshift dependence of quasar clustering . Chehade, Ben, Shanks, T., et all. . MNRAS . 459-1179 . 2016 . 2016MNRAS.459.1179C ,
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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 ,
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Instrument EPN, RGS1, OM, RGS2, EMOS1, EMOS2
Temporal Coverage 2003-12-06T01:35:03Z/2005-05-15T00:37:42Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 2008-01-05T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2008-01-05T00:00:00Z, 020336, 17.56_20190403_1200. https://doi.org/10.5270/esa-o7ynu4m