A dataset provided by the European Space Agency

Name 008324
Title Groups and clusters near multiply lensed QSOs
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0083240201

DOI 10.5270/esa-9std489
Author Dr Jens Hjorth
Description Gravitationally lensed QSOs are powerful tools for measuring cosmological parameters if their lens potentials can be adequately constrained. Groups and clusters of galaxies close to the line of sight to multiply lensed QSOs contribute significantly to the potential. Such collapsed mass concentrations can be traced by X-rays. We here propose to map the mass distribution around four well-constrained quadruple lenses with 0.3 < z < 0.8 and predicted temperatures 1 keV < kT < 6 keV. The primary aim of these observations will be to constrain the mass models of the lenses, to study the low-mass end of scaling relations relating mass to X-ray observables and finaly to put constrains on the Hubble constant and the cosmological constant.
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The XMM-Newton EPIC background: Production of background maps and event files . Read, A. M., Ponman, T. J., . A&A . 409-395 . 2003 . 2003A&A...409..395R ,
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Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . 2012AN....333..313C ,
Detectability of low-energy X-ray spectral components in type 1 active galactic nuclei . Scott, A. E., Stewart, G. C., . MNRAS . 423-2633 . 2012 . 2012MNRAS.423.2633S ,
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 ,
The XMM-Newton serendipitous ultraviolet source survey catalogue . Page, M. J., Brindle, C., et all. . MNRAS . 426-903 . 2012 . 2012MNRAS.426..903P ,
The stellar content of the XMM-Newton bright serendipitous survey . Lopez-Santiago, J., Micela, G., et all. . A&A . 463-165 . 2007 . 2007A&A...463..165L ,
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A statistical relation between the X-ray spectral index and Eddington ratio of active galactic nuclei in deep surveys . Brightman, M., Silverman, J. D., et all. . MNRAS . 433-2485 . 2013 . 2013MNRAS.433.2485B ,
Structure and substructure analysis of DAFT-FADA galaxy clusters in the [0.4-0.9] redshift range . Guennou, L., Adami, C., et all. . A&A . 561-112 . 2014 . 2014A&A...561A.112G ,
Automatic Classification of Time-variable X-Ray Sources . Lo, Kitty K., Farrell, Sean, et all. . ApJ . 786-20 . 2014 . 2014ApJ...786...20L ,
Confirming the thermal Comptonization model for black hole X-ray emission in the low-hard state . Castro, M., D.Amico, F., et all. . A&A . 569-82 . 2014 . 2014A&A...569A..82C ,
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Swift follow-up of IceCube triggers, and implications for the Advanced-LIGO era . Evans, P. A., Osborne, J. P., et all. . MNRAS . 448-2210 . 2015 . 2015MNRAS.448.2210E ,
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The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Studying Cosmic Evolution with the XMM-Newton Distant Cluster Project: X-ray Luminous Galaxy Clusters at z>~1 and their Galaxy Populations . Fassbender, Rene, . PhDT . 0-116 . 2008 . 2008PhDT.......116F ,
Anisotropy of the galaxy cluster X-ray luminosity-temperature relation . Migkas, Konstantinos, Reiprich, Thomas H., . A&A . 611-50 . 2018 . 2018A&A...611A..50M ,
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The evolving X-ray spectrum of active galactic nuclei: Evidence for an increasing reflection fraction with redshift . Avirett-Mackenzie, M. S., Ballantyne, D. R., . MNRAS . 486-3488 . 2019 . 2019MNRAS.486.3488A ,
Testing emergent gravity on galaxy cluster scales . Tamosiunas, Andrius, Bacon, David, et all. . JCAP . 5-53 . 2019 . 2019JCAP...05..053T ,
Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline . Hollowood, Devon L., Jeltema, Tesla, et all. . ApJS . 244-22 . 2019 . 2019ApJS..244...22H ,
Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters . Palmese, A., Annis, J., et all. . MNRAS . 493-4591 . 2020 . 2020MNRAS.493.4591P ,
X-ray properties of the X-CLASS-redMaPPer galaxy cluster sample: the luminosity-temperature relation . Molham, Mona, Clerc, Nicolas, et all. . MNRAS . 494-161 . 2020 . 2020MNRAS.494..161M ,
Accretion History of AGNs. II. Constraints on AGN Spectral Parameters Using the Cosmic X-Ray Background . Ananna, Tonima Tasnim, Treister, Ezequiel, et all. . ApJ . 889-17 . 2020 . 2020ApJ...889...17A ,
Multiwavelength classification of X-ray selected galaxy cluster candidates using convolutional neural networks . Kosiba, Matej, Lieu, Maggie, et all. . MNRAS . 496-4141 . 2020 . 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 all. . MNRAS . 497-3976 . 2020 . 2020MNRAS.497.3976C ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2001-11-02T02:01:20Z/2001-11-02T07:45:46Z
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 2002-11-23T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2002-11-23T00:00:00Z, 008324, 17.56_20190403_1200. https://doi.org/10.5270/esa-9std489