A dataset provided by the European Space Agency

Name 060234
Title X-raying strong gravitational lenses: dark halos and the environment
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0602340101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0602340201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0602340301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0602340401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0602340701

DOI 10.5270/esa-j52iyra
Author Prof Tommaso Treu
Description The SLACS collaboration measured the dark matter halos of elliptical galaxies on scales from 1 to 100 kpc, using a combination of lensing (strong and weak) and stellar dynamics. This provides new tests of the standard cosmological models at galaxy-group scales. However, lensing can only measure the total projected mass along the line of sight, and therefore can be affected by large-scale structures in projection. We propose to observe a complete subset of SLACS lenses to identify nearby groups and clusters, determine their location, temperature, and mass and study the dependency of halo profiles on the local environment, expected because of tidal interactions. The selected low redshift (average 0.13) lens sample is ideal for an X-ray investigation at galaxy-group scales.
Publication The Atacama Cosmology Telescope: Physical Properties of Sunyaev-Zel.dovich Effect Clusters on the Celestial Equator . Menanteau, Felipe, Sifon, Cristobal, et all. . ApJ . 765-67 . 2013 . 2013ApJ...765...67M ,
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 ,
Reaching the peak of the quasar spectral energy distribution - I. Observations and models . Collinson, James S., Ward, Martin J., et all. . MNRAS . 449-2174 . 2015 . 2015MNRAS.449.2174C ,
XMM-Newton publication statistics . Ness, J.-U., Parmar, A. N., et all. . AN . 335-210 . 2014 . 2014AN....335..210N ,
Spectral clustering for optical confirmation and redshift estimation of X-ray selected galaxy cluster candidates in the SDSS Stripe 82 . Mahmoud, E., Takey, A., . A&C . 16-174 . 2016 . 2016A&C....16..174M ,
Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function . Vagnetti, F., Middei, R., et all. . A&A . 593-55 . 2016 . 2016A&A...593A..55V ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 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 . ...,
Dependence of the broad Fe Kalpha line on the physical parameters of AGN . Liu, Zhu, Yuan, Weimin, et all. . MNRAS . 463-684 . 2016 . 2016MNRAS.463..684L ,
Reaching the peak of the quasar spectral energy distribution - II. Exploring the accretion disc, dusty torus and host galaxy . Collinson, James S., Ward, Martin J., et all. . MNRAS . 465-358 . 2017 . 2017MNRAS.465..358C ,
A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies . Ojha, Vineet, Chand, Hum, et all. . ApJ . 896-95 . 2020 . 2020ApJ...896...95O ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2009-11-15T03:39:17Z/2010-04-15T22:48:58Z
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 2011-05-07T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2011-05-07T00:00:00Z, 060234, 17.56_20190403_1200. https://doi.org/10.5270/esa-j52iyra