A dataset provided by the European Space Agency

Name: X-raying strong gravitational lenses: dark halos and the environment
Published: 2011-05-07T00:00:00Z

Proposal ID	060234
Title	X-raying strong gravitational lenses: dark halos and the environment
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0602340101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0602340201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0602340301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0602340401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0602340701
DOI	https://doi.org/10.5270/esa-j52iyra
Principal Investigator, PI	Prof Tommaso Treu
Abstract	The SLACS collaboration measured the dark matter halos of elliptical galaxies onscales from 1 to 100 kpc, using a combination of lensing (strong and weak) andstellar dynamics. This provides new tests of the standard cosmological models atgalaxy/group scales. However, lensing can only measure the total projected massalong the line of sight, and therefore can be affected by large-scale structuresin projection. We propose to observe a complete subset of SLACS lenses toidentify nearby groups and clusters, determine their location, temperature, andmass 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.
Publications	The Atacama Cosmology Telescope: Physical Properties of Sunyaev-Zel.dovich Effect Clusters on the Celestial Equator \|Menanteau, Felipe, Sifon, Cristobal, et al. \| ApJ \| 765-67 \| 2013 \| 2013ApJ...765...67M \| http://ui.adsabs.harvard.edu/#abs/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 \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y Reaching the peak of the quasar spectral energy distribution - I. Observations and models \|Collinson, James S., Ward, Martin J., et al. \| MNRAS \| 449-2174 \| 2015 \| 2015MNRAS.449.2174C \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.449.2174C 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 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 \| http://ui.adsabs.harvard.edu/#abs/2016A&C....16..174M 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 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 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 al. \| MNRAS \| 465-358 \| 2017 \| 2017MNRAS.465..358C \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.465..358C 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 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 X-Ray spectra of AGN.s with strong emission lines \|Tugay, A. V., Vasylenko, A. A., \| AstSR \| 8-160 \| 2012 \| 2012AstSR...8..160T \| http://ui.adsabs.harvard.edu/#abs/2012AstSR...8..160T 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 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 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	2009-11-15T03:39:17Z/2010-04-15T22:48:58Z
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	2011-05-07T00:00:00Z
Keywords	"tidal interactions", "low redshift average", "xray investigation", "lens sample", "halo profiles", "stellar dynamics", "slacs lenses", "total projected mass", "gravitational lens", "elliptical galaxy", "dark matter halos", "slacs collaboration", "SLACS", "standard cosmological models", "x raying", "scale structures", "dark halos", "complete subset"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Tommaso Treu, 2011, 'X-raying strong gravitational lenses: dark halos and the environment', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-j52iyra