A dataset provided by the European Space Agency

Name: Mass and entropy in the most dynamically disturbed REXCESS clusters
Published: 2012-05-04T00:00:00Z

Proposal ID	065444
Title	Mass and entropy in the most dynamically disturbed REXCESS clusters
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0654440101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0654440201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0654440401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0654440501
DOI	https://doi.org/10.5270/esa-q9zaj1f
Principal Investigator, PI	Dr Gabriel Pratt
Abstract	We propose to re-observe the four most morphologically disturbed clusters in theREXCESS sample. Our aim is to measure the temperature at R_500 and improve thespatial resolution of the temperature profiles in the flat surface brightnesscentral regions, in order to have measurements of similar quality to thatavailable for relaxed systems. With these data we will precisely measure the HEmass profiles, to test the hypothesis that unrelaxed systems have lessconcentrated mass distributions, a critical test of the dark matter collapse. Wewill also dramatically improve measurements of the entropy in the centralregions, to provide a critical benchmark for numerical simulations.
Publications	Confirming the thermal Comptonization model for black hole X-ray emission in the low-hard state \|Castro, M., D.Amico, F., et al. \| A&A \| 569-82 \| 2014 \| 2014A&A...569A..82C \| http://ui.adsabs.harvard.edu/#abs/2014A&A...569A..82C 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 The XMM spectral catalog of SDSS optically selected Seyfert 2 galaxies \|Koulouridis, E., Georgantopoulos, I., et al. \| A&A \| 586-3 \| 2016 \| 2016A&A...586A...3K \| http://ui.adsabs.harvard.edu/#abs/2016A&A...586A...3K 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 The SAMI Pilot Survey: the kinematic morphology-density relation in Abell 85, Abell 168 and Abell 2399 \|Fogarty, L. M. R., Scott, Nicholas, et al. \| MNRAS \| 443-485 \| 2014 \| 2014MNRAS.443..485F \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.443..485F 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 Connecting optical and X-ray tracers of galaxy cluster relaxation \|Roberts, Ian D., Parker, Laura C., \| MNRAS \| 475-4704 \| 2018 \| 2018MNRAS.475.4704R \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.475.4704R The cool-core state of Planck SZ-selected clusters versus X-ray-selected samples: evidence for cool-core bias \|Rossetti, M., Gastaldello, F., et al. \| MNRAS \| 468-1917 \| 2017 \| 2017MNRAS.468.1917R \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.468.1917R The non-uniformity of galaxy cluster metallicity profiles \|Lovisari, L., Reiprich, T. H., \| MNRAS \| 483-540 \| 2019 \| 2019MNRAS.483..540L \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483..540L High entropy and evidence for a merger in the low surface brightness cluster Abell 2399 \|Mitsuishi, Ikuyuki, Babazaki, Yasunori, et al. \| PASJ \| 70-112 \| 2018 \| 2018PASJ...70..112M \| http://ui.adsabs.harvard.edu/#abs/2018PASJ...70..112M Probing cosmic isotropy with a new X-ray galaxy cluster sample through the LX-T scaling relation \|Migkas, K., Schellenberger, G., et al. \| A&A \| 636-15 \| 2020 \| 2020A&A...636A..15M \| http://ui.adsabs.harvard.edu/#abs/2020A&A...636A..15M The dynamical state of Abell 2399: a bullet-like cluster \|Louren\\u00e7o, Ana C. C., Lopes, P. A. A., et al. \| MNRAS \| 498-835 \| 2020 \| 2020MNRAS.498..835L \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.498..835L 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 On the Reliability of Photometric and Spectroscopic Tracers of Halo Relaxation \|Zhoolideh Haghighi, Mohammad H., Raouf, Mojtaba, et al. \| ApJ \| 904-36 \| 2020 \| 2020ApJ...904...36Z \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...904...36Z 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 Cosmological implications of the anisotropy of ten galaxy cluster scaling relations \|Migkas, K., Pacaud, F., et al. \| A&A \| 649-151 \| 2021 \| 2021A&A...649A.151M \| http://ui.adsabs.harvard.edu/#abs/2021A&A...649A.151M 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	2010-05-12T07:36:57Z/2011-04-10T21:51:15Z
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	2012-05-04T00:00:00Z
Keywords	"temperature profiles", "unrelaxed systems", "mass profiles", "numerical simulations", "relaxed systems", "central region", "dark matter collapse", "spatial resolution", "concentrated mass distributions", "rexcess sample", "morphologically disturbed cluster"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Gabriel Pratt, 2012, 'Mass and entropy in the most dynamically disturbed REXCESS clusters', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-q9zaj1f