A dataset provided by the European Space Agency

Name: The Thermal Structure of Distant Cooling Flows
Published: 2003-09-04T00:00:00Z

Proposal ID	010867
Title	The Thermal Structure of Distant Cooling Flows
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0108670101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0108670201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0108670401
DOI	https://doi.org/10.5270/esa-zzpm2ht
Principal Investigator, PI	Dr Richard Mushotzky
Abstract	GT- RGS spectra are required to distinguish two- or three-temperature plasmasfrom true multi-phase media in cooling flow clusters. We propose to observe twovery massive cooling flows at redshift about one-quarter -- sufficiently distantso that the highly peaked cooling flow region inside 200 kpc appearsapproximately point-like to the XMM mirrors. 50 ksec XMM exposures of theseobjects yield >15-20 line photons for 15-25 features,thus enabling the thermalstructure to be disentangled.
Publications	Exploring the X-ray sky with the XMM-Newton bright serendipitous survey \|Della Ceca R. Maccacaro T. et al. \| A&A \| 428-383 \| 2004 \| 2004A&A...428..383D \| http://ui.adsabs.harvard.edu/#abs/2004A&A...428..383D The XMM-Newton Needles in the Haystack Survey: the local X-ray luminosity function of normal galaxies \|Georgantopoulos I. Georgakakis A. \| MNRAS \| 360-782 \| 2005 \| 2005MNRAS.360..782G \| http://ui.adsabs.harvard.edu/#abs/2005MNRAS.360..782G ARCRAIDER. I. Detailed optical and X-ray analysis of the cooling flow cluster Z3146 \|Kausch W. Gitti M. et al. \| A&A \| 471-31 \| 2007 \| 2007A&A...471...31K \| http://ui.adsabs.harvard.edu/#abs/2007A&A...471...31K High-precision multi-band measurements of the angular clustering of X-ray sources \|Ebrero J. Mateos S. et al. \| A&A \| 500-749 \| 2009 \| 2009A&A...500..749E \| http://ui.adsabs.harvard.edu/#abs/2009A&A...500..749E The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue \|Watson M. G. Schroder A. C. et al. \| A&A \| 493-339 \| 2009 \| 2009A&A...493..339W \| http://ui.adsabs.harvard.edu/#abs/2009A&A...493..339W An Extremely Luminous Panchromatic Outburst from the Nucleus of a Distant Galaxy \|Levan A. J. Tanvir N. R. et al. \| Sci \| 333-199 \| 2011 \| 2011Sci...333..199L \| http://ui.adsabs.harvard.edu/#abs/2011Sci...333..199L New constraints on the X-ray spectral properties of type 1 active galactic nuclei \|Scott A. E. Stewart G. C. et al. \| MNRAS \| 417-992 \| 2011 \| 2011MNRAS.417..992S \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.417..992S The x-ray luminous galaxy cluster population at 0.9 < z ≲ 1.6 as revealed by the XMM-Newton Distant Cluster Project \|Fassbender R. Bohringer H. et al. \| NJPh \| 13-125014 \| 2011 \| 2011NJPh...13l5014F \| http://ui.adsabs.harvard.edu/#abs/2011NJPh...13l5014F Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras \|Mateos S. Saxton R. D. et al. \| A&A \| 496-879 \| 2009 \| 2009A&A...496..879M \| http://ui.adsabs.harvard.edu/#abs/2009A&A...496..879M The XMM Cluster Survey: optical analysis methodology and the first data release \|Mehrtens Nicola Romer A. Kathy et al. \| MNRAS \| 423-1024 \| 2012 \| 2012MNRAS.423.1024M \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.1024M LoCuSS: A Comparison of Cluster Mass Measurements from XMM-Newton and Subaru---Testing Deviation from Hydrostatic Equilibrium and Non-thermal Pressure Support \|Zhang Yu-Ying Okabe Nobuhiro et al. \| ApJ \| 711-1033 \| 2010 \| 2010ApJ...711.1033Z \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...711.1033Z The Axis Ratio Distribution of X-ray Clusters Observed by XMM-Newton \|Kawahara Hajime \| ApJ \| 719-1926 \| 2010 \| 2010ApJ...719.1926K \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...719.1926K LoCuSS: Calibrating Mass-observable Scaling Relations for Cluster Cosmology with Subaru Weak-lensing Observations \|Okabe N. Zhang Y.-Y. et al. \| ApJ \| 721-875 \| 2010 \| 2010ApJ...721..875O \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...721..875O Mass profiles and c-MDM relation in X-ray luminous galaxy clusters \|Ettori S. Gastaldello F. et al. \| A&A \| 524-68 \| 2010 \| 2010A&A...524A..68E \| http://ui.adsabs.harvard.edu/#abs/2010A&A...524A..68E BLOX: the Bonn lensing optical and X-ray selected galaxy clusters. I. Cluster catalog construction \|Dietrich J. P. Erben T. et al. \| A&A \| 470-821 \| 2007 \| 2007A&A...470..821D \| http://ui.adsabs.harvard.edu/#abs/2007A&A...470..821D A catalog of galaxy clusters observed by XMM-Newton \|Snowden S. L. Mushotzky R. F. et al. \| A&A \| 478-615 \| 2008 \| 2008A&A...478..615S \| http://ui.adsabs.harvard.edu/#abs/2008A&A...478..615S LoCuSS: comparison of observed X-ray and lensing galaxy cluster scaling relations with simulations \|Zhang Y.-Y. Finoguenov A. et al. \| A&A \| 482-451 \| 2008 \| 2008A&A...482..451Z \| http://ui.adsabs.harvard.edu/#abs/2008A&A...482..451Z Radial temperature profiles for a large sample of galaxy clusters observed with XMM-Newton \|Leccardi A. Molendi S. \| A&A \| 486-359 \| 2008 \| 2008A&A...486..359L \| http://ui.adsabs.harvard.edu/#abs/2008A&A...486..359L Radial metallicity profiles for a large sample of galaxy clusters observed with XMM-Newton \|Leccardi A. Molendi S. \| A&A \| 487-461 \| 2008 \| 2008A&A...487..461L \| http://ui.adsabs.harvard.edu/#abs/2008A&A...487..461L High precision X-ray log N - log S distributions: implications for the obscured AGN population \|Mateos S. Warwick R. S. et al. \| A&A \| 492-51 \| 2008 \| 2008A&A...492...51M \| http://ui.adsabs.harvard.edu/#abs/2008A&A...492...51M Star Formation Rates in Cooling Flow Clusters: A UV Pilot Study with Archival XMM-Newton Optical Monitor Data \|Hicks A. K. Mushotzky R. \| ApJ \| 635-9 \| 2005 \| 2005ApJ...635L...9H \| http://ui.adsabs.harvard.edu/#abs/2005ApJ...635L...9H Characterizing the Properties of Clusters of Galaxies as a Function of Luminosity and Redshift \|Andersson K. Peterson J. R. et al. \| ApJ \| 696-1029 \| 2009 \| 2009ApJ...696.1029A \| http://ui.adsabs.harvard.edu/#abs/2009ApJ...696.1029A The XMM-Newton serendipitous survey. VI. The X-ray luminosity function \|Ebrero J. Carrera F. J. et al. \| A&A \| 493-55 \| 2009 \| 2009A&A...493...55E \| http://ui.adsabs.harvard.edu/#abs/2009A&A...493...55E Breaking the sigma8-Omega m Degeneracy Using the Clustering of High-z X-ray Active Galactic Nuclei \|Basilakos Spyros Plionis Manolis \| ApJ \| 714-185 \| 2010 \| 2010ApJ...714L.185B \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...714L.185B The X-ray spectral properties of the AGN population in the XMM-Newton bright serendipitous survey \|Corral A. Della Ceca R. et al. \| A&A \| 530-42 \| 2011 \| 2011A&A...530A..42C \| http://ui.adsabs.harvard.edu/#abs/2011A&A...530A..42C An XMM-Newton Survey of the Soft X-ray Background. I. The O VII and O VIII Lines Between l = 120 and l = 240 \|Henley David B. Shelton Robin L. \| ApJS \| 187-388 \| 2010 \| 2010ApJS..187..388H \| http://ui.adsabs.harvard.edu/#abs/2010ApJS..187..388H Constraints on turbulent velocity broadening for a sample of clusters groups and elliptical galaxies using XMM-Newton \|Sanders J. S. Fabian A. C. \| MNRAS \| 410-1797 \| 2011 \| 2011MNRAS.410.1797S \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.410.1797S Revealing O VII from stacked X-ray grating spectra of clusters groups and elliptical galaxies \|Sanders J. S. Fabian A. 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Brusa M. et al. \| A&A \| 518-58 \| 2010 \| 2010A&A...518A..58C \| http://ui.adsabs.harvard.edu/#abs/2010A&A...518A..58C Rest-frame stacking of 2XMM catalog sources. Properties of the Fe Kalpha line \|Chaudhary P. Brusa M. et al. \| A&A \| 537-6 \| 2012 \| 2012A&A...537A...6C \| http://ui.adsabs.harvard.edu/#abs/2012A&A...537A...6C 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 al. \| MNRAS \| 426-3271 \| 2012 \| 2012MNRAS.426.3271M \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.426.3271M Cross-correlation of the 2XMMi catalogue with Data Release 7 of the Sloan Digital Sky Survey \|Pineau F.-X. Motch C. et al. \| A&A \| 527-126 \| 2011 \| 2011A&A...527A.126P \| http://ui.adsabs.harvard.edu/#abs/2011A&A...527A.126P Exploring X-ray and radio emission of type 1 AGN up to z ~ 2.3 \|Ballo L. Heras F. J. H. et al. \| A&A \| 545-66 \| 2012 \| 2012A&A...545A..66B \| http://ui.adsabs.harvard.edu/#abs/2012A&A...545A..66B The XMM-Newton serendipitous source catalogue \|Watson M. G. Pye J. P. et al. \| AN \| 324-89 \| 2003 \| 2003AN....324...89W \| http://ui.adsabs.harvard.edu/#abs/2003AN....324...89W The 2-8 keV cosmic X-ray background spectrum as observed with XMM-Newton \|De Luca A. Molendi S. \| A&A \| 419-837 \| 2004 \| 2004A&A...419..837D \| http://ui.adsabs.harvard.edu/#abs/2004A&A...419..837D Velocity width measurements of the coolest X-ray emitting material in the cores of clusters groups and elliptical galaxies \|Sanders J. S. Fabian A. C. \| MNRAS \| 429-2727 \| 2013 \| 2013MNRAS.429.2727S \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.429.2727S Planck intermediate results. III. The relation between galaxy cluster mass and Sunyaev-Zeldovich signal \|Planck Collaboration Ade P. A. R. et al. \| A&A \| 550-129 \| 2013 \| 2013A&A...550A.129P \| http://ui.adsabs.harvard.edu/#abs/2013A&A...550A.129P Joint Analysis of Cluster Observations. II. Chandra/XMM-Newton X-Ray and Weak Lensing Scaling Relations for a Sample of 50 Rich Clusters of Galaxies \|Mahdavi Andisheh Hoekstra Henk et al. \| ApJ \| 767-116 \| 2013 \| 2013ApJ...767..116M \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...767..116M Uncovering obscured luminous AGN with WISE \|Mateos S. Alonso-Herrero A. et al. \| MNRAS \| 434-941 \| 2013 \| 2013MNRAS.434..941M \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.434..941M Automatic Classification of Time-variable X-Ray Sources \|Lo Kitty K. Farrell Sean et al. \| ApJ \| 786-20 \| 2014 \| 2014ApJ...786...20L \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...786...20L Detection of an Unidentified Emission Line in the Stacked X-Ray Spectrum of Galaxy Clusters \|Bulbul Esra Markevitch Maxim et al. \| ApJ \| 789-13 \| 2014 \| 2014ApJ...789...13B \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...789...13B LoCuSS: hydrostatic mass measurements of the high-LX cluster sample - cross-calibration of Chandra and XMM-Newton \|Martino Rossella Mazzotta Pasquale et al. \| MNRAS \| 443-2342 \| 2014 \| 2014MNRAS.443.2342M \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.443.2342M 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 Relativistic Fe Kalpha line revealed in the composite X-ray spectrum of narrow-line Seyfert 1 galaxies - do their black holes have averagely low or intermediate spins? \|Liu Zhu Yuan Weimin et al. \| MNRAS \| 447-517 \| 2015 \| 2015MNRAS.447..517L \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.447..517L X-ray spectral and variability properties of low-mass active galactic nuclei \|Ludlam R. M. Cackett E. M. et al. \| MNRAS \| 447-2112 \| 2015 \| 2015MNRAS.447.2112L \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.447.2112L Obscuration-dependent Evolution of Active Galactic Nuclei \|Buchner Johannes Georgakakis Antonis et al. \| ApJ \| 802-89 \| 2015 \| 2015ApJ...802...89B \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...802...89B Revisiting the relationship between 6 mum and 2-10 keV continuum luminosities of AGN \|Mateos S. Carrera F. 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Merloni A. et al. \| MNRAS \| 463-4490 \| 2016 \| 2016MNRAS.463.4490C \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.463.4490C 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 The XMM Cluster Survey: the halo occupation number of BOSS galaxies in X-ray clusters \|Mehrtens Nicola Romer A. Kathy et al. \| MNRAS \| 463-1929 \| 2016 \| 2016MNRAS.463.1929M \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.463.1929M A new sample of X-ray selected narrow emission-line galaxies. II. Looking for True Seyfert 2 \|Pons E. Watson M. 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Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2000-12-05T14:31:17Z/2002-08-03T19:36:00Z
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	2003-09-04T00:00:00Z
Last Update	2025-01-27
Keywords	"temperature plasmas", "xmm mirrors", "distant cooling flows", "appears approximately", "cooling flow clusters", "line photons", "rgs spectra", "massive cooling flows", "thermal structure", "XMM", "multi phase media"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Richard Mushotzky, 2003, 'The Thermal Structure of Distant Cooling Flows', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-zzpm2ht