A dataset provided by the European Space Agency

Name: The X-ray coolest gas in cool core clusters
Published: 2009-08-27T00:00:00Z

Proposal ID	055183
Title	The X-ray coolest gas in cool core clusters
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0551830101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0551830201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0551830301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0551830401
DOI	https://doi.org/10.5270/esa-maob1mr
Principal Investigator, PI	Dr Jeremy Sanders
Abstract	We propose to continue our programme of deep RGS observations by observing thenext best three clusters spanning a range of redshift, luminosity andtemperature in order to make definitive statements about the range oftemperature in the clusters and the level of cooling. All three clusters havecool cores, short central cooling times and central radio sources. The mainspectral target is the FeXVII emission lines at 15 and 17A, the ratio of whichdepends on the gas temperature in the 3-7 million K range. In the case of A1835we shall for the first time probe mass cooling rates similar to the observedstar formation rate. These observations will exploit the unique capability ofthe RGS, and build on one of XMM.s major discoveries.
Publications	A direct limit on the turbulent velocity of the intracluster medium in the core of Abell 1835 from XMM-Newton \|Sanders, J. S., Fabian, A. C., et al. \| MNRAS \| 402-11 \| 2010 \| 2010MNRAS.402L..11S \| http://ui.adsabs.harvard.edu/#abs/2010MNRAS.402L..11S An All-Sky Atlas of Radio/X-ray Associations \|Flesch, E., \| PASA \| 27-283 \| 2010 \| 2010PASA...27..283F \| http://ui.adsabs.harvard.edu/#abs/2010PASA...27..283F Luminous X-ray Active Galactic Nuclei in Clusters of Galaxies \|Koulouridis, E., Plionis, M., \| ApJ \| 714-181 \| 2010 \| 2010ApJ...714L.181K \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...714L.181K Exospheric solar wind charge exchange as seen by XMM-Newton \|Carter, J. A., Semba, S., \| AN \| 333-313 \| 2012 \| 2012AN....333..313C \| http://ui.adsabs.harvard.edu/#abs/2012AN....333..313C The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive \|Clerc, N., Sadibekova, T., et al. \| MNRAS \| 423-3561 \| 2012 \| 2012MNRAS.423.3561C \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.3561C Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog \|Lin, Dacheng, Webb, Natalie A., \| ApJ \| 756-27 \| 2012 \| 2012ApJ...756...27L \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...756...27L Deprojected analysis of Abell 1835 observed with Chandra and compared with XMM-Newton \|Li, C. K., Jia, S. M., et al. \| A&A \| 545-100 \| 2012 \| 2012A&A...545A.100L \| http://ui.adsabs.harvard.edu/#abs/2012A&A...545A.100L Ensemble X-ray variability of active galactic nuclei from serendipitous source catalogues \|Vagnetti, F., Turriziani, S., \| A&A \| 536-84 \| 2011 \| 2011A&A...536A..84V \| http://ui.adsabs.harvard.edu/#abs/2011A&A...536A..84V Properties of the integrated spectrum of serendipitous 2XMM catalog sources \|Chaudhary, P., 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 A systematic cross-search for radio/infrared counterparts of XMM- Newton sources \|Combi, J. A., Albacete Colombo, J. F., et al. \| Ap&SS \| 331-53 \| 2011 \| 2011Ap&SS.331...53C \| http://ui.adsabs.harvard.edu/#abs/2011Ap&SS.331...53C 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 Probing of the Interactions between the Hot Plasmas and Galaxies in Clusters from z = 0.1 to 0.9 \|Gu, Liyi, Gandhi, Poshak, et al. \| ApJ \| 767-157 \| 2013 \| 2013ApJ...767..157G \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...767..157G 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 The diversity of quasars unified by accretion and orientation \|Shen, Yue, Ho, Luis C., \| Natur \| 513-210 \| 2014 \| 2014Natur.513..210S \| http://ui.adsabs.harvard.edu/#abs/2014Natur.513..210S 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 New XMM-Newton observation of the Phoenix cluster: properties of the cool core \|Tozzi, P., Gastaldello, F., et al. \| A&A \| 580-6 \| 2015 \| 2015A&A...580A...6T \| http://ui.adsabs.harvard.edu/#abs/2015A&A...580A...6T LoCuSS: The Slow Quenching of Star Formation in Cluster Galaxies and the Need for Pre-processing \|Haines, C. P., Pereira, M. J., et al. \| ApJ \| 806-101 \| 2015 \| 2015ApJ...806..101H \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...806..101H Where do the 3.5 keV photons come from? A morphological study of the Galactic Center and of Perseus \|Carlson, Eric, Jeltema, Tesla, \| JCAP \| 2-9 \| 2015 \| 2015JCAP...02..009C \| http://ui.adsabs.harvard.edu/#abs/2015JCAP...02..009C A novel scenario for the possible X-ray line feature at virgul3.5 keV. Charge exchange with bare sulfur ions \|Gu, L., Kaastra, J., et al. \| A&A \| 584-11 \| 2015 \| 2015A&A...584L..11G \| http://ui.adsabs.harvard.edu/#abs/2015A&A...584L..11G 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 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 SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV \|Clerc, N., 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 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 Gas mass fractions from XMM-Newton \|Della Monica Ferreira, Desiree, \| PhDT \| 0-186 \| 2011 \| 2011PhDT.......186D \| http://ui.adsabs.harvard.edu/#abs/2011PhDT.......186D AGN spectral states from simultaneous UV and X-ray observations by XMM-Newton \|Svoboda, J., Guainazzi, M., \| A&A \| 603-127 \| 2017 \| 2017A&A...603A.127S \| http://ui.adsabs.harvard.edu/#abs/2017A&A...603A.127S LoCuSS: pre-processing in galaxy groups falling into massive galaxy clusters at z = 0.2 \|Bianconi, M., Smith, G. P., et al. \| MNRAS \| 473-79 \| 2018 \| 2018MNRAS.473L..79B \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.473L..79B X-Ray Lines from Dark Matter Annihilation at the keV Scale \|Brdar, Vedran, Kopp, Joachim, et al. \| PhRvL \| 120-61301 \| 2018 \| 2018PhRvL.120f1301B \| http://ui.adsabs.harvard.edu/#abs/2018PhRvL.120f1301B WIMP dark matter candidates and searches---current status and future prospects \|Roszkowski, Leszek, Sessolo, Enrico Maria, \| RPPh \| 81-66201 \| 2018 \| 2018RPPh...81f6201R \| http://ui.adsabs.harvard.edu/#abs/2018RPPh...81f6201R Resonantly Produced 7A keV Sterile Neutrino Dark Matter Models and the Properties of Milky Way Satellites \|Abazajian, Kevork N., \| PhRvL \| 112-161303 \| 2014 \| 2014PhRvL.112p1303A \| http://ui.adsabs.harvard.edu/#abs/2014PhRvL.112p1303A LoCuSS: The infall of X-ray groups on to massive clusters \|Haines, C. P., Finoguenov, A., et al. \| MNRAS \| 477-4931 \| 2018 \| 2018MNRAS.477.4931H \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.477.4931H Limits on turbulent propagation of energy in cool-core clusters of galaxies \|Bambic, C. J., Pinto, C., et al. \| MNRAS \| 478-44 \| 2018 \| 2018MNRAS.478L..44B \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.478L..44B LoCuSS: scaling relations between galaxy cluster mass, gas, and stellar content \|Mulroy, Sarah L., Farahi, Arya, et al. \| MNRAS \| 484-60 \| 2019 \| 2019MNRAS.484...60M \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.484...60M Laboratory Measurements of X-Ray Emission from Highly Charged Argon Ions \|Bulbul, Esra, Foster, Adam, et al. \| ApJ \| 870-21 \| 2019 \| 2019ApJ...870...21B \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...870...21B Searching for cool and cooling X-ray emitting gas in 45 galaxy clusters and groups \|Liu, Haonan, Pinto, Ciro, et al. \| MNRAS \| 485-1757 \| 2019 \| 2019MNRAS.485.1757L \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.485.1757L Detection of anti-correlation of hot and cold baryons in galaxy clusters \|Farahi, Arya, Mulroy, Sarah L., et al. \| NatCo \| 10-2504 \| 2019 \| 2019NatCo..10.2504F \| http://ui.adsabs.harvard.edu/#abs/2019NatCo..10.2504F X-ray properties of the X-CLASS-redMaPPer galaxy cluster sample: the luminosity-temperature relation \|Molham, Mona, Clerc, Nicolas, et al. \| MNRAS \| 494-161 \| 2020 \| 2020MNRAS.494..161M \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494..161M Multiwavelength classification of X-ray selected galaxy cluster candidates using convolutional neural networks \|Kosiba, Matej, Lieu, Maggie, et al. \| MNRAS \| 496-4141 \| 2020 \| 2020MNRAS.496.4141K \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.496.4141K The XMM Cluster Survey: new evidence for the 3.5-keV feature in clusters is inconsistent with a dark matter origin \|Bhargava, S., Giles, P. A., et al. \| MNRAS \| 497-656 \| 2020 \| 2020MNRAS.497..656B \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497..656B SPIDERS: overview of the X-ray galaxy cluster follow-up and the final spectroscopic data release \|Clerc, N., Kirkpatrick, C. C., et al. \| MNRAS \| 497-3976 \| 2020 \| 2020MNRAS.497.3976C \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497.3976C 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 Metastable conformal dark matter \|Brax, Philippe, Kaneta, Kunio, et al. \| PhRvD \| 103-115016 \| 2021 \| 2021PhRvD.103k5016B \| http://ui.adsabs.harvard.edu/#abs/2021PhRvD.103k5016B A Search for the 3.5 keV Line from the Milky Way.s Dark Matter Halo with HaloSat \|Silich, E. M., Jahoda, K., et al. \| ApJ \| 916-2 \| 2021 \| 2021ApJ...916....2S \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...916....2S 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 Scaling relations of X-ray luminous clusters in the Hyper Suprime-Cam Subaru Strategic Program field \|Poon, Helen, Okabe, Nobuhiro, et al. \| MNRAS \| 520-6001 \| 2023 \| 2023MNRAS.520.6001P \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.520.6001P Was There a 3.5 keV Line? \|Dessert, Christopher, Foster, Joshua W., et al. \| ApJ \| 964-185 \| 2024 \| 2024ApJ...964..185D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...964..185D 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 AGNs in massive galaxy clusters: Role of galaxy merging, infalling groups, cluster mass, and dynamical state \|Koulouridis, E., Gkini, A., \| A&A \| 684-A111 \| 2024 \| 2024A&A...684A.111K \| http://ui.adsabs.harvard.edu/#abs/2024A&A...684A.111K 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	2008-07-15T08:03:47Z/2008-07-26T18:09:57Z
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	2009-08-27T00:00:00Z
Keywords	"definitive statements", "XMM", "gas temperature", "star formation rate", "cluster spanning", "fexvii emission lines", "central radio sources", "cool cores", "deep rgs", "cool core clusters", "major discoveries", "xray coolest gas", "short central cooling", "main spectral target"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Jeremy Sanders, 2009, 'The X-ray coolest gas in cool core clusters', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-maob1mr