Clusters of galaxies are excellent laboratories for the study of the nucleosynthesis and chemical enrichment history of the Universe. These studies are currently biased toward relatively cooler (2-4 keV) clusters. However, the enrichment history of the massive hot clusters might be different from that of the smaller and cooler systems. Therefore, we propose to enlarge the sample of clusters observed with the RGS on XMM-Newton with Abell 2029, a hot luminous massive cluster with a cooling core. Despite of the high mass of this system, the cool gas in the core will allow us to measure the abundances of many elements. A deep (130 ks) observation will provide us with EPIC and RGS spectra of excellent statistics, which allows us to accurately measure the abundances O, Ne, Mg, Si, S, Ar, Ca, Fe, and Ni.
Publication
Planck early results. XI. Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations . Planck Collaboration, Ade, P. A. R., et all. . A&A . 536-11 . 2011 . 2011A&A...536A..11P , Star Formation Efficiency in the Cool Cores of Galaxy Clusters . McDonald, Michael, Veilleux, Sylvain, et all. . ApJ . 734-95 . 2011 . 2011ApJ...734...95M , Cold fronts in galaxy clusters . Ghizzardi, S., Rossetti, M., . A&A . 516-32 . 2010 . 2010A&A...516A..32G , Inhomogeneous metal distribution in the intracluster medium . Lovisari, L., Schindler, S., . A&A . 528-60 . 2011 . 2011A&A...528A..60L , 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 , Revealing O VII from stacked X-ray grating spectra of clusters, groups and elliptical galaxies . Sanders, J. S., Fabian, A. C., . MNRAS . 412-35 . 2011 . 2011MNRAS.412L..35S , An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F , On the Origin of the Extended Halpha Filaments in Cooling Flow Clusters . McDonald, Michael, Veilleux, Sylvain, et all. . ApJ . 721-1262 . 2010 . 2010ApJ...721.1262M , Exospheric solar wind charge exchange as seen by XMM-Newton... . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . 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 all. . MNRAS . 423-3561 . 2012 . 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 , The cool-core bias in X-ray galaxy cluster samples. I. Method and application to HIFLUGCS . Eckert, D., Molendi, S., . A&A . 526-79 . 2011 . 2011A&A...526A..79E , A systematic cross-search for radio-infrared counterparts of XMM- Newton sources . Combi, J. A., Albacete Colombo, J. F., et all. . Ap&SS . 331-53 . 2011 . 2011Ap&SS.331...53C , Characterization of Intracluster Medium Temperature Distributions of 62 Galaxy Clusters with XMM-Newton . Frank, K. A., Peterson, J. R., et all. . ApJ . 764-46 . 2013 . 2013ApJ...764...46F , 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 , Planck intermediate results. V. Pressure profiles of galaxy clusters from the Sunyaev-Zeldovich effect . Planck Collaboration, Ade, P. A. R., et all. . A&A . 550-131 . 2013 . 2013A&A...550A.131P , Insight into Active Galactic Nucleus and Host Galaxy Co-evolution from Hard X-Ray Emission . Wang, J., Zhou, X. L., . ApJ . 768-176 . 2013 . 2013ApJ...768..176W , Galaxy Cluster Baryon Fractions Revisited . Gonzalez, Anthony H., Sivanandam, Suresh, et all. . ApJ . 778-14 . 2013 . 2013ApJ...778...14G , The diversity of quasars unified by accretion and orientation . Shen, Yue, Ho, Luis C., . Natur . 513-210 . 2014 . 2014Natur.513..210S , Confirming the thermal Comptonization model for black hole X-ray emission in the low-hard state . Castro, M., D.Amico, F., et all. . A&A . 569-82 . 2014 . 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 , XMM-Newton and Chandra cross-calibration using HIFLUGCS galaxy clusters . Systematic temperature differences and cosmological impact . Schellenberger, G., Reiprich, T. H., et all. . A&A . 575-30 . 2015 . 2015A&A...575A..30S , Chemical Enrichment RGS cluster Sample (CHEERS): Constraints on turbulence . Pinto, Ciro, Sanders, Jeremy S., et all. . A&A . 575-38 . 2015 . 2015A&A...575A..38P , Origin of central abundances in the hot intra-cluster medium. I. Individual and average abundance ratios from XMM-Newton EPIC . Mernier, F., de Plaa, J., et all. . A&A . 592-157 . 2016 . 2016A&A...592A.157M , 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 , SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV . Clerc, N., Merloni, A., et all. . MNRAS . 463-4490 . 2016 . 2016MNRAS.463.4490C , The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F , Origin of central abundances in the hot intra-cluster medium. II. Chemical enrichment and supernova yield models . Mernier, F., de Plaa, J., et all. . A&A . 595-126 . 2016 . 2016A&A...595A.126M , X-Ray Morphological Analysis of the Planck ESZ Clusters . Lovisari, Lorenzo, Forman, William R., et all. . ApJ . 846-51 . 2017 . 2017ApJ...846...51L , HICOSMO: cosmology with a complete sample of galaxy clusters - II. Cosmological results . Schellenberger, G., Reiprich, T. H., . MNRAS . 471-1370 . 2017 . 2017MNRAS.471.1370S , CHEERS: The chemical evolution RGS sample . de Plaa, J., Kaastra, J. S., et all. . A&A . 607-98 . 2017 . 2017A&A...607A..98D , Solar abundance ratios of the iron-peak elements in the Perseus cluster . Hitomi Collaboration, Aharonian, Felix, et all. . Natur . 551-478 . 2017 . 2017Natur.551..478H , Charge exchange in galaxy clusters . Gu, Liyi, Mao, Junjie, et all. . A&A . 611-26 . 2018 . 2018A&A...611A..26G , Mass-invariance of the iron enrichment in the hot haloes of massive ellipticals, groups, and clusters of galaxies . Mernier, F., de Plaa, J., et all. . MNRAS . 478-116 . 2018 . 2018MNRAS.478L.116M , Solar chemical composition in the hot gas of cool-core ellipticals, groups, and clusters of galaxies . Mernier, F., Werner, N., et all. . MNRAS . 480-95 . 2018 . 2018MNRAS.480L..95M , The non-uniformity of galaxy cluster metallicity profiles . Lovisari, L., Reiprich, T. H., . MNRAS . 483-540 . 2019 . 2019MNRAS.483..540L , Enrichment of the Hot Intracluster Medium: Observations . Mernier, F., Biffi, V., et all. . SSRv . 214-129 . 2018 . 2018SSRv..214..129M , Deriving the Hubble constant using Planck and XMM-Newton observations of galaxy clusters . Kozmanyan, Arpine, Bourdin, Herve, et all. . A&A . 621-34 . 2019 . 2019A&A...621A..34K , Universal thermodynamic properties of the intracluster medium over two decades in radius in the X-COP sample . Ghirardini, V., Eckert, D., et all. . A&A . 621-41 . 2019 . 2019A&A...621A..41G , Discovery of Dying Active Galactic Nucleus in Arp 187: Experience of Drastic Luminosity Decline within 104 yr . Ichikawa, Kohei, Ueda, Junko, et all. . ApJ . 870-65 . 2019 . 2019ApJ...870...65I , The Galaxy Cluster Mass Scale and Its Impact on Cosmological Constraints from the Cluster Population . Pratt, G. W., Arnaud, M., et all. . SSRv . 215-25 . 2019 . 2019SSRv..215...25P , Physical properties of the X-ray gas as a dynamical diagnosis for galaxy clusters . Lagana, T. F., Durret, F., . MNRAS . 484-2807 . 2019 . 2019MNRAS.484.2807L , Searching for cool and cooling X-ray emitting gas in 45 galaxy clusters and groups . Liu, Haonan, Pinto, Ciro, et all. . MNRAS . 485-1757 . 2019 . 2019MNRAS.485.1757L , The Fornax3D project: Tracing the assembly history of the cluster from the kinematic and line-strength maps . Iodice, E., Sarzi, M., et all. . A&A . 627-136 . 2019 . 2019A&A...627A.136I , Why are some galaxy clusters underluminous?. The very low concentration of the CL2015 mass profile . Andreon, S., Moretti, A., et all. . A&A . 630-78 . 2019 . 2019A&A...630A..78A , X-Ray Scaling Relations for a Representative Sample of Planck-selected Clusters Observed with XMM-Newton . Lovisari, Lorenzo, Schellenberger, Gerrit, et all. . ApJ . 892-102 . 2020 . 2020ApJ...892..102L , X-ray properties of the X-CLASS-redMaPPer galaxy cluster sample: the luminosity-temperature relation . Molham, Mona, Clerc, Nicolas, et all. . MNRAS . 494-161 . 2020 . 2020MNRAS.494..161M , Multiwavelength classification of X-ray selected galaxy cluster candidates using convolutional neural networks . Kosiba, Matej, Lieu, Maggie, et all. . MNRAS . 496-4141 . 2020 . 2020MNRAS.496.4141K , SPIDERS: overview of the X-ray galaxy cluster follow-up and the final spectroscopic data release . Clerc, N., Kirkpatrick, C. C., et all. . MNRAS . 497-3976 . 2020 . 2020MNRAS.497.3976C , Hot Atmospheres of Galaxies, Groups, and Clusters of Galaxies . Werner, Norbert, Mernier, Franu00e7ois, . rfma . 0-279 . 2020 . 2020rfma.book..279K ,
Instrument
EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage
2008-07-17T08:01:53Z/2008-08-18T11:50:05Z
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.
