A dataset provided by the European Space Agency

Name: The Local Galaxy Cluster Mass Function of the Brightest Clusters in the Sky - I
Published: 2009-04-01T00:00:00Z

Proposal ID	050521
Title	The Local Galaxy Cluster Mass Function of the Brightest Clusters in the Sky - I
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505210101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505210201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505210301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505210401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505210601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505210801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505211001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505211101
DOI	https://doi.org/10.5270/esa-3h2i9z5
Principal Investigator, PI	Dr Thomas Reiprich
Abstract	Galaxy clusters have proven to be highly competitive and complementarycosmological probes. For the next major breakthrough more reliable massestimates and, therefore, a better understanding of cluster physics areessential. We propose to complete XMM-Newton observations of a flux-limitedsample of the 64 X-ray brightest clusters in the sky to (i) take full advantageof 3 Ms of XMM-Newton data already available, (ii) determine very precise gastemperature profiles, (iii) characterize merging clusters by direct comparisonto simulations, (iv) update the luminosity-mass relation, (v) construct the mostprecise local cluster mass function, (vi) improve constraints on OmegaM andsigma8 significantly, and (vii) provide a reliable statistical baseline for comparison to high-redshift samples.
Publications	HIFLUGCS: Galaxy cluster scaling relations between X-ray luminosity, gas mass, cluster radius, and velocity dispersion \|Zhang, Y.-Y., Andernach, H., et al. \| A&A \| 526-105 \| 2011 \| 2011A&A...526A.105Z \| http://ui.adsabs.harvard.edu/#abs/2011A&A...526A.105Z Planck early results. XI. Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations \|Planck Collaboration, Ade, P. A. R., et al. \| A&A \| 536-11 \| 2011 \| 2011A&A...536A..11P \| http://ui.adsabs.harvard.edu/#abs/2011A&A...536A..11P The Swift Burst Alert Telescope Perspective on Non-thermal Emission in HIFLUGCS Galaxy Clusters \|Wik, Daniel R., Sarazin, Craig L., et al. \| ApJ \| 748-67 \| 2012 \| 2012ApJ...748...67W \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...748...67W 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 Evidence for Rapidly Rotating Black Holes in Fanaroff-Riley I Radio Galaxies \|Wu, Qingwen, Cao, Xinwu, \| ApJ \| 735-50 \| 2011 \| 2011ApJ...735...50W \| http://ui.adsabs.harvard.edu/#abs/2011ApJ...735...50W Star-formation efficiency and metal enrichment of the intracluster medium in local massive clusters of galaxies \|Zhang, Y.-Y., Lagana, T. F., et al. \| A&A \| 535-78 \| 2011 \| 2011A&A...535A..78Z \| http://ui.adsabs.harvard.edu/#abs/2011A&A...535A..78Z XMM-Newton/Sloan Digital Sky Survey: Star Formation Efficiency in Galaxy Clusters and Constraints on the Matter-density Parameter \|Lagana, Tatiana F., Zhang, Yu-Ying, et al. \| ApJ \| 743-13 \| 2011 \| 2011ApJ...743...13L \| http://ui.adsabs.harvard.edu/#abs/2011ApJ...743...13L X-Ray Substructure Studies of Four Galaxy Clusters Using XMM-Newton Data \|Zhang, Yu-Ying, Reiprich, Thomas H., et al. \| ApJ \| 699-1178 \| 2009 \| 2009ApJ...699.1178Z \| http://ui.adsabs.harvard.edu/#abs/2009ApJ...699.1178Z Cold fronts in galaxy clusters \|Ghizzardi, S., Rossetti, M., \| A&A \| 516-32 \| 2010 \| 2010A&A...516A..32G \| http://ui.adsabs.harvard.edu/#abs/2010A&A...516A..32G A serendipitous XMM survey of the SDSS: the evolution of the colour-magnitude diagram of X-ray AGN from z= 0.8 to 0.1 \|Georgakakis, Antonis, Nandra, K., \| MNRAS \| 414-992 \| 2011 \| 2011MNRAS.414..992G \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.414..992G 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 Detection of X-ray galaxy clusters based on the Kolmogorov method \|Gurzadyan, V. G., Durret, F., et al. \| EL \| 95-69001 \| 2011 \| 2011EL.....9569001G \| http://ui.adsabs.harvard.edu/#abs/2011EL.....9569001G The XMM Cluster Survey: X-ray analysis methodology \|Lloyd-Davies, E. J., Romer, A. Kathy, et al. \| MNRAS \| 418-14 \| 2011 \| 2011MNRAS.418...14L \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.418...14L 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 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 \| http://ui.adsabs.harvard.edu/#abs/2011A&A...526A..79E Characterization of Intracluster Medium Temperature Distributions of 62 Galaxy Clusters with XMM-Newton \|Frank, K. A., Peterson, J. R., et al. \| ApJ \| 764-46 \| 2013 \| 2013ApJ...764...46F \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...764...46F Planck intermediate results. V. Pressure profiles of galaxy clusters from the Sunyaev-Zeldovich effect \|Planck Collaboration, Ade, P. A. R., et al. \| A&A \| 550-131 \| 2013 \| 2013A&A...550A.131P \| http://ui.adsabs.harvard.edu/#abs/2013A&A...550A.131P A Good Mass Proxy for Galaxy Clusters with XMM-Newton \|Zhao, Hai-Hui, Jia, Shu-Mei, et al. \| ApJ \| 778-124 \| 2013 \| 2013ApJ...778..124Z \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...778..124Z A volume-limited sample of X-ray galaxy groups and clusters - I. Radial entropy and cooling time profiles \|Panagoulia, E. K., Fabian, A. C., \| MNRAS \| 438-2341 \| 2014 \| 2014MNRAS.438.2341P \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.438.2341P 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 Stellar tidal disruption candidates found by cross-correlating the ROSAT Bright Source Catalogue and XMM-Newton observations \|Khabibullin, I., Sazonov, S., \| MNRAS \| 444-1041 \| 2014 \| 2014MNRAS.444.1041K \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.444.1041K 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 XMM-Newton and Chandra cross-calibration using HIFLUGCS galaxy clusters . Systematic temperature differences and cosmological impact \|Schellenberger, G., Reiprich, T. H., et al. \| A&A \| 575-30 \| 2015 \| 2015A&A...575A..30S \| http://ui.adsabs.harvard.edu/#abs/2015A&A...575A..30S 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 Sunyaev-Zel.dovich effect or not? Detecting the main foreground effect of most galaxy clusters \|Xiao, Weike, Chen, Chen, et al. \| MNRAS \| 432-41 \| 2013 \| 2013MNRAS.432L..41X \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.432L..41X 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 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 A volume-limited sample of X-ray galaxy groups and clusters - II. X-ray cavity dynamics \|Panagoulia, E. K., Fabian, A. C., et al. \| MNRAS \| 444-1236 \| 2014 \| 2014MNRAS.444.1236P \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.444.1236P 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 A Catalog Sample of Low-mass Galaxies Observed in X-Rays with Central Candidate Black Holes \|Nucita, A. A., Manni, L., et al. \| ApJ \| 837-66 \| 2017 \| 2017ApJ...837...66N \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...837...66N HIFLUGCS: X-ray luminosity-dynamical mass relation and its implications for mass calibrations with the SPIDERS and 4MOST surveys \|Zhang, Yu-Ying, Reiprich, Thomas H., et al. \| A&A \| 599-138 \| 2017 \| 2017A&A...599A.138Z \| http://ui.adsabs.harvard.edu/#abs/2017A&A...599A.138Z 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 HICOSMO - cosmology with a complete sample of galaxy clusters - I. Data analysis, sample selection and luminosity-mass scaling relation \|Schellenberger, G., Reiprich, T. H., \| MNRAS \| 469-3738 \| 2017 \| 2017MNRAS.469.3738S \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.469.3738S X-Ray Morphological Analysis of the Planck ESZ Clusters \|Lovisari, Lorenzo, Forman, William R., et al. \| ApJ \| 846-51 \| 2017 \| 2017ApJ...846...51L \| http://ui.adsabs.harvard.edu/#abs/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 \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.471.1370S 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 Anisotropy of the galaxy cluster X-ray luminosity-temperature relation \|Migkas, Konstantinos, Reiprich, Thomas H., \| A&A \| 611-50 \| 2018 \| 2018A&A...611A..50M \| http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..50M The 3CR Chandra Snapshot Survey: Extragalactic Radio Sources with Redshifts between 1 and 1.5 \|Stuardi, C., Missaglia, V., et al. \| ApJS \| 235-32 \| 2018 \| 2018ApJS..235...32S \| http://ui.adsabs.harvard.edu/#abs/2018ApJS..235...32S 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 The XMM Cluster Survey: Present status and latest results \|Viana, P. T. P., Mehrtens, N., et al. \| AN \| 334-462 \| 2013 \| 2013AN....334..462V \| http://ui.adsabs.harvard.edu/#abs/2013AN....334..462V 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 Deriving the Hubble constant using Planck and XMM-Newton observations of galaxy clusters \|Kozmanyan, Arpine, Bourdin, Herve, et al. \| A&A \| 621-34 \| 2019 \| 2019A&A...621A..34K \| http://ui.adsabs.harvard.edu/#abs/2019A&A...621A..34K 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 The Galaxy Cluster Mass Scale and Its Impact on Cosmological Constraints from the Cluster Population \|Pratt, G. W., Arnaud, M., et al. \| SSRv \| 215-25 \| 2019 \| 2019SSRv..215...25P \| http://ui.adsabs.harvard.edu/#abs/2019SSRv..215...25P A new, clean catalogue of extragalactic non-nuclear X-ray sources in nearby galaxies \|Earnshaw, H. P., Roberts, T. P., et al. \| MNRAS \| 483-5554 \| 2019 \| 2019MNRAS.483.5554E \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483.5554E 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 \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.484.2807L Dynamics of Faint Clusters of Galaxies \|Erkurt, A., Tektunali, H. G., et al. \| POBeo \| 86-305 \| 2009 \| 2009POBeo..86..305E \| http://ui.adsabs.harvard.edu/#abs/2009POBeo..86..305E The Fornax3D project: Tracing the assembly history of the cluster from the kinematic and line-strength maps \|Iodice, E., Sarzi, M., et al. \| A&A \| 627-136 \| 2019 \| 2019A&A...627A.136I \| http://ui.adsabs.harvard.edu/#abs/2019A&A...627A.136I Testing emergent gravity on galaxy cluster scales \|Tamosiunas, Andrius, Bacon, David, et al. \| JCAP \| 5-53 \| 2019 \| 2019JCAP...05..053T \| http://ui.adsabs.harvard.edu/#abs/2019JCAP...05..053T Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline \|Hollowood, Devon L., Jeltema, Tesla, et al. \| ApJS \| 244-22 \| 2019 \| 2019ApJS..244...22H \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..244...22H The Y SZ,Planck - Y SZ,XMM scaling relation and its difference between cool-core and non-cool-core clusters \|Zhu, Yue, Wang, Yuan-Hao, et al. \| RAA \| 19-104 \| 2019 \| 2019RAA....19..104Z \| http://ui.adsabs.harvard.edu/#abs/2019RAA....19..104Z Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters \|Palmese, A., Annis, J., et al. \| MNRAS \| 493-4591 \| 2020 \| 2020MNRAS.493.4591P \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.4591P X-Ray Scaling Relations for a Representative Sample of Planck-selected Clusters Observed with XMM-Newton \|Lovisari, Lorenzo, Schellenberger, Gerrit, et al. \| ApJ \| 892-102 \| 2020 \| 2020ApJ...892..102L \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...892..102L 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 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 Comparing different mass estimators for a large subsample of the Planck-ESZ clusters \|Lovisari, L., Ettori, S., et al. \| A&A \| 644-78 \| 2020 \| 2020A&A...644A..78L \| http://ui.adsabs.harvard.edu/#abs/2020A&A...644A..78L 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 Mass-Velocity Dispersion Relation in HIFLUGCS Galaxy Clusters \|Tian, Yong, Yu, Po-Chieh, et al. \| ApJ \| 910-56 \| 2021 \| 2021ApJ...910...56T \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...910...56T 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 The thermalization of massive galaxy clusters \|Sereno, Mauro, Lovisari, Lorenzo, et al. \| MNRAS \| 507-5214 \| 2021 \| 2021MNRAS.507.5214S \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.507.5214S 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 PACT. II. Pressure profiles of galaxy clusters using Planck and ACT \|Pointecouteau, E., Santiago-Bautista, I., et al. \| A&A \| 651-73 \| 2021 \| 2021A&A...651A..73P \| http://ui.adsabs.harvard.edu/#abs/2021A&A...651A..73P The impact of precession on the observed population of ULXs \|Khan, Norman, Middleton, Matthew J., et al. \| MNRAS \| 509-2493 \| 2022 \| 2022MNRAS.509.2493K \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.509.2493K The Redshift Evolution of Ultraluminous X-Ray Sources out to z 0.5: Comparison with X-Ray Binary Populations and Contribution to the Cosmic X-Ray Background \|Scott Barrows, R., Comerford, Julia M., et al. \| ApJ \| 932-27 \| 2022 \| 2022ApJ...932...27S \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...932...27S A systematic comparison of galaxy cluster temperatures measured with NuSTAR and Chandra \|Wallbank, A. N., Maughan, B. J., et al. \| MNRAS \| 517-5594 \| 2022 \| 2022MNRAS.517.5594W \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.517.5594W Heating of the intracluster medium by buoyant bubbles and sound waves \|Iqbal, Asif, Majumdar, Subhabrata, et al. \| MNRAS \| 518-2735 \| 2023 \| 2023MNRAS.518.2735I \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.518.2735I 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 Constraining the mass and redshift evolution of the hydrostatic mass bias using the gas mass fraction in galaxy clusters \|Wicker, R., Douspis, M., et al. \| A&A \| 674-48 \| 2023 \| 2023A&A...674A..48W \| http://ui.adsabs.harvard.edu/#abs/2023A&A...674A..48W Studying X-ray instruments with galaxy clusters \|Nevalainen, J., Molendi, S., \| A&A \| 676-142 \| 2023 \| 2023A&A...676A.142N \| http://ui.adsabs.harvard.edu/#abs/2023A&A...676A.142N A radio bubble shredded by gas sloshing? \|Botteon, A., Gastaldello, F., et al. \| MNRAS \| 527-919 \| 2024 \| 2024MNRAS.527..919B \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.527..919B 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 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	2007-06-16T19:12:07Z/2008-02-25T09:10:21Z
Version	PPS_NOT_AVAILABLE
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	2009-04-01T00:00:00Z
Keywords	"complementary cosmological probes", "brightest cluster", "xmm newton data", "luminosity mass relation", "XMM", "merging cluster", "cluster physics", "major breakthrough", "iv update", "redshift samples", "complete xmm newton", "galaxy cluster", "xray brightest cluster", "reliable mass", "XMM-Newton", "reliable statistical baseline", "flux limited sample"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Thomas Reiprich, 2009, 'The Local Galaxy Cluster Mass Function of the Brightest Clusters in the Sky - I', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-3h2i9z5