A dataset provided by the European Space Agency

Name: PROBING THE DYNAMICS OF JETS AND CLUSTERS WITH WATS
Published: 2005-10-08T00:00:00Z

Proposal ID	020425
Title	PROBING THE DYNAMICS OF JETS AND CLUSTERS WITH WATS
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0204250101
DOI	https://doi.org/10.5270/esa-3ql8wcp
Principal Investigator, PI	Dr IRINI SAKELLIOU
Abstract	Wide-angle tail radio galaxies (WATs) have distinctive radio properties and arewithin rich clusters. Most importantly, our recent work has provided evidencethat their relativistic small-scale jets disrupt and decelerate significantly atthe ISM/ICM interface. We now propose observations of a small sample of WATclusters to test this. With these data we will: locate the position of theinterface, measure the properties of the medium on either side, and uncover finestructure in the hot gas due to the motion of the galaxies and/or clustermergers. This investigation will enable us to resolve some outstanding puzzles:what disrupts (terminates and bends) their jets? Are they within cooling flows?Are their clusters merger remnants?
Publications	Galaxy Clusters in the Swift/BAT Era. II. 10 More Clusters Detected Above 15 keV \|Ajello, M., Rebusco, P., et al. \| ApJ \| 725-1688 \| 2010 \| 2010ApJ...725.1688A \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...725.1688A Radial profiles of Fe abundance in the intracluster medium of nearby clusters observed with XMM-Newton \|Matsushita, K., \| A&A \| 527-134 \| 2011 \| 2011A&A...527A.134M \| http://ui.adsabs.harvard.edu/#abs/2011A&A...527A.134M 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 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 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 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 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 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 Every BCG with a Strong Radio Agn has an X-Ray Cool Core: Is the Cool Core-Noncool Core Dichotomy Too Simple? \|Sun, M., \| ApJ \| 704-1586 \| 2009 \| 2009ApJ...704.1586S \| http://ui.adsabs.harvard.edu/#abs/2009ApJ...704.1586S 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 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 Halpha Tail, Intracluster H II Regions, and Star Formation: ESO 137-001 in Abell 3627 \|Sun, M., Donahue, M., \| ApJ \| 671-190 \| 2007 \| 2007ApJ...671..190S \| http://ui.adsabs.harvard.edu/#abs/2007ApJ...671..190S 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 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 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 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 Collimated synchrotron threads linking the radio lobes of ESO 137-006 \|Ramatsoku, M., Murgia, M., et al. \| A&A \| 636-1 \| 2020 \| 2020A&A...636L...1R \| http://ui.adsabs.harvard.edu/#abs/2020A&A...636L...1R 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 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	2004-09-19T10:12:11Z/2004-09-19T16:29:41Z
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	2005-10-08T00:00:00Z
Keywords	"hot gas", "distinctive radio properties", "cluster mergers", "cluster merger remnant", "icm interface", "scale jets disrupt", "wat cluster", "disrupts terminates", "uncover fine structure", "cooling flows", "rich clusters", "provided evidence"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr IRINI SAKELLIOU, 2005, 'PROBING THE DYNAMICS OF JETS AND CLUSTERS WITH WATS', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-3ql8wcp