A dataset provided by the European Space Agency

Name: Relics and Halos at intermediate redshift: testing the merging paradigm
Published: 2008-09-27T00:00:00Z

Proposal ID	050173
Title	Relics and Halos at intermediate redshift: testing the merging paradigm
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0501730101
DOI	https://doi.org/10.5270/esa-pcxdkl1
Principal Investigator, PI	Prof Pasquale Mazzotta
Abstract	Within the framework of an extensive radio observational campaign aimed tosearch for radio halos and relics in galaxy clusters in the redshift range0.2-0.4 at 610 MHz, we propose to observe one cluster of our sample which isexceptional in the radio band and therefore extremely promising for testing themerging paradigm. RXCJ1314.4-2515 is the unique case known to date of galaxycluster hosting both a radio halo and a double relic. Our goal is to reconstructthe detailed dynamics of this cluster and to test the physical properties of theICM related to the relics and halo formation.
Publications	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 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 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 Low frequency follow up of radio haloes and relics in the GMRT Radio Halo Cluster Survey \|Venturi, T., Giacintucci, S., et al. \| A&A \| 551-24 \| 2013 \| 2013A&A...551A..24V \| http://ui.adsabs.harvard.edu/#abs/2013A&A...551A..24V Occurrence of radio halos in galaxy clusters. Insight from a mass-selected sample \|Cuciti, V., Cassano, R., et al. \| A&A \| 580-97 \| 2015 \| 2015A&A...580A..97C \| http://ui.adsabs.harvard.edu/#abs/2015A&A...580A..97C 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 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 study of halo and relic radio emission in merging clusters using the Murchison Widefield Array \|George, L. T., Dwarakanath, K. S., et al. \| MNRAS \| 467-936 \| 2017 \| 2017MNRAS.467..936G \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.467..936G 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 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 Merging Cluster Collaboration: A Panchromatic Atlas of Radio Relic Mergers \|Golovich, N., Dawson, W. A., et al. \| ApJ \| 882-69 \| 2019 \| 2019ApJ...882...69G \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...882...69G Particle re-acceleration and Faraday-complex structures in the RXC J1314.4-2515 galaxy cluster \|Stuardi, C., Bonafede, A., et al. \| MNRAS \| 489-3905 \| 2019 \| 2019MNRAS.489.3905S \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.489.3905S Shock acceleration efficiency in radio relics \|Botteon, A., Brunetti, G., et al. \| A&A \| 634-64 \| 2020 \| 2020A&A...634A..64B \| http://ui.adsabs.harvard.edu/#abs/2020A&A...634A..64B 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 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 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 Synchrotron intensity gradient revealing magnetic fields in galaxy clusters \|Hu, Yue, Stuardi, C., et al. \| NatCo \| 15-1006 \| 2024 \| 2024NatCo..15.1006H \| http://ui.adsabs.harvard.edu/#abs/2024NatCo..15.1006H 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2007-08-07T15:38:17Z/2007-08-08T07:50:13Z
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	2008-09-27T00:00:00Z
Keywords	"610 mhz", "double relic", "redshift range", "merging paradigm", "extensive radio", "radio halos", "intermediate redshift", "galaxy cluster", "campaign aimed", "icm related", "physical properties", "radio halo", "halo formation", "radio band"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Pasquale Mazzotta, 2008, 'Relics and Halos at intermediate redshift: testing the merging paradigm', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-pcxdkl1