A dataset provided by the European Space Agency

Name 055104
Title Relics and Halos at intermediate redshift: testing the merging paradigm
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0551040101

DOI 10.5270/esa-pvv3wtc
Author Prof Pasquale Mazzotta
Description In A0-6 we proposed to observe the galaxy cluster RXCJ1314.4--2515 which was approved in priority A. Unfortunately the observation is affected by strong flares for 69% of the time. We propose to re-observe it to compensate for the time loss. RXCJ1314.4--2515 was selected from an extensive radio observational campaign aimed to search for radio halos and relics in galaxy clusters in the redshift range 0.2 div 0.4 at 610 MHz. RXCJ1314.4--2515 is exceptional as it is the unique case known to date of a cluster hosting both a radio halo and a double relic. The detailed study of the dynamics of this cluster will help us to test the merging paradigm and the physical properties of the ICM related to the relics and halo formation.
Publication 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 ,
Detection of an Unidentified Emission Line in the Stacked X-Ray Spectrum of Galaxy Clusters . Bulbul, Esra, Markevitch, Maxim, et all. . ApJ . 789-13 . 2014 . 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 ,
Low frequency follow up of radio haloes and relics in the GMRT Radio Halo Cluster Survey . Venturi, T., Giacintucci, S., et all. . A&A . 551-24 . 2013 . 2013A&A...551A..24V ,
Occurrence of radio halos in galaxy clusters. Insight from a mass-selected sample . Cuciti, V., Cassano, R., et all. . A&A . 580-97 . 2015 . 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 ,
A novel scenario for the possible X-ray line feature at ~3.5 keV. Charge exchange with bare sulfur ions . Gu, L., Kaastra, J., et all. . A&A . 584-11 . 2015 . 2015A&A...584L..11G ,
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 . ...,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 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 all. . MNRAS . 467-936 . 2017 . 2017MNRAS.467..936G ,
X-Ray Lines from Dark Matter Annihilation at the keV Scale . Brdar, Vedran, Kopp, Joachim, et all. . PhRvL . 120-61301 . 2018 . 2018PhRvL.120f1301B ,
WIMP dark matter candidates and searches---current status and future prospects . Roszkowski, Leszek, Sessolo, Enrico Maria, . RPPh . 81-66201 . 2018 . 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 ,
Laboratory Measurements of X-Ray Emission from Highly Charged Argon Ions . Bulbul, Esra, Foster, Adam, et all. . ApJ . 870-21 . 2019 . 2019ApJ...870...21B ,
Merging Cluster Collaboration: A Panchromatic Atlas of Radio Relic Mergers . Golovich, N., Dawson, W. A., et all. . ApJ . 882-69 . 2019 . 2019ApJ...882...69G ,
Particle re-acceleration and Faraday-complex structures in the RXC J1314.4-2515 galaxy cluster . Stuardi, C., Bonafede, A., et all. . MNRAS . 489-3905 . 2019 . 2019MNRAS.489.3905S ,
Shock acceleration efficiency in radio relics . Botteon, A., Brunetti, G., et all. . A&A . 634-64 . 2020 . 2020A&A...634A..64B ,
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 ,
Probing cosmic isotropy with a new X-ray galaxy cluster sample through the LX-T scaling relation . Migkas, K., Schellenberger, G., et all. . A&A . 636-15 . 2020 . 2020A&A...636A..15M ,
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 ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2009-01-21T01:43:38Z/2009-01-21T16:08:56Z
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.
Creator Contact https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published 2010-03-03T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2010-03-03T00:00:00Z, 055104, 17.56_20190403_1200. https://doi.org/10.5270/esa-pvv3wtc