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 |
|
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 |
Last Update | 2025-01-27 |
Keywords | "radio halos", "double relic", "merging paradigm", "610 mhz", "radio halo", "extensive radio", "redshift range", "halo formation", "icm related", "physical properties", "galaxy cluster", "intermediate redshift", "campaign aimed", "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 |