A dataset provided by the European Space Agency

Proposal ID 089242
Title X-raying Giant Radio Galaxies
Download Data Associated to the proposal

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0892420201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0892420301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0892420401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0892420501

DOI https://doi.org/10.57780/esa-199lyjw
Principal Investigator, PI Dr Ming Sun
Abstract As the largest and most energetic single objects in the Universe, giant radiogalaxies (GRGs), are of particular interest as they are less common but extremeexamples of radio source evolution. No unified model has emerged to explain theproperties of this extreme class of radio galaxies. Previous studies of GRGs aremostly at radio and optical bands, and there is a lack of systematic study ofGRGs in X-rays. As the energetic radio jets of GRGs extend outwards, theyinteract with the surrounding medium. We select a complete sample of nearby GRGsand propose new XMM observations to complete the X-ray coverage of the sample tostudy the X-ray properties of GRGs and their environments, which helps tounderstand the processes responsible for the formation and evolution of GRGs.
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2021-11-11T02:54:40Z/2022-02-14T17:03:27Z
Version 19.17_20220121_1250
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 2023-03-02T00:00:00Z
Keywords "xray properties", "XMM", "optical bands", "unified model", "xray coverage", "energetic single objects", "giant radiogalaxy grgs", "complete sample", "nearby grgs", "energetic radio jets", "radio source evolution"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Ming Sun, 2023, 'X-raying Giant Radio Galaxies', 19.17_20220121_1250, European Space Agency, https://doi.org/10.57780/esa-199lyjw