A dataset provided by the European Space Agency

Name 050250
Title The properties and environments of giant radio sources
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502500101

DOI 10.5270/esa-yc7zfvd
Author Mr Chiranjib Konar
Description Giant radio sources (GRSs) raise several important questions related to their confinement and evolution and the properties of the IGM they inhabit. We request to observe two radio galaxies, 3C46 and 3C457, with {it XMM} to image and determine the spectra of the X-ray emission towards addressing some of these questions. The detection of inverse-Compton emission from the radio lobes will enable us to estimate lobe pressures. We will also determine any X-ray emission from a hot-gas environment, and thus understand the properties of the external medium and the confinement of the radio lobes. These observations will provide insights towards using GRSs as cosmological probes and also understanding the evolution of magnetic fields and energy densities with age.
Publication The active nuclei of z < 1.0 3CRR radio sources . Hardcastle, M. J., Evans, D. A., . MNRAS . 396-1929 . 2009 . 2009MNRAS.396.1929H ,
The dynamics of the giant radio galaxy 3C457 . Konar, C., Hardcastle, M. J., et all. . MNRAS . 400-480 . 2009 . 2009MNRAS.400..480K ,
Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . 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 all. . MNRAS . 423-3561 . 2012 . 2012MNRAS.423.3561C ,
An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities . Henley, David B., Shelton, Robin L., . ApJS . 202-14 . 2012 . 2012ApJS..202...14H ,
Radio-loud Active Galactic Nucleus: Is There a Link between Luminosity and Cluster Environment? . Ineson, J., Croston, J. H., et all. . ApJ . 770-136 . 2013 . 2013ApJ...770..136I ,
An XMM-Newton Survey of the Soft X-Ray Background. III. The Galactic Halo X-Ray Emission . Henley, David B., Shelton, Robin L., . ApJ . 773-92 . 2013 . 2013ApJ...773...92H ,
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 ,
The Or...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2007-12-02T20:29:20Z/2007-12-03T11:16:31Z
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 2009-01-18T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2009-01-18T00:00:00Z, 050250, 17.56_20190403_1200. https://doi.org/10.5270/esa-yc7zfvd