A dataset provided by the European Space Agency

Name 040083
Title Observations of the 1 Mpc radio source 6C0905+3955 and the half-Mpc source 3C356
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0400830301

DOI 10.5270/esa-8gu4pjo
Author Prof Andrew Fabian
Description Extended X-ray emission has been discovered around several distant powerful radio galaxies. The emission is most likely due to inverse Compton scattering of CMB photons by old radio synchrotron particles. The X-ray emission thus traces the total input of relativistic electrons into the surroundings of the radio galaxy, and the amount of energy injected, which will affect the gas properties of the host galaxy, group and cluster. All massive galaxies may have passed through such a phase. We propose to take a deep 60 ks observation of the exceptionally large 1 Mpc diameter, distant z=1.88 radio galaxy, 6C0905+3955, and a 20 ks observation of the 1-2 Mpc diameter z=1.08 radio galaxy 3C356. Both sources are known from our previous work to have extended X-ray emission along the radio source axis.
Publication An Extremely Luminous Panchromatic Outburst from the Nucleus of a Distant Galaxy . Levan, A. J., Tanvir, N. R., et all. . Sci . 333-199 . 2011 . 2011Sci...333..199L ,
New constraints on the X-ray spectral properties of type 1 active galactic nuclei . Scott, A. E., Stewart, G. C., et all. . MNRAS . 417-992 . 2011 . 2011MNRAS.417..992S ,
The inverse Compton X-ray-emitting lobes of the high-redshift giant radio galaxy 6C0905+39 . Erlund, M. C., Fabian, A. C., . MNRAS . 386-1774 . 2008 . 2008MNRAS.386.1774E ,
The Origin of the Hot Gas in the Galactic Halo: Confronting Models with XMM-Newton Observations . Henley, David B., Shelton, Robin L., et all. . ApJ . 723-935 . 2010 . 2010ApJ...723..935H ,
An XMM-Newton Survey of the Soft X-ray Background. I. The O VII and O VIII Lines Between l = 120 and l = 240 . Henley, David B., Shelton, Robin L., . ApJS . 187-388 . 2010 . 2010ApJS..187..388H ,
A serendipitous XMM survey of the SDSS: the evolution of the colour-magnitude diagram of X-ray AGN from z= 0.8 to 0.1 . Georgakakis, Antonis, Nandra, K., . MNRAS . 414-992 . 2011 . 2011MNRAS.414..992G ,
Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . 2012AN....333..313C ,
Detectability of low-energy X-ray spectral components in type 1 active galactic nuclei . Scott, A. E., Stewart, G. C., . MNRAS . 423-2633 . 2012 . <...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2006-10-30T11:59:09Z/2006-10-31T05:16:01Z
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 2007-12-01T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2007-12-01T00:00:00Z, 040083, 17.56_20190403_1200. https://doi.org/10.5270/esa-8gu4pjo