A dataset provided by the European Space Agency

Name 050412
Title X-ray Environment of Radio Galaxy 4C 29.30
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0504120101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0504120201

DOI 10.5270/esa-vlnderd
Author Dr Aneta Siemiginowska
Description We propose to observe a radio galaxy, 4C 29.30 with XMM-Newton for 40ksec in order to study (1) the spectral properties of the nucleus; and (2) search for X-ray emission associated with the radio halo surrounding this source. This low redshift galaxy is embedded in a rich environment studied in optical and radio bands. The radio jets end just outside the host galaxy and this 60kpc structure is embedded in a ~600kpc radio halo. The good quality X-ray observations are missing. A short ~8ksec Chandra archival data with a low S-N do not allow for detailed analysis. Our new XMM-Newton observation will provide the best quality X-ray spectra of the radio core. The large field of view of the XMM-Newton is required for studies of any large scale emission associated with the radio halo.
Publication 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 ,
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 ,
Nuclear X-Ray Properties of the Peculiar Radio-loud Hidden AGN 4C+29.30 . Sobolewska, M. A., Siemiginowska, Aneta, et all. . ApJ . 758-90 . 2012 . 2012ApJ...758...90S ,
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 ,
The 2XMMi-SDSS Galaxy Cluster Survey. III. Clusters associated with spectroscopically targeted luminous red galaxies in SDSS-DR10 . Takey, A., Schwope, A., . A&A . 564-54 . 2014 . 2014A&A...564A..54T ,
Ultrafast outflows in radio-loud active galactic nuclei . Tombesi, F., Tazaki, F., et all. . MNRAS . 443-2154 . 2014 . 2014MNRAS.443.2154T ,
Confirming the thermal Comptonization model for black hole X-ray emission in the low-hard state . Castro, M., D.Amico, F., et all. ...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2008-04-11T09:33:36Z/2008-04-12T01:16:26Z
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 2009-06-06T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2009-06-06T00:00:00Z, 050412, 17.56_20190403_1200. https://doi.org/10.5270/esa-vlnderd