A dataset provided by the European Space Agency

Name 050612
Title The Broad Line Radio Galaxy 3C 382


DOI 10.5270/esa-mhujinu
Author Dr Anna Lia Longinotti
Description It is proposed to obtain the first XMM-Newton observation of the Broad Line Radio Galaxies 3C382. This object is characterised by warm absorption in the soft X-ray spectrum and a controversial Fe line the origin of which is still largely unknown. In earlier data it appears to be extremely broad (ASCA), possibly relativistically broadened, while it is reported unresolved and consistent with an origin in distant reflection in BeppoSAX data. The capabilities of XMM-Newton will be fully exploited. It will be possible to study in detail the Fe~K line profile and the jet contribution to the soft X-ray spectrum using a high S-N pn spectrum and it will be possible to elucidate the presence of X-ray absorption thanks to the RGS high resolution data.
Publication First high-resolution detection of a warm absorber in the Broad Line Radio Galaxy 3C 382 . Torresi, E., Grandi, P., et all. . MNRAS . 401-10 . 2010 . 2010MNRAS.401L..10T ,
The Suzaku view of 3C 382 . Sambruna, R. M., Tombesi, F., et all. . ApJ . 734-105 . 2011 . 2011ApJ...734..105S ,
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 ,
Ultrafast outflows in radio-loud active galactic nuclei . Tombesi, F., Tazaki, F., et all. . MNRAS . 443-2154 . 2014 . 2014MNRAS.443.2154T ,
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 ,
X-ray spectral parameters for a sample of 95 active galactic nuclei . Vasylenko, A. A., Zhdanov, V. I., . Ap&SS . 360-71 . 2015 . 2015Ap&SS.360...71V ,
A hard X-ray view of the soft excess in AGN . Boissay, Rozenn, Ricci, Claudio, . A&A . 588-70 . 2016 . 2016A&A...588A..70B ,
The Interaction of the Fermi Bubbles with the Milky Way.s Hot Gas Halo . Miller, Matthew J., Bregman, Joel N., . ApJ . 829-9 . 2016 . 2016ApJ...829....9M ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2008-04-28T11:23:33Z/2008-04-28T22:19:42Z
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 2009-06-07T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2009-06-07T00:00:00Z, 050612, 17.56_20190403_1200. https://doi.org/10.5270/esa-mhujinu