A dataset provided by the European Space Agency

Name 020709
Title HIGH-RESOLUTION X-RAY AND UV SPECTROSCOPY OF THE SEYFERT 1 GALAXY NGC7469
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0207090101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0207090201

DOI 10.5270/esa-6ipiyx1
Author Mr ALEXANDER BLUSTIN
Description We propose a long (150 ks) XMM-Newton observation of the Seyfert 1 galaxy NGC7469, to be carried out simultaneously with FUSE UV spectroscopy. We will investigate the connection between the X-ray and UV warm absorber-emitters in this object. A short XMM-Newton observation showed that at least one of the multiple phases of the X-ray warm absorber can be identified with a UV absorber phase. A fuller understanding of this system can only be achieved with a better signal-to-noise RGS spectrum. By understanding the ionisation and velocity structure of the outflow, we can determine its mass and kinetic luminosity, which are necessary for understanding the influence of outflows on the evolution of AGN, their host galaxies, and the surrounding intergalactic medium.
Publication The mass-energy budget of the ionised outflow in NGC 7469 . Blustin, A. J., Kriss, G. A., et all. . A&A . 466-107 . 2007 . 2007A&A...466..107B ,
The X-ray Power Spectral Density Function of the Seyfert Active Galactic Nucleus NGC 7469 . Markowitz, A., . ApJ . 724-26 . 2010 . 2010ApJ...724...26M ,
The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue . Watson, M. G., Schroder, A. C., et all. . A&A . 493-339 . 2009 . 2009A&A...493..339W ,
Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras . Mateos, S., Saxton, R. D., et all. . A&A . 496-879 . 2009 . 2009A&A...496..879M ,
X-ray colour-colour selection for heavily absorbed active galactic nuclei . Brightman, Murray, Nandra, Kirpal, . MNRAS . 422-1166 . 2012 . 2012MNRAS.422.1166B ,
Evidence for ultra-fast outflows in radio-quiet AGNs. I. Detection and statistical incidence of Fe K-shell absorption lines . Tombesi, F., Cappi, M., et all. . A&A . 521-57 . 2010 . 2010A&A...521A..57T ,
X-ray spectral properties of Seyfert galaxies and the unification scheme . Singh, V., Shastri, P., . A&A . 532-84 . 2011 . 2011A&A...532A..84S ,
On the apparent absence of broad iron lines in Seyfert galaxies . Bhayani, S., Nandra, K., . MNRAS . 416-629 . 2011 . 2011MNRAS.416..629B ,
X-Ray Abs...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2004-11-30T21:06:16Z/2004-12-03T23:20:41Z
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 2005-12-23T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2005-12-23T00:00:00Z, 020709, 17.56_20190403_1200. https://doi.org/10.5270/esa-6ipiyx1