A dataset provided by the European Space Agency

Name 011283
Title STRONG GRAVITY AND COMPLEX FE-LINE EMISSION IN SEYFERT I NUCLEI
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112830201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112830301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112830401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112830501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112830601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112830701

DOI 10.5270/esa-asdb4vl
Author Prof RICHARD GRIFFITHS
Description GT - We propose to constrain the possible contributors to the complex Fe-K line emission in Sy I nuclei, where these contributors include relativistically broadened disk line emission and narrow line emission originating in a torus or other dense material in the vicinity of the nucleus.
Publication Iron K-features in the hard X-ray XMM-Newton spectrum of NGC 4151 . Schurch, N. J., Warwick, R. S., et all. . MNRAS . 345-423 . 2003 . 2003MNRAS.345..423S ,
The complex soft X-ray spectrum of NGC 4151 . Schurch, N. J., Warwick, R. S., et all. . MNRAS . 350-1 . 2004 . 2004MNRAS.350....1S ,
Clearing up the clouds around NGC 4151: evidence of a highly ionized absorber . Piro, L., de Rosa, A., et all. . A&A . 441-13 . 2005 . 2005A&A...441L..13P ,
Kinematics of ionized gas in the barred Seyfert galaxy NGC 4151 . Asif, M. W., Mundell, C. G., . MNRAS . 359-408 . 2005 . 2005MNRAS.359..408A ,
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 ,
On the origin of soft X-rays in obscured AGN: answers from high-resolution spectroscopy with XMM-Newton . Guainazzi, Matteo, Bianchi, Stefano, . MNRAS . 374-1290 . 2007 . 2007MNRAS.374.1290G ,
The X-ray Energy Dependence of the Relation Between Optical and X-ray Emission in Quasars . Young, M., Elvis, M., . ApJ . 708-1388 . 2010 . 2010ApJ...708.1388Y ,
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 ,
Studying t...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2000-12-22T02:53:42Z/2001-12-02T04:28:47Z
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 2003-01-09T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2003-01-09T00:00:00Z, 011283, 17.56_20190403_1200. https://doi.org/10.5270/esa-asdb4vl