A dataset provided by the European Space Agency

Name 011284
Title STUDIES OF COMPLEX FE-LINE EMISSION IN LLAGN AND LINERS
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112840101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112840201

DOI 10.5270/esa-i45dj38
Author Prof RICHARD GRIFFITHS
Description GT - We propose to determine whether complex, possibly ionized Fe-K emission is present in M81, NGC4579 and M51 as suggested by examination of ASCA data. We will constrain the energy of the line centroid and thus resolve whether the line-emitting gas is ionized. The line E.W. will be used as a diagnostic to discriminate between various models for the origin of the Fe-K lines. Constraints on the line profiles will be used to indicate the extent of any relativistic line broadening or line complexity.
Publication Long-term Spectral Variations of Ultraluminous X-ray Sources in the Interacting Galaxy Systems M 51 and NGC 4490-85 . Yoshida, Tessei, Ebisawa, Ken, et all. . ApJ . 722-760 . 2010 . 2010ApJ...722..760Y ,
Radial profiles of Fe abundance in the intracluster medium of nearby clusters observed with XMM-Newton . Matsushita, K., . A&A . 527-134 . 2011 . 2011A&A...527A.134M ,
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 ,
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 the X-ray-UV Variability of Active Galactic Nuclei with data from Swift and XMM archives . Turriziani, Sara, . JPhCS . 280-12005 . 2011 . 2011JPhCS.280a2005T ,
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 x-ray luminous galaxy cluster population at 0.9 < z ≲ 1.6 as revealed by the XMM-Newton Distant Cluster Project . Fassbender, R., Bohringer, H., et all. ...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2003-01-15T13:12:55Z/2003-06-12T15:09:47Z
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 2004-07-01T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2004-07-01T00:00:00Z, 011284, 17.56_20190403_1200. https://doi.org/10.5270/esa-i45dj38