A dataset provided by the European Space Agency

Name 020113
Title THE INTRIGUING FE-LINE PROFILE IN SEYFERT 1 NUCLEI: EXPANDING THE XMM-N CENSUS
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0201130101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0201130201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0201130301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0201130501

DOI 10.5270/esa-sw09oa1
Author Dr Maria Santos-Lleo
Description We propose to obtain high signal to noise EPIC spectra of a sample of X-ray bright Seyfert 1 galaxies. The main objective is to properly characterize the profile of the iron fluorescence line. Hence, the sample of Seyfert 1 galaxies with proper measurements of the iron line width will be increased and current (contradictory) models for its origin will be probed. The relatively long exposure times needed will also allow good signal to noise RGS spectra to characterize the soft X-ray emission and measure possible emission-absorption lines from photoionised gas in the vicinity of the nucleus. Rapid variability, when detected, will be used to constrain sizes and causality effects between the different emitting-absorbing regions.
Publication Discovery of Hard X-Ray Delays in the X-Ray Emission of the Seyfert 1 Galaxy Markarian 110: Possible Evidence of Comptonization . Dasgupta, Surajit, Rao, A. R., . ApJ . 651-13 . 2006 . 2006ApJ...651L..13D ,
XMM-Newton observation of Mrk 110 . Boller, Th., Balestra, I., . A&A . 465-87 . 2007 . 2007A&A...465...87B ,
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 ,
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 ,
The Swift Burst Alert Telescope Detected Seyfert 1 Galaxies: X-Ray Broadband Properties and Warm Absorbers . Winter, Lisa M., Veilleux, Sylvain, et all. . ApJ . 745-107 . 2012 . 2012ApJ...745..107W ,
A combined optical and X-ray study of unobscured type 1 active galactic nuclei - I. Optical spectra and spectral energy distribution modelling . Jin, Chichuan, Ward, Martin, et all. . MNR...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2004-03-09T05:53:17Z/2004-11-15T18:15:01Z
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 2006-03-05T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2006-03-05T00:00:00Z, 020113, 17.56_20190403_1200. https://doi.org/10.5270/esa-sw09oa1