A dataset provided by the European Space Agency

Name 040036
Title The broad Fe line and complex X-ray spectrum of the Seyfert 1 galaxy Mrk 290
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0400360201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0400360301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0400360401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0400360501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0400360601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0400360701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0400360801
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0400360901

DOI 10.5270/esa-7o58c98
Author Dr Giovanni Miniutti
Description We propose to observe the Seyfert 1 galaxy Mrk 290 for the first time with XMM-Newton for a total exposure of 50 ks. Our main goals are: 1) study the details of the broad Fe line profile detected by ASCA, measure its parameters inferring limits on the black hole spin, and study its short-timescale variability and response to the continuum; 2) characterise at both CCD and RGS resolution the complex soft X-ray spectrum where ASCA detected clear signatures of warm absorber and possible emission lines; 3) use the expected X-ray variability to unveil the main spectral components and their contribution to the (already observed) spectral variability.
Publication 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 ,
X-ray Emission from Optically Selected Radio-intermediate and Radio-loud Quasars . Miller, B. P., Brandt, W. N., et all. . ApJ . 726-20 . 2011 . 2011ApJ...726...20M ,
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 ,
The XMM Cluster Survey: optical analysis methodology and the first data release . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 423-1024 . 2012 . 2012MNRAS.423.1024M ,
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 ,
Evidence for Ultra-fast Outflows in Radio-quiet Active Galactic Nuclei. II. Detailed Photoionization Modeling of Fe K-shell Absorpti...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2006-04-30T16:47:58Z/2006-05-07T00:58:32Z
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 2007-06-01T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2007-06-01T00:00:00Z, 040036, 17.56_20190403_1200. https://doi.org/10.5270/esa-7o58c98