A dataset provided by the European Space Agency

Name 009436
Title X-ray Spectroscopy of Low-Luminosity Active Galactic Nuclei with XMM
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0094360201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0094360401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0094360501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0094360601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0094360701

DOI 10.5270/esa-l8ten9x
Author Dr Eliot Quataert
Description We propose to use {it XMM} to perform X-ray spectroscopy on the nuclei of several nearby galaxies which harbor low-luminosity active galactic nuclei (LLAGN; NGC 4736, NGC 5033, and NGC 1052). {it ASCA} observations of these and other LLAGN suggest iron emission-line properties quite different from those of luminous Seyfert galaxies. {it XMM} will provide definitive measurements of the iron line properties in these systems (physical line width, equivalent width, centroid energy). This has important implications for the physics of accretion in LLAGN.
Publication High-resolution observations of SN 2001gd in NGC 5033 . Perez-Torres, M. A., Alberdi, A., et all. . MNRAS . 360-1055 . 2005 . 2005MNRAS.360.1055P ,
The X-ray variability and the near-IR to X-ray spectral energy distribution of four low luminosity Seyfert 1 galaxies . Papadakis, I. E., Ioannou, Z., et all. . A&A . 490-995 . 2008 . 2008A&A...490..995P ,
XMM-Newton observations of Seyfert galaxies from the Palomar spectroscopic survey: the X-ray absorption distribution . Akylas, A., Georgantopoulos, I., . A&A . 500-999 . 2009 . 2009A&A...500..999A ,
A Multi-wavelength Study of the Nature of Type 1.8-1.9 Seyfert Galaxies . Trippe, M. L., Crenshaw, D. M., et all. . ApJ . 725-1749 . 2010 . 2010ApJ...725.1749T ,
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 ,
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...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2001-02-09T23:51:15Z/2002-12-18T19:00:53Z
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 2004-01-31T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2004-01-31T00:00:00Z, 009436, 17.56_20190403_1200. https://doi.org/10.5270/esa-l8ten9x