Proposal ID | 040278 |
Title | XMM Observations of Intermediate-Luminosity BLRGs: Expanding the parameter space |
Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0402780101 |
DOI | https://doi.org/10.5270/esa-748pc14 |
Principal Investigator, PI | Dr R. Sambruna |
Abstract | From the SDSS radio-loud AGN sample of Best et al. (2005) we extracted avolume-limited ($z<0.1$) sample of 11 Broad Line Radio Galaxies, with X-rayluminosities in the range 10^41-10^43 erg/s, 3 orders of magnitude lower thanclassical BLRGs, and matching most Seyferts. The XMM observations of this newsample will allow us to: 1) measure the X-ray continua; 2) test multiwavelengthcorrelations valid for bright BLRGs; and 3) constrain the optical-to-X-ray SEDs.We will constrain the nature of the accretion flow and relative importance ofthe jet in these sources,and compare to luminous radio-loud and radio-quiet AGNsto uncover the fundamental parameters that determine the properties ofradio-loud AGN. |
Publications |
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Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2006-05-30T15:40:49Z/2007-04-21T01:26:51Z |
Version | 17.56_20190403_1200 |
Mission Description | The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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 | 2008-05-21T00:00:00Z |
Last Update | 2025-01-27 |
Keywords | "intermediate luminosity blrgs", "fundamental parameters", "parameter space", "magnitude lower", "broad line radiogalaxy", "SDSS", "volume limited", "bright blrgs", "radio quiet agns", "relative importance", "luminous radio loud", "classical blrgs", "xray luminosities", "XMM", "xray continua", "radio loud agn", "accretion flow" |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, Dr R. Sambruna, 2008, 'XMM Observations of Intermediate-Luminosity BLRGs: Expanding the parameter space', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-748pc14 |