| Proposal ID | 015267 |
| Title | STUDY OF A COMPLETE SAMPLE OF BROAD LINE RADIO GALAXIES |
| Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0152670101 |
| DOI | https://doi.org/10.5270/esa-qhvtn0y |
| Principal Investigator, PI | Dr Paola Grandi |
| Abstract | We propose to pursue the spectral survey of Broad Line Radio Galaxies proposedin AO1 through the observation of 2 new sources. Previous X-ray observationshave shown that in BLRGs iron lines and reflections are weaker than in Seyfert1s. This result suggests that either: 1) a non-thermal continuum possiblyassociated with the core radiation emission dilutes the Seyfert-like emission;or 2) the physical conditions of the accretion flow in radio-loud type I AGNsare different. Our first XMM-Newton observation (Pictor A) has revealed a coldnarrow iron line and a very small UV bump, confirming the discrepancy with aSeyfert-like picture. More XMM-Newton observations are necessary to definitivelyestablish the physical geometrical reasons of the BLRG-Seyfert 1 differences. |
| Publications |
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| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2003-10-19T23:09:26Z/2003-10-20T14:59:52Z |
| 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 | 2004-11-11T00:00:00Z |
| Last Update | 2025-01-27 |
| Keywords | "spectral survey", "blrg seyfert", "radio loud type", "physical conditions", "complete sample", "broad line radiogalaxy", "physical geometrical reasons", "blrgs iron lines", "xmm newton", "uv bump", "seyfert 1s", "XMM-Newton", "XMM", "nonthermal continuum", "accretion flow" |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, Dr Paola Grandi, 2004, 'STUDY OF A COMPLETE SAMPLE OF BROAD LINE RADIO GALAXIES', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-qhvtn0y |