
| Proposal ID | 040232 |
| Title | X-ray spectral characterization of optically selected narrow-line Seyfert 1 gal |
| Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0402320101 |
| DOI | https://doi.org/10.5270/esa-v56zug2 |
| Principal Investigator, PI | Dr Luigi Foschini |
| Abstract | We propose the observation with XMM-Newton of a sample of 12 optically selectedNarrow-Line Seyfert 1 galaxies (NLS1) discovered in the Sloan Digital Sky Survey(SDSS) and never observed in X-rays. The key aim of this project is the study ofthe X-ray spectral properties and correlations of optically selected NLS1. Thesuperior capabilities of XMM will allow to deconvolve spectral components ifappropriate. The results will be compared with those of X-ray selected NLS1samples and classical Seyfert-1s to discuss/infer systematic trends of the X-rayspectral shape as a function of the FWHM of (Hbeta) which, combined withluminosity, allows to estimate the Eddington ratio and the mass of the centralblack hole. |
| Publications |
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| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2007-02-02T17:58:35Z/2007-02-03T01:44:22Z |
| Version | 21.51_20241115_1113 |
| 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 | 2008-03-10T00:00:00Z |
| Last Update | 2026-06-19 |
| Keywords | "xray spectral properties", "infer systematic trends", "deconvolve spectral components", "XMM", "xmm newton", "narrow line seyfert", "classical seyfert 1s", "nls1 samples", "xray spectral shape", "XMM-Newton", "central black hole", "galaxy nls1", "eddington ratio", "SDSS" |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, Dr Luigi Foschini, 2008, 'X-ray spectral characterization of optically selected narrow-line Seyfert 1 gal', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-v56zug2 |
| Rights | Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license. |