| Name | 011089 |
| Title | XMM Study of Ultrasoft Narrow-Line Seyfert 1 Galaxies SSC_4 |
| URL | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0110890101 |
| DOI | https://doi.org/10.5270/esa-hc8islm |
| Author | Dr Michael Watson |
| Description | GT- We propose to extend X-ray studies of ultrasoft narrow-line Seyfert 1 galaxies (NLS1) by making XMM observations of the most interesting members of this class. The broad band, large effective area and high spectral resolution of XMM will allow the best X-ray studies of NLS1 to date. We will measure their soft and hard X-ray continua, their spectral features and their strong flux and spectral variability. |
| Publication | No observations found associated with the current proposal |
| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2000-07-31T01:41:10Z/2003-01-19T03:26:26Z |
| 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 | 2004-02-19T00:00:00Z |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, 2004-02-19T00:00:00Z, 011089, 17.56_20190403_1200. https://doi.org/10.5270/esa-hc8islm |