Name | 014526 |
Title | Uncovering bright heavily absorbed type 1 AGN |
URL | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0145260301 |
DOI | https://doi.org/10.5270/esa-vvh1klu |
Author | European Space Agency |
Description | We propose to carry out a snapshot survey of 6 luminous and X-ray bright broad line AGN (5 Seyfert 1 and 1 QSO) with very hard X-ray colours and hence, probably strongly absorbed in X-rays. We want to study their X-ray spectra (continuum and Fe K lines) to measure the column density and to understand the nature of the X-ray absorber and the geometry of their central regions. These sources could provide bright examples of the optically unobscured but X-ray absorbed AGN that are routinely found in medium to deep X-ray surveys. |
Publication | No observations found associated with the current proposal |
Instrument | OM |
Temporal Coverage | 2003-11-17T10:15:03Z/2003-11-17T11:59:51Z |
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 | 2005-01-01T00:00:00Z |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, 2005, Uncovering Bright Heavily Absorbed Type 1 Agn, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-vvh1klu |