Name | 008515 |
Title | A joint deep XMM-AXAF survey in the Lynx.3A field |
URL | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0085150101 |
DOI | https://doi.org/10.5270/esa-e9z42h1 |
Author | Prof A B |
Description | The ROSAT Ultradeep HRI Survey in the Lockman Hole has resolved 70-80 percent of the soft X-ray background (XRB) into discrete sources, most of which have been identified as AGN with the Keck including some type 2 AGN, which are thought to be responsible for the hard spectrum of the XRB. The space density of AGN apparently does not decline at z>3 like seen in optical and radio surveys. However, the sample statistics of a single deep fied is rather limited. The next generation X-ray deep surveys ideally combine XMM and AXAF observations of the same field. Here we propose a 150 ksec XMM survey of the Lynx.3A field, which will be observed for 190 ksec with AXAF. We will thus double the X-ray deep survey area and will obtain high quality XMM spectra of 25 and hardness ratios for 100 objects. |
Publication | No observations found associated with the current proposal |
Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2001-10-15T07:31:45Z/2001-10-22T09:09:36Z |
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 | 2003-01-03T00:00:00Z |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, 2003-01-03T00:00:00Z, 008515, 17.56_20190403_1200. https://doi.org/10.5270/esa-e9z42h1 |