Proposal ID | 002274 |
Title | A hard X-ray survey in the Lockman Hole |
Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0022740101 |
DOI | https://doi.org/10.5270/esa-mn9mz1e |
Principal Investigator, PI | Dr Xavier Barcons |
Abstract | We propose to carry out a deep survey in hard X-rays in the Lockman Hole by complementing the 150 ksec of the PV phase observations with another 200 ksec.The scientific goals include: 1. testing the AGN origin of the X-ray background by detecting hard X-rays in all soft X-ray sources, 2. test specific unified scheme models for the XRB, 3. detection of ~30 Compton-thick AGN in hard X-rays,4. detection of the hard X-ray sources missing in soft X-ray surveys, 5. direct determination of hard X-ray source counts down to a 2-10 keV 2E-15 erg/cm2/s and6. determination, via fluctuation analyses, of 2-10 keV source counts to muchfainter fluxes. |
Publications |
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Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2001-10-25T07:21:55Z/2001-11-04T20:02:52Z |
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 | 2003-01-09T00:00:00Z |
Last Update | 2025-01-27 |
Keywords | "kev source counts", "soft xray sources", "compton thick agn", "hard xray", "soft xray surveys", "agn origin", "pv phase", "lockman hole", "kev 2e", "via fluctuation analyses", "deep survey", "fainter fluxes", "xray background", "hard xray survey" |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, Dr Xavier Barcons, 2003, 'A hard X-ray survey in the Lockman Hole', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-mn9mz1e |