A dataset provided by the European Space Agency

Proposal ID 015087
Title Spectroscopy of Z>4 Quasars
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https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0150870201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0150870301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0150870401

DOI https://doi.org/10.5270/esa-egx7fkg
Principal Investigator, PI Prof Jill Bechtold
Abstract We propose to measure the X-ray spectra of 5 quasars with z>4. We have carriedout a survey of 14 optically bright, radio-quiet z>4 quasars using short ChandraACIS-S exposures. From the measured fluxes, we can estimate exposure timesrequired for spectroscopy. To date, only four z>4 quasars have X-rayspectroscopy, and all 4 are radio-loud blazars. Our sample includes one z=5quasar, and we ask for a deep exposure which may detect its flux to 60 keV inthe rest frame. We can test whether the high energy turnover seen in localSeyferts is present in this z=5 quasar. The only other z>5 quasar with ameasured X-ray flux is too faint to obtain spectroscopy in a reasonable exposuretime.
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2002-12-20T01:42:09Z/2003-07-15T14:26:39Z
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 2004-11-18T00:00:00Z
Last Update 2025-01-27
Keywords "reasonable exposure time", "sample includes z", "short chandra acis", "xray spectroscopy", "optically bright", "local seyferts", "radio quiet z", "energy turnover", "rest frame", "xray flux", "radio loud blazar", "xray spectra", "deep exposure"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Prof Jill Bechtold, 2004, 'Spectroscopy of Z>4 Quasars', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-egx7fkg