A dataset provided by the European Space Agency

Name 084383
Title X-RAY SPECTROSCOPIC SURVEY OF HIGHLY-ACCRETING AGN
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0843830101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0843830201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0843830301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0843830401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0843830501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0843830601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0843830701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0843830801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0843830901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0843831001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0843831101
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https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0843831201

DOI https://doi.org/10.5270/esa-ltl9a1w
Author Dr Enrico Piconcelli
Description We propose here to perform X-ray spectroscopy of a sample of 13 optically-bright
AGN with an Eddington ratio virgul1 in a restricted range of redshift (z virgul 0.5-0.7),
SMBH mass (virgul1e8 Msun) and bolometric luminosity (virgul1e46 erg/s). Our program is
designed to significantly improve our understanding of the X-ray spectral
properties of highly-accreting AGN. Specifically, we aim at providing a
reference dataset for shedding definitive light on the hotly-debated,
recently-questioned correlations Edd_ratio vs. Gamma, and Edd_ratio vs. X-ray
bolometric correction. The current lack of data at Edd_ratio >virgul 1 indeed hampers
firm conclusions on the strength of these relations.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2019-05-05T21:05:48Z/2019-12-23T11:45:40Z
Version 18.00_20191217_1110
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 2021-02-03T23:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Enrico Piconcelli, 2021, 084383, 18.00_20191217_1110, European Space Agency, https://doi.org/10.5270/esa-ltl9a1w