A dataset provided by the European Space Agency

Name 078327
Title The XMM-Newton PG-Bright Quasar Survey Legacy Program
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0783270101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0783270201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0783270401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0783271401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0783272101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0783272701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0783272801

DOI https://doi.org/10.5270/esa-0uig7t3
Author European Space Agency
Description We propose to obtain high S/N XMM/EPIC spectra of 28 PG quasars in order to
complete the coverage of the Bright Quasar Survey (PG) sample of 87 z<0.5
quasars. This sample has been a cornerstone for studies of quasars in the past
40 years. Some of the immediate questions we plan to address with the complete
sample are: What produces the soft X-ray excess, which occurs universally around
0.5 keV? What controls the strength of the FeKa line? What is the relation of UV
and X-ray absorbers? We also request 5 joint HST orbits to complete the UV
coverage of this sample. This XMM Legacy Program will establish the most
accurate, complete, and high quality data set of the 0.3-10 keV emission
properties of quasars and will provide the base for detailed studies of physical processes in type 1 AGN.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2016-11-16T14:17:33Z/2017-01-28T10:37:03Z
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 2018-03-29T22:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2018, The Xmm-Newton Pg-Bright Quasar Survey Legacy Program, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-0uig7t3