A dataset provided by the European Space Agency

Name 014792
Title The complete Piccinotti AGN sample
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0147920101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0147920301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0147920401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0147920601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0147920701

DOI https://doi.org/10.5270/esa-z8a541d
Author European Space Agency
Description The Piccinotti survey contains the only existing hard (2-10 keV) X-ray selected
sample of bright AGNs. Therefore it plays a basic role in our knowledge of the
statistical distribution of spectral properties of AGN, e.g. intrinsic
absorption, soft excess, absorption edges, emission lines, or warm absorbers.
The distribution of these properties is fundamental for the understanding of
the two main cosmological measurements in the X-ray region: the background and
the log N -- log S relation of X-ray sources, because both are dominated by
AGN. Although the Piccinotti sample contains only 33 sources, 6 of them are
not part of the AO-1 program. Given the brightness of the sources and the
importance of the sample, we propose to observe these six sources.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2002-11-18T23:28:25Z/2003-08-21T08:45:02Z
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 2004-09-24T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2004, The Complete Piccinotti Agn Sample, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-z8a541d