A dataset provided by the European Space Agency

Name 072011
Title Deciphering AGN outflows: multiwavelength monitoring of NGC 5548
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0720110301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0720110401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0720110501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0720110601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0720110701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0720110801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0720110901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0720111001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0720111101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0720111201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0720111301
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https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0720111401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0720111501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0720111601

DOI https://doi.org/10.5270/esa-ftzxscj
Author European Space Agency
Description AGN outflows couple supermassive black holes to their environments. Using an
ambitious multiwavelength campaign on NGC 5548, (XMM-Newton, HST, Swift, and
optical) we propose to achieve a new level of physical understanding for these
enigmatic winds by obtaining the deepest RGS spectrum of any AGN, allowing us to
determine the ionisation structure of the gas. Using EPIC data we will measure
the response of the outflow to continuum variations, which combined with HST/COS
data determines unambiguously the location and tomography of the outflow
components. Time-dependent UV and X-ray continuum variations will constrain the
geometry and physics close to the black hole. Our team pioneered this approach,
and recently applied it successfully (12 refereed papers) to Mrk 509.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2013-06-22T04:10:29Z/2014-02-05T01:23:43Z
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 2015-02-27T23:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2015, Deciphering Agn Outflows: Multiwavelength Monitoring Of Ngc 5548, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-ftzxscj