A dataset provided by the European Space Agency

Name 067013
Title X-ray Reverberation Mapping: Ark 564
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670130201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670130301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670130401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670130501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670130601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670130701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670130801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670130901

DOI https://doi.org/10.5270/esa-5s69vkb
Author European Space Agency
Description Recent progress mapping AGN accretion disks reveals X-ray continuum
reverberation from material at a few hundred Schwarzschild radii in NGC 4051. We
have further demonstrated that claims of reverberation in 1H0707-495 from
ultra-small radii, on the scale of the event horizon, are incorrect: like NGC
4051, this AGN may be understood as exhibiting X-ray reverberation from material
further out. Ark 564 is known to exhibit large time delays when analyzed over
long timescales, and, like 1H0707-495, shows negative time lags on the fastest
variability timescales. We propose eight 55 ks observations of Ark 564 to
thoroughly test the reverberation model, measure the transfer function and to
derive strong constraints on the location and distribution of the X-ray reprocessor.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2011-05-24T05:56:05Z/2011-07-01T22:17:46Z
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 2012-07-21T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2012, X-Ray Reverberation Mapping: Ark 564, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-5s69vkb