A dataset provided by the European Space Agency

Name 088234
Title MAPPING GAS FLOWS IN THE AGN MRK 817 WITH XMM-NEWTON AND HST
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0882340601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0882340701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0882340801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0882340901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0882341001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0882341101

DOI https://doi.org/10.57780/esa-7q9dx81
Author European Space Agency
Description Knowledge of the structure and kinematics of gas around supermassive black holes
is vital to understanding accretion and thus AGN feedback. To this end, we, the
AGN STORM 2 team, have been awarded a Large 198-orbit Hubble Space Telescope
program and a Las Cumbres Observatory Key Project to measure reverberation lags
in Mrk 817. Previous UV/optical reverberation mapping campaigns have
successfully mapped the outer accretion disc and broad line region, but reveal
that X-rays (thought to be the primary driver of multi-wavelength variability)
do not correlate with longer wavelengths as well as expected. X-ray spectral and
timing measurements are necessary to track changes in the geometry and dynamics
of the inner accretion flow that likely affect our inference of the outer disc and outflow str
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2021-04-18T21:09:38Z/2021-10-28T22:41:26Z
Version 19.16_20210326_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 2022-11-16T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2022, Mapping Gas Flows In The Agn Mrk 817 With Xmm-Newton And Hst, 19.16_20210326_1200, European Space Agency, https://doi.org/10.57780/esa-7q9dx81