A dataset provided by the European Space Agency

Name 084434
Title Shining light on obscuring outflows in AGN
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0844341301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0844341401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0844341501

DOI https://doi.org/10.57780/esa-jad4zk1
Author Prof Jelle Kaastra
Description AGN can be obscured by gas streams close to the black hole that shield remote
regions from ionising radiation. We witnessed such an event in NGC 5548 and NGC
3783 where 90% of the soft X-rays are blocked by a dense gas stream close to the
BLR. Our joint observations with XMM-Newton, NuSTAR and HST/COS showed UV broad
absorption lines associated with the X-ray absorption and allowed us to
characterise this unique obscuration event completely. We propose to investigate
a similar event in another Seyfert 1 using the same instruments. Swift
monitoring (98 ks) will be used to find the event, which will be characterised
by joint ToO observations with XMM-Newton (150 ks), HST/COS (4 orbits) and
NuSTAR (50 ks).
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2019-11-15T08:03:30Z/2019-12-06T12:37:09Z
Version 18.00_20191217_1110
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 2020-12-31T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Prof Jelle Kaastra, 2020, 084434, 18.00_20191217_1110, European Space Agency, https://doi.org/10.57780/esa-jad4zk1