A dataset provided by the European Space Agency

Name 086209
Title The connection between the X-ray corona and the nuclear radio emission in AGN
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862090101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862090201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862090301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862090401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862090501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862090601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862090701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862090801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862090901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862091001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862091101
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https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862091201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862091301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862091401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862091501

DOI https://doi.org/10.57780/esa-n2w6qzy
Author Dr Claudio Ricci
Description We propose here the first joint study of the mm/X-ray variability of a
radio-quiet AGN, using XMM-Newton and ALMA to monitor the brightest unobscured
AGN in the southern sky, IC 4329A, observing it once per day over ten
consecutive days. The ALMA monitoring has already been approved (priority A,
highest resolution). This would be the first time such a monitoring is carried
out, and the detection of correlated mm/X-ray variability would be a crucial
proof of the coronal origin of the nuclear radio emission in radio-quiet AGN.
Besides, this would also be fundamental to understand the origin of the X-ray
emission, proving, for the first time, that the X-ray corona is
magnetically-heated.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2021-08-10T13:37:05Z/2021-08-19T23:03:37Z
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 2022-09-28T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Claudio Ricci, 2022, 086209, 19.16_20210326_1200, European Space Agency, https://doi.org/10.57780/esa-n2w6qzy