A dataset provided by the European Space Agency

Name 079060
Title NUSTAR-XMM MONITORING OF THE BROAD-LINE RADIO GALAXY 3C 382
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0790600101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0790600201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0790600301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0790600401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0790600501

DOI 10.5270/esa-y9igmoj
Author Mr FRANCESCO URSINI
Description We propose a joint NuSTAR-XMM monitoring of the broad-line radio galaxy (BLRG) 3C 382, consisting of 5x20 ks observations spaced by 10-15 days. 3C 382 is an ideal radio-loud source to obtain high sensitivity measurements over a broad (UV-hard X-rays) high-energy range, which will allow us to: 1) study the UV-X-ray spectrum of a BLRG with unprecedented accuracy and test physically motivated Comptonization models, 2) understand the origin of the puzzling reflection component, and 3) investigate the nature of the soft X-ray excess. These observations will allow for a direct comparison with radio-quiet Seyfert 1s, in particular with a similar, successful NuSTAR-XMM monitoring of NGC 4593.
Publication The 3CR Chandra Snapshot Survey: Extragalactic Radio Sources with Redshifts between 1 and 1.5 . Stuardi, C., Missaglia, V., et all. . ApJS . 235-32 . 2018 . 2018ApJS..235...32S ,
Radio-X-ray monitoring of the broad-line radio galaxy 3C 382. High-energy view with XMM-Newton and NuSTAR . Ursini, F., Petrucci, P.-O., et all. . MNRAS . 478-2663 . 2018 . 2018MNRAS.478.2663U ,
Relation between winds and jets in radio-loud AGN . Mehdipour, Missagh, Costantini, Elisa, . A&A . 625-25 . 2019 . 2019A&A...625A..25M ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2016-08-29T16:30:04Z/2016-10-17T12:27:47Z
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 2017-11-02T23:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2017-11-02T23:00:00Z, 079060, 17.56_20190403_1200. https://doi.org/10.5270/esa-y9igmoj