A dataset provided by the European Space Agency

Name: NUSTAR/XMM MONITORING OF THE BROAD-LINE RADIO GALAXY 3C 382
Published: 2017-11-02T23:00:00Z

Proposal ID	079060
Title	NUSTAR/XMM MONITORING OF THE BROAD-LINE RADIO GALAXY 3C 382
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0790600101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0790600201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0790600301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0790600401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0790600501
DOI	https://doi.org/10.5270/esa-y9igmoj
Principal Investigator, PI	Mr FRANCESCO URSINI
Abstract	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. 3C382 is an ideal radio-loud source to obtain high sensitivity measurementsover 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 testphysically motivated Comptonization models, 2) understand the origin of thepuzzling reflection component, and 3) investigate the nature of the softX-ray excess. These observations will allow for a direct comparison withradio-quiet Seyfert 1s, in particular with a similar, successful NuSTAR/XMMmonitoring of NGC 4593.
Publications	The 3CR Chandra Snapshot Survey: Extragalactic Radio Sources with Redshifts between 1 and 1.5 \|Stuardi C. Missaglia V. et al. \| ApJS \| 235-32 \| 2018 \| 2018ApJS..235...32S \| http://ui.adsabs.harvard.edu/#abs/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 al. \| MNRAS \| 478-2663 \| 2018 \| 2018MNRAS.478.2663U \| http://ui.adsabs.harvard.edu/#abs/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 \| http://ui.adsabs.harvard.edu/#abs/2019A&A...625A..25M Classification of 4XMM-DR9 sources by machine learning \|Zhang Yanxia Zhao Yongheng \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z Fundamental X-ray corona parameters of Swift/BAT AGN \|Hinkle Jason T. Mushotzky Richard \| MNRAS \| 506-4960 \| 2021 \| 2021MNRAS.506.4960H \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.506.4960H X-Ray Coronal Properties of Swift/BAT-selected Seyfert 1 Active Galactic Nuclei \|Kamraj Nikita Brightman Murray et al. \| ApJ \| 927-42 \| 2022 \| 2022ApJ...927...42K \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...927...42K Soft excess in AGN with relativistic Xu2011ray reflection \|Ezhikode Savithri H. Shyam Prakash V. P. et al. \| AN \| 344-20230042 \| 2023 \| 2023AN....34430042E \| http://ui.adsabs.harvard.edu/#abs/2023AN....34430042E The Reliability of Accretion Disk Inclination Derived from X-Ray Spectroscopy of Active Galaxies \|Du Rong Ding Yuanze et al. \| ApJ \| 963-152 \| 2024 \| 2024ApJ...963..152D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...963..152D The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII O VIII and Fe L-shell Transitions \|Pan Zeyang Qu Zhijie et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez Antonio C. \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
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 Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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
Last Update	2025-01-27
Keywords	"3c 382", "sensitivity measurements", "energy range", "soft xray excess", "hard xray", "reflection component", "broad uv", "NGC 4593", "NuSTAR", "ngc 4593", "successful nustar", "XMM", "x ray spectrum"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mr FRANCESCO URSINI, 2017, 'NUSTAR/XMM MONITORING OF THE BROAD-LINE RADIO GALAXY 3C 382', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-y9igmoj