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
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 X\\u2011ray 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
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.
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
