A dataset provided by the European Space Agency

Name: Testing the AGN unified theory with XMM observations of PBC J2333.9-2343
Published: 2016-11-23T23:00:00Z

Proposal ID	076099
Title	Testing the AGN unified theory with XMM observations of PBC J2333.9-2343
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0760990101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0760990201
DOI	https://doi.org/10.5270/esa-ukrh7ep
Principal Investigator, PI	Dr Pietro Parisi
Abstract	The leading theory on the nature of AGNs holds that the different observed typesof AGNs are basically the same kind of source. Some observations reveal someobjects that do not follow this scheme. One such object is PBC J2333.9-2343which has three different classifications if observed in Radio (blazar), X-ray(Type 1 AGN) or optical (Type 2 AGN) wavebands. The only way to unveil thenature of this peculiar source is through X-ray observations complemented byquasi simultaneous optical and radio coverage. If this proposal will beaccepted, we will plan to ask time at the VLBA within February 1, 2015, andoptical at the San Pedro Martir telescope, in order to have almost simultaneouscoverage in the X-ray, radio and optical wavebands. These data will be used to test and refine the unification model.
Publications	Restarting activity in the nucleus of PBC J2333.9-2343. An extreme case of jet realignment \|Hernandez-Garcia, L., Panessa, F., et al. \| A&A \| 603-131 \| 2017 \| 2017A&A...603A.131H \| http://ui.adsabs.harvard.edu/#abs/2017A&A...603A.131H Galactic Sources Detected in the NuSTAR Serendipitous Survey \|Tomsick, John A., Lansbury, George B., et al. \| ApJS \| 230-25 \| 2017 \| 2017ApJS..230...25T \| http://ui.adsabs.harvard.edu/#abs/2017ApJS..230...25T Variable broad lines and outflow in the weak blazar PBC J2333.9-2343 \|Hernandez-Garcia, L., Vietri, G., et al. \| MNRAS \| 478-4634 \| 2018 \| 2018MNRAS.478.4634H \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.478.4634H Hard X-ray-selected giant radio galaxies - I. The X-ray properties and radio connection \|Ursini, F., Bassani, L., et al. \| MNRAS \| 481-4250 \| 2018 \| 2018MNRAS.481.4250U \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.481.4250U 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 High-energy Emission Component, Population, and Contribution to the Extragalactic Gamma-Ray Background of Gamma-Ray-emitting Radio Galaxies \|Fukazawa, Yasushi, Matake, Hiroto, et al. \| ApJ \| 931-138 \| 2022 \| 2022ApJ...931..138F \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...931..138F Relationship between gamma-ray loudness and X-ray spectra of radio galaxies \|Kayanoki, Taishu, Fukazawa, Yasushi, \| PASJ \| 74-791 \| 2022 \| 2022PASJ...74..791K \| http://ui.adsabs.harvard.edu/#abs/2022PASJ...74..791K Multiwavelength monitoring of the nucleus in PBC J2333.9-2343: the giant radio galaxy with a blazar-like core \|Hern\\u00e1ndez-Garc\\u00eda, L., Panessa, F., et al. \| MNRAS \| 525-2187 \| 2023 \| 2023MNRAS.525.2187H \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.525.2187H 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	2015-05-15T04:50:01Z/2015-11-17T15:24:27Z
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	2016-11-23T23:00:00Z
Keywords	"XMM", "unification model", "J2333.9", "agn wavebands", "leading theory", "xray type", "optical wavebands", "agn unified theory", "radio coverage", "radio blazar", "optical type", "pbc j2333", "agns holds"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Pietro Parisi, 2016, 'Testing the AGN unified theory with XMM observations of PBC J2333.9-2343', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-ukrh7ep