A dataset provided by the European Space Agency

Name: Changing look AGN caught in the act
Published: 2017-11-23T23:00:00Z

Proposal ID	078345
Title	Changing look AGN caught in the act
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0783450101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0783450201
DOI	https://doi.org/10.5270/esa-gwi2joz
Principal Investigator, PI	Dr Magdalena Kunert-Bajraszewska
Abstract	A recent multi-year Jansky VLA legacy program, the Caltech-NRAO Stripe 82 Survey(CNSS), revealed several radio transient sources on timescales of 5-20 years,largely associated with renewed AGN activity. The rates of such AGN possiblyimply episodes of enhanced accretion and jet activity occurring once every40,000 years in these galaxies. Since X-rays may originate from the base ofrelativistic jets, we expect X-ray flares to be associated with the radiobrightening. The proposed observations could then result in the first X-raydetection of the changing look AGN.
Publications	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 Caltech-NRAO Stripe 82 Survey (CNSS). V. AGNs That Transitioned to Radio-loud State \|Wou0142owska Aleksandra Kunert-Bajraszewska Magdalena et al. \| ApJ \| 914-22 \| 2021 \| 2021ApJ...914...22W \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...914...22W 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 Search for Young Stellar Objects within 4XMM-DR13 Using CatBoost and SPE \|Ma Xiangyao Zhang Yanxia et al. \| AJ \| 168-210 \| 2024 \| 2024AJ....168..210M \| http://ui.adsabs.harvard.edu/#abs/2024AJ....168..210M New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2016-05-23T07:05:29Z/2016-11-12T19:53:58Z
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	2017-11-23T23:00:00Z
Last Update	2025-08-04
Keywords	"radio transient sources", "enhanced accretion", "jet activity occurring", "changing look", "radio brightening", "renewed agn activity", "jansky vla", "expect xray flare", "xray detection", "relativistic jets"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Magdalena Kunert-Bajraszewska, 2017, 'Changing look AGN caught in the act', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-gwi2joz