A dataset provided by the European Space Agency

Name: Completing the Missing X-ray Information of Newly Discovered gamma-ray NLS1
Published: 2017-11-22T23:00:00Z

Proposal ID	078409
Title	Completing the Missing X-ray Information of Newly Discovered gamma-ray NLS1
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784090201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784090301
DOI	https://doi.org/10.5270/esa-psouqcq
Principal Investigator, PI	Mr Su Yao
Abstract	As hybrids of NLS1s and blazars, the recently discovered gamma-ray emittingNLS1s excited a great interests to the AGN community. With relatively smallblack hole (BH) mass and accreting close to Eddington, these NLS1s provides anew perspective to investigate the properties and formation of jets and theircoupling with BH accretion. However, gamma-ray emitting NLS1s are rare and thereare only sevend significantly detected in the gamma-ray band and being studiedso far. We propose to observe a newly discovered gamma-ray NLS1 with XMM-Newtonin the X-ray, UV and optical bands. These observations will help to complete themissing X-ray spectral and temporal information and constructing its broad bandSED, which are crucial for modeling and constraining the jet parameters in this object.
Publications	SDSS J211852.96-073227.5: a new gamma-ray flaring narrow-line Seyfert 1 galaxy \|Yang, Hui, Yuan, Weimin, et al. \| MNRAS \| 477-5127 \| 2018 \| 2018MNRAS.477.5127Y \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.477.5127Y General Physical Properties of Gamma-Ray-emitting Narrow-line Seyfert 1 Galaxies \|Paliya, Vaidehi S., Parker, M. L., et al. \| ApJ \| 872-169 \| 2019 \| 2019ApJ...872..169P \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...872..169P A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies \|Ojha, Vineet, Chand, Hum, et al. \| ApJ \| 896-95 \| 2020 \| 2020ApJ...896...95O \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...896...95O 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 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	2016-05-10T12:18:46Z/2016-10-27T20:02:38Z
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	2017-11-22T23:00:00Z
Keywords	"gamma ray band", "temporal information", "agn community", "XMM", "optical bands", "missing xray information", "bh accretion", "accreting close", "gamma ray nls1", "jet parameters", "broad band sed", "XMM-Newton", "missing xray spectral", "blackhole bh mass", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mr Su Yao, 2017, 'Completing the Missing X-ray Information of Newly Discovered gamma-ray NLS1', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-psouqcq