A dataset provided by the European Space Agency

Name: One day in the extraordinary life of the first gamma-ray NLS1: PMN J0948+0022
Published: 2012-06-17T00:00:00Z

Proposal ID	067373
Title	One day in the extraordinary life of the first gamma-ray NLS1: PMN J0948+0022
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673730101
DOI	https://doi.org/10.5270/esa-n3qrjxl
Principal Investigator, PI	Dr Filippo DAmmando
Abstract	The discovery by Fermi-LAT of variable gamma-ray emission from 4 radio-loudNarrow Line Seyfert 1 revealed the presence of an emerging third class ofgamma-ray emitting AGNs. This poses intriguing questions on the knowledge of theUnified model of AGNs, the development of relativistic jets, the disc/jetconnection, and the evolution of radio-loud AGNs. We propose a 90 ksecXMM-Newton observation of the first RL-NLS1 detected in gamma-rays by Fermi-LAT:PMN J0948+0022. The XMM-Newton satellite, thanks to the high sensitivity of theEPIC cameras and the broad band coverage from optical to X-rays, creates aperfect synergy with Fermi for a complete understanding of properties of thisprototypical gamma-ray radio-loud Narrow Line Seyfert 1.
Publications	Multiwavelength observations of the gamma-ray-emitting narrow-line Seyfert 1 PMN J0948+0022 in 2011 \|DAmmando F. Larsson J. et al. \| MNRAS \| 438-3521 \| 2014 \| 2014MNRAS.438.3521D \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.438.3521D The XMM-Newton view of the radio-loud narrow-line Seyfert 1 galaxy PMN J0948+0022 \|Bhattacharyya Subir Bhatt Himali et al. \| MNRAS \| 440-106 \| 2014 \| 2014MNRAS.440..106B \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.440..106B Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov V. N. \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y Properties of flat-spectrum radio-loud narrow-line Seyfert 1 galaxies \|Foschini L. Berton M. et al. \| A&A \| 575-13 \| 2015 \| 2015A&A...575A..13F \| http://ui.adsabs.harvard.edu/#abs/2015A&A...575A..13F The most powerful flaring activity from the NLSy1 PMN J0948+0022 \|DAmmando F. Orienti M. et al. \| MNRAS \| 446-2456 \| 2015 \| 2015MNRAS.446.2456D \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.446.2456D XMM-Newton publication statistics \|Ness J.-U. Parmar A. N. et al. \| AN \| 335-210 \| 2014 \| 2014AN....335..210N \| http://ui.adsabs.harvard.edu/#abs/2014AN....335..210N The Tight Relation between X-Ray and Ultraviolet Luminosity of Quasars \|Lusso E. Risaliti G. \| ApJ \| 819-154 \| 2016 \| 2016ApJ...819..154L \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...819..154L The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch Eric W. \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F A new sample of X-ray selected narrow emission-line galaxies. II. Looking for True Seyfert 2 \|Pons E. Watson M. G. \| A&A \| 594-72 \| 2016 \| 2016A&A...594A..72P \| http://ui.adsabs.harvard.edu/#abs/2016A&A...594A..72P AGN spectral states from simultaneous UV and X-ray observations by XMM-Newton \|Svoboda J. Guainazzi M. \| A&A \| 603-127 \| 2017 \| 2017A&A...603A.127S \| http://ui.adsabs.harvard.edu/#abs/2017A&A...603A.127S 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 Relativistic Jets in Gamma-Ray-Emitting Narrow-Line Seyfert 1 Galaxies \|DAmmando Filippo \| Galax \| 7-87 \| 2019 \| 2019Galax...7...87D \| http://ui.adsabs.harvard.edu/#abs/2019Galax...7...87D A Luminous X-Ray Transient in SDSS J143359.16+400636.0: A Likely Tidal Disruption Event \|Brightman Murray Ward Charlotte et al. \| ApJ \| 909-102 \| 2021 \| 2021ApJ...909..102B \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...909..102B 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 X-ray emission from a rapidly accreting narrow-line Seyfert 1 galaxy at z = 6.56 \|Wolf J. Nandra K. et al. \| A&A \| 669-127 \| 2023 \| 2023A&A...669A.127W \| http://ui.adsabs.harvard.edu/#abs/2023A&A...669A.127W 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	2011-05-28T11:20:57Z/2011-05-29T13:09:33Z
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	2012-06-17T00:00:00Z
Last Update	2025-01-27
Keywords	"rl nls1", "broad band coverage", "xmm newton", "xmm newton satellite", "poses intriguing", "fermi lat", "radio loud agns", "unified model", "gamma rays", "extraordinary life", "EPIC", "pmn j0948", "jet connection", "XMM-Newton", "perfect synergy", "gamma ray nls1", "relativistic jets", "XMM", "epic cameras"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Filippo D'Ammando, 2012, 'One day in the extraordinary life of the first gamma-ray NLS1: PMN J0948+0022', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-n3qrjxl