A dataset provided by the European Space Agency

Name: ILLUMINATING THE DISK/CORONA/JET CONNECTION IN NLS1 GALAXIES
Published: 2017-11-23T23:00:00Z

Proposal ID	079086
Title	ILLUMINATING THE DISK/CORONA/JET CONNECTION IN NLS1 GALAXIES
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0790860101
DOI	https://doi.org/10.5270/esa-9q1yjha
Principal Investigator, PI	Dr LAURA BRENNEMAN
Abstract	We propose a 200-ks NuSTAR observation of the radio-loud narrow line Seyfert 1galaxy PMN J0948+0022, to be executed contemporaneously with an 80-ks XMM-Newtonobservation. The high accretion rate and rapid variability of NLS1s make themideal candidates in which to observe the disk/corona system, but there are onlya small handful of radio-loud members of this population. The broadband X-rayand optical/UV spectra we obtain, along with information from existing Fermi andradio campaigns, will allow us to address some of the key questions regardingthe physics of jet formation in this critical sample, such as the physicalconditions under which a jet can be launched, the relation of the jet to theputative corona in AGN, and correlations with the inner accretion flow.
Publications	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 Broadband X-ray observations of four gamma-ray narrow-line Seyfert 1 galaxies \|Berton M. Braito V. et al. \| A&A \| 632-120 \| 2019 \| 2019A&A...632A.120B \| http://ui.adsabs.harvard.edu/#abs/2019A&A...632A.120B 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 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	2016-11-04T00:50:46Z/2016-11-05T02:55:46Z
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	2025-01-27
Keywords	"xmm newton", "inner accretion flow", "broadband xray", "jet formation", "corona system", "nls1 galaxy", "existing fermi", "ideal candidates", "uv spectra", "accretion rate", "jet connection", "XMM-Newton", "NuSTAR", "galaxy pmn j0948", "rapid variability", "physical conditions", "radio loud", "XMM", "executed contemporaneously", "radio campaigns"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr LAURA BRENNEMAN, 2017, 'ILLUMINATING THE DISK/CORONA/JET CONNECTION IN NLS1 GALAXIES', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-9q1yjha