A dataset provided by the European Space Agency

Name: Exploring the Disc-Jet Properties in the Most Super-Eddington Radio-Loud NLS1
Published: 2021-01-14T23:00:00Z

Proposal ID	084180
Title	Exploring the Disc-Jet Properties in the Most Super-Eddington Radio-Loud NLS1
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0841800201
DOI	https://doi.org/10.57780/esa-0g0qm1m
Principal Investigator, PI	Dr Chichuan Jin
Abstract	The mechanism of launching and powering relativistic jets in AGN is still notunderstood, but must link to the accretion flow. Evidence for this comes fromthe clear change in blazar jet properties at L/LEddvirgul0.01, probably due to theaccretion flow transition from a geometrically thick ADAF to a thin disc. Thereshould be another transition at L/LEdd > 1, where the accretion disc should puffup, but this is harder to study as few radio-loud AGN are super-Eddington. RXJ0134.2-4258 is a robust super-Eddington NLS1 with L/LEddvirgul11, the highest of allradio-loud AGN known. Therefore, we propose a joint XMM-Newton/NuSTAR program tostudy the accretion disc, corona and jet mechanism in this new radio-loudsuper-Eddington regime.
Publications	Multiwavelength campaign on the Super-Eddington NLS1 RX J0134.2-4258 - I. Peculiar X-ray spectra and variability \|Jin, Chichuan, Done, Chris, et al. \| MNRAS \| 512-5642 \| 2022 \| 2022MNRAS.512.5642J \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.512.5642J The extreme super-eddington NLS1 RX J0134.2-4258 - II. A weak-line Seyfert linking to the weak-line quasar \|Jin, Chichuan, Done, Chris, et al. \| MNRAS \| 518-6065 \| 2023 \| 2023MNRAS.518.6065J \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.518.6065J 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2019-12-19T06:18:32Z/2019-12-20T21:00:12Z
Version	18.00_20191217_1110
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	2021-01-14T23:00:00Z
Keywords	"NuSTAR", "XMM", "jet mechanism", "rx j0134", "geometrically thick adaf", "nustar program", "powering relativistic jets", "blazar jet properties", "J0134.2", "disc jet properties", "accretion disc", "accretion flow transition", "radio loud agn", "accretion flow", "XMM-Newton", "super eddington", "thin disc", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Chichuan Jin, 2021, 'Exploring the Disc-Jet Properties in the Most Super-Eddington Radio-Loud NLS1', 18.00_20191217_1110, European Space Agency, https://doi.org/10.57780/esa-0g0qm1m