A dataset provided by the European Space Agency

Name: Is the Relativistic Fe K Line in the High-Luminosity Quasar RBS 1423 Persistent?
Published: 2015-02-27T23:00:00Z

Proposal ID	072324
Title	Is the Relativistic Fe K Line in the High-Luminosity Quasar RBS 1423 Persistent?
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723240101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723240201
DOI	https://doi.org/10.5270/esa-ttdu01w
Principal Investigator, PI	Dr Tahir Yaqoob
Abstract	RBS 1423 is one of only a few high-luminosity QSO with a relativisticallybroadened Fe K line, which was found by Krumpe et al. (2007) from a 20 ks XMMobservation. The QSO is an important case study for probing the inner accretiondisk and strong gravity regime in high-luminosity QSO, and potentially theblack-hole spin. We propose another XMM 20 ks snapshot to investigate if the FeK line is persistent or variable. This will help to strategize future longerfollow-ups since a varaiable line would benefit from a monitoring program,whereas a deep exposure to better constrain the accretion disk and black-holespin would be more appropriate for a persistent line.
Publications	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 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 The composite X-ray spectra of radio-loud and radio-quiet SDSS quasars \|Zhou Min-Hua Gu Min-Feng \| RAA \| 21-4 \| 2021 \| 2021RAA....21....4Z \| http://ui.adsabs.harvard.edu/#abs/2021RAA....21....4Z 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	2014-01-06T11:34:50Z/2014-02-10T23:31:28Z
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	2015-02-27T23:00:00Z
Last Update	2025-01-27
Keywords	"accretion disk", "strategize future", "gravity regime", "luminosity qso", "varaiable line", "inner accretion disk", "blackhole spin", "relativistically broadened fe", "rbs 1423", "XMM", "relativistic fe", "deep exposure"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Tahir Yaqoob, 2015, 'Is the Relativistic Fe K Line in the High-Luminosity Quasar RBS 1423 Persistent?', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-ttdu01w