A dataset provided by the European Space Agency

Name: Investigating Time Lags In Reflection-Dominated AGN
Published: 2018-07-19T22:00:00Z
License: https://creativecommons.org/licenses/by-nc/3.0/igo

Proposal ID	080151
Title	Investigating Time Lags In Reflection-Dominated AGN
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0801510101
DOI	https://doi.org/10.5270/esa-o3t5315
Principal Investigator, PI	Dr Abderahmen Zoghbi
Abstract	Iron K relativistic reverberation has been observed in several AGN, with delayscomparable to the light crossing time very close to the black hole. In thisframework, objects with no reflection or with reflection only spectra shouldshow no relativistic reverberation. An object with no reflection was the targetof a previous accepted XMM proposal. This proposal explores the case of areflection- only source. We request a 120 ks observation of thereflection-dominated MRK 478, a highly variable object whosereflection-dominated state is brighter than other objects in similar state. Thegoal is to directly test the prediction of relativistic reverberation that nodirect-to-reflected delay is present. The data will allows us to search for second order delays in the reflected emission itself.
Publications	Low-mass Active Galactic Nuclei on the Fundamental Plane of Black Hole Activity \|Qian Lei Dong Xiao-Bo et al. \| ApJ \| 860-134 \| 2018 \| 2018ApJ...860..134Q \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...860..134Q Multi-epoch X-ray spectral analysis of the narrow-line Seyfert 1 galaxy Mrk 478 \|Waddell S. G. H. Gallo L. C. et al. \| MNRAS \| 489-5398 \| 2019 \| 2019MNRAS.489.5398W \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.489.5398W 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 Correlated variability of the reflection fraction with the X-ray flux and spectral index for Mrk 478 \|Barua Samuzal Jithesh V. et al. \| MNRAS \| 517-801 \| 2022 \| 2022MNRAS.517..801B \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.517..801B A Systematic Study of the Short-term X-Ray Variability of Seyfert Galaxies. I. Diversity of the X-Ray rms Spectra \|Hu Jingwei Jin Chichuan et al. \| ApJ \| 936-105 \| 2022 \| 2022ApJ...936..105H \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...936..105H 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 Search for Young Stellar Objects within 4XMM-DR13 Using CatBoost and SPE \|Ma Xiangyao Zhang Yanxia et al. \| AJ \| 168-210 \| 2024 \| 2024AJ....168..210M \| http://ui.adsabs.harvard.edu/#abs/2024AJ....168..210M New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D Windy or Not: Radio Parsec-scale Evidence for a Broad-line Region Wind in Radio-quiet Quasars \|Chen Sina Laor Ari et al. \| ApJ \| 975-35 \| 2024 \| 2024ApJ...975...35C \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...975...35C
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2017-06-30T18:55:38Z/2017-07-02T08:30:38Z
Version	21.51_20241115_1113
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	2018-07-19T22:00:00Z
Last Update	2026-07-09
Keywords	"relativistic reverberation", "light crossing time", "investigating time lags", "reflected emission", "black hole", "delays comparable", "XMM", "reflected delay", "reflection dominated agn", "variable object", "reflection dominated"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Abderahmen Zoghbi, 2018, 'Investigating Time Lags In Reflection-Dominated AGN', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-o3t5315
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.