A dataset provided by the European Space Agency

Name: Probing the response of warm-absorbers to the variable continuum in PG1404+226
Published: 2017-02-25T23:00:00Z

Proposal ID	076348
Title	Probing the response of warm-absorbers to the variable continuum in PG1404+226
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763480101
DOI	https://doi.org/10.5270/esa-zdkyws3
Principal Investigator, PI	Dr Gulab Dewangan
Abstract	We request 110ks XMM-Newton observation of the highly variable, narrow-linequasar PG1404+226. The existing short 21ks XMM-Newton observation has revealedhigh velocity (>=25000 km/s), variable absorption features in the 1-3keV rangedue to NeIX and SXVI. The absorption lines were weaker at lower flux. Theprimary objective is to determine the response of the high velocity warmabsorbing gas to the variable continuum and put tight constraints on the densityand the location of the WA gas. The long observation will also allow us to studyvariability of the soft excess, hard power-law and UV emission and proberelationship between them in this extreme quasar.
Publications	Large-amplitude Rapid X-Ray Variability in the Narrow-line Seyfert 1 Galaxy PG 1404+226 \|Mallick L. Dewangan G. C. \| ApJ \| 863-178 \| 2018 \| 2018ApJ...863..178M \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...863..178M 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 Xu2011HESS: A large sample of highly accreting serendipitous AGN under the XMMu2011Newton microscope \|Laurenti M. Tombesi F. et al. \| AN \| 344-20230053 \| 2023 \| 2023AN....34430053L \| http://ui.adsabs.harvard.edu/#abs/2023AN....34430053L 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	2016-01-25T11:14:30Z/2016-01-26T15:51:09Z
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	2017-02-25T23:00:00Z
Last Update	2025-01-27
Keywords	"variable continuum", "wa gas", "variable absorption", "tight constraints", "warm absorbers", "lower flux", "hard power law", "xmm newton", "absorption lines", "110 xmm newton", "XMM-Newton", "primary objective", "uv emission", "probe relationship", "existing short", "3kev range", "soft excess", "XMM"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Gulab Dewangan, 2017, 'Probing the response of warm-absorbers to the variable continuum in PG1404+226', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-zdkyws3