A dataset provided by the European Space Agency

Name: UV to hard X-ray spectroscopy of the prototype disk wind quasar, PDS 456
Published: 2018-05-09T22:00:00Z
License: https://creativecommons.org/licenses/by-nc/3.0/igo

Proposal ID	078069
Title	UV to hard X-ray spectroscopy of the prototype disk wind quasar, PDS 456
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0780690201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0780690301
DOI	https://doi.org/10.5270/esa-xmrb5dg
Principal Investigator, PI	Dr James Reeves
Abstract	PDS 456, the most luminous nearby AGN, is now recognised as the prototype ultrafast outflow. Our recent XMM-Newton and NuSTAR campaign on PDS 456 establishedthe presence of a fast (0.3c), wide angle disk wind, sufficient to providesignificant mechanical feedback into its host galaxy. The new RGS data haverevealed the presence of variable, broad soft X-ray absorption lines from thedisk wind, which may be associated to the partial covering absorber. Here wepropose for 2x80 ks XMM-Newton observations of PDS 456 and a two orbit HST/COSsnapshot which will simultaneously measure the wind in the UV and X-rays. Therequested observations will be concurrent with a likely Astro-H observationduring 2016. For the first time we will obtain high resolution coverage of the wind from the UV to hard X-rays.
Publications	A New Relativistic Component of the Accretion Disk Wind in PDS 456 \|Reeves J. N. Braito V. et al. \| ApJ \| 854-8 \| 2018 \| 2018ApJ...854L...8R \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...854L...8R Resolving the X-Ray Obscuration in a Low-flux Observation of the Quasar PDS 456 \|Reeves J. N. Braito V. et al. \| ApJ \| 867-38 \| 2018 \| 2018ApJ...867...38R \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...867...38R Ionized outflows from active galactic nuclei as the essential elements of feedback \|Laha Sibasish Reynolds Christopher S. et al. \| NatAs \| 5-13 \| 2021 \| 2021NatAs...5...13L \| http://ui.adsabs.harvard.edu/#abs/2021NatAs...5...13L 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 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 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 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2017-03-23T18:38:38Z/2017-03-26T06:29:31Z
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	2018-05-09T22:00:00Z
Last Update	2026-07-09
Keywords	"2x80 xmm newton", "hard xray", "XMM-Newton", "pds 456 established", "luminous nearby agn", "hard xray spectroscopy", "disk wind", "cos snapshot", "rgs data", "NuSTAR", "XMM", "HST", "pds 456", "mechanical feedback", "orbit hst", "nustar campaign", "resolution coverage", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr James Reeves, 2018, 'UV to hard X-ray spectroscopy of the prototype disk wind quasar, PDS 456', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-xmrb5dg
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.