A dataset provided by the European Space Agency

Name: XMM-RM: Quasar Accretion Physics in the Reverberation-Mapping Field
Published: 2017-02-25T23:00:00Z

Proposal ID	076508
Title	XMM-RM: Quasar Accretion Physics in the Reverberation-Mapping Field
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0765080101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0765080601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0765080801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0765080901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0765081001
DOI	https://doi.org/10.5270/esa-sh2r9tx
Principal Investigator, PI	Dr Paul Green
Abstract	To study the cosmic history of accretion, two reliable measurements are crucial:black hole mass and bolometric luminosity. Our SDSS Reverberation Mapping (RM)program is the first multi-object spectroscopic RM campaign, providingsignificantly improved BH mass estimates for a large sample of quasars toredshift 4 in a single field of 7 square degrees. Now with XMM-Newton, we willcharacterize the X-ray emission for about 700 of these quasars, enhancingmeasurements of bolometric luminosity and therefore Eddington ratio. From X-raybrightness, power-law slopes, and variability characteristics within the sample,we will also test accretion models in correlations that extend across the massrange, from Galactic X-ray binaries to quasars.
Publications	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 The Sloan Digital Sky Survey Reverberation Mapping Project: the XMM-Newton X-Ray Source Catalog and Multiband Counterparts \|Liu Teng Merloni Andrea et al. \| ApJS \| 250-32 \| 2020 \| 2020ApJS..250...32L \| http://ui.adsabs.harvard.edu/#abs/2020ApJS..250...32L 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 miniJPAS survey: AGN and host galaxy coevolution of X-ray-selected sources \|Lu00f3pez I. E. Brusa M. et al. \| A&A \| 672-137 \| 2023 \| 2023A&A...672A.137L \| http://ui.adsabs.harvard.edu/#abs/2023A&A...672A.137L The miniJPAS survey. Cluster and galaxy group detections with AMICO \|Maturi M. Finoguenov A. et al. \| A&A \| 678-145 \| 2023 \| 2023A&A...678A.145M \| http://ui.adsabs.harvard.edu/#abs/2023A&A...678A.145M 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2016-01-21T07:16:11Z/2016-01-27T20:03:09Z
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	"power law slopes", "xmm newton", "square degrees", "reliable measurements", "test accretion models", "enhancing measurements", "bolometric luminosity", "SDSS", "reverberation mapping field", "eddington ratio", "galactic xray binary", "mass range", "xray emission", "blackhole mass", "xmm rm", "xray brightness", "XMM-Newton", "single field", "cosmic history", "improved bh mass", "quasar accretion physics", "XMM", "variability characteristics"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Paul Green, 2017, 'XMM-RM: Quasar Accretion Physics in the Reverberation-Mapping Field', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-sh2r9tx