A dataset provided by the European Space Agency

Name: The most X-ray luminous QSOs from the ROSAT Bright Survey
Published: 2009-07-03T00:00:00Z

Proposal ID	055502
Title	The most X-ray luminous QSOs from the ROSAT Bright Survey
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0555020101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0555020201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0555020601
DOI	https://doi.org/10.5270/esa-vrje106
Principal Investigator, PI	Mr Mirko Krumpe
Abstract	We propose XMM EPIC spectroscopy of the five most X-ray luminous radio-quietQSOs found in the ROSAT Bright Survey (RBS). The RBS contains the brightestX-ray sources in the sky. Hence, the sample marks the high end of the local ( z<0.5 ) QSO luminosity function. Self-consistent disk reflection models predictstrong, neutral Fe lines emission in low X-ray luminosity AGN, while high X-rayluminous QSOs are expected to show weaker, high ionization Fe lines. A furtherincrease in X-ray luminosity elimates the Fe line emission (X-ray Baldwineffect). Observational evidence for these predictions are so far poorlyestablished and controversally discussed.
Publications	The XMM-Newton X-ray Spectra of the Most X-ray Luminous Radio-quiet ROSAT Bright Survey-QSOs: A Reference Sample for the Interpretation of High-redshift QSO Spectra \|Krumpe, M., Lamer, G., et al. \| ApJ \| 725-2444 \| 2010 \| 2010ApJ...725.2444K \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...725.2444K CAIXA: a catalogue of AGN in the XMM-Newton archive. III. Excess variance analysis \|Ponti, G., Papadakis, I., et al. \| A&A \| 542-83 \| 2012 \| 2012A&A...542A..83P \| http://ui.adsabs.harvard.edu/#abs/2012A&A...542A..83P Exospheric solar wind charge exchange as seen by XMM-Newton \|Carter, J. A., Semba, S., \| AN \| 333-313 \| 2012 \| 2012AN....333..313C \| http://ui.adsabs.harvard.edu/#abs/2012AN....333..313C The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive \|Clerc, N., Sadibekova, T., et al. \| MNRAS \| 423-3561 \| 2012 \| 2012MNRAS.423.3561C \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.3561C An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities \|Henley, David B., Shelton, Robin L., \| ApJS \| 202-14 \| 2012 \| 2012ApJS..202...14H \| http://ui.adsabs.harvard.edu/#abs/2012ApJS..202...14H Cross-calibration of the XMM-Newton EPIC pn and MOS on-axis effective areas using 2XMM sources \|Read, A. M., Guainazzi, M., \| A&A \| 564-75 \| 2014 \| 2014A&A...564A..75R \| http://ui.adsabs.harvard.edu/#abs/2014A&A...564A..75R Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov, V. N., \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y Missing cosmic metals revealed by X-ray absorption towards distant sources \|Campana, Sergio, Salvaterra, Ruben, et al. \| A&A \| 575-43 \| 2015 \| 2015A&A...575A..43C \| http://ui.adsabs.harvard.edu/#abs/2015A&A...575A..43C X-ray reverberation around accreting black holes \|Uttley, P., Cackett, E. M., et al. \| A&ARv \| 22-72 \| 2014 \| 2014A&ARv..22...72U \| http://ui.adsabs.harvard.edu/#abs/2014A&ARv..22...72U A New Sample of Obscured AGNs Selected from the XMM-Newton and AKARI Surveys \|Terashima, Yuichi, Hirata, Yoshitaka, et al. \| ApJ \| 814-11 \| 2015 \| 2015ApJ...814...11T \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...814...11T The Spatial Clustering of ROSAT All-Sky Survey Active Galactic Nuclei. IV. More Massive Black Holes Reside in More Massive Dark Matter Halos \|Krumpe, Mirko, Miyaji, Takamitsu, et al. \| ApJ \| 815-21 \| 2015 \| 2015ApJ...815...21K \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...815...21K The Interaction of the Fermi Bubbles with the Milky Way.s Hot Gas Halo \|Miller, Matthew J., Bregman, Joel N., \| ApJ \| 829-9 \| 2016 \| 2016ApJ...829....9M \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...829....9M SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV \|Clerc, N., Merloni, A., et al. \| MNRAS \| 463-4490 \| 2016 \| 2016MNRAS.463.4490C \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.463.4490C 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 Cosmology with XMM galaxy clusters: the X-CLASS/GROND catalogue and photometric redshifts \|Ridl, J., Clerc, N., et al. \| MNRAS \| 468-662 \| 2017 \| 2017MNRAS.468..662R \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.468..662R AGN spectral states from simultaneous UV and X-ray observations by XMM-Newton \|Svoboda, J., Guainazzi, M., \| A&A \| 603-127 \| 2017 \| 2017A&A...603A.127S \| http://ui.adsabs.harvard.edu/#abs/2017A&A...603A.127S The close environments of accreting massive black holes are shaped by radiative feedback \|Ricci, Claudio, Trakhtenbrot, Benny, et al. \| Natur \| 549-488 \| 2017 \| 2017Natur.549..488R \| http://ui.adsabs.harvard.edu/#abs/2017Natur.549..488R BAT AGN Spectroscopic Survey (BASS) - VI. The GammaX-L/LEdd relation \|Trakhtenbrot, Benny, Ricci, Claudio, et al. \| MNRAS \| 470-800 \| 2017 \| 2017MNRAS.470..800T \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.470..800T BAT AGN Spectroscopic Survey. V. X-Ray Properties of the Swift/BAT 70-month AGN Catalog \|Ricci, C., Trakhtenbrot, B., et al. \| ApJS \| 233-17 \| 2017 \| 2017ApJS..233...17R \| http://ui.adsabs.harvard.edu/#abs/2017ApJS..233...17R The Swift/BAT AGN Spectroscopic Survey. IX. The Clustering Environments of an Unbiased Sample of Local AGNs \|Powell, M. C., Cappelluti, N., et al. \| ApJ \| 858-110 \| 2018 \| 2018ApJ...858..110P \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...858..110P Hot corona properties of Swift/BAT-detected AGNs \|Wang, Chan, Yu, Li-Ming, et al. \| MNRAS \| 487-2463 \| 2019 \| 2019MNRAS.487.2463W \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.487.2463W X-ray properties of the X-CLASS-redMaPPer galaxy cluster sample: the luminosity-temperature relation \|Molham, Mona, Clerc, Nicolas, et al. \| MNRAS \| 494-161 \| 2020 \| 2020MNRAS.494..161M \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494..161M Multiwavelength classification of X-ray selected galaxy cluster candidates using convolutional neural networks \|Kosiba, Matej, Lieu, Maggie, et al. \| MNRAS \| 496-4141 \| 2020 \| 2020MNRAS.496.4141K \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.496.4141K SPIDERS: overview of the X-ray galaxy cluster follow-up and the final spectroscopic data release \|Clerc, N., Kirkpatrick, C. C., et al. \| MNRAS \| 497-3976 \| 2020 \| 2020MNRAS.497.3976C \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497.3976C An X-Ray- and SZ-bright Diffuse Source toward M31: A Local Hot Bridge \|Qu, Zhijie, Huang, Rui, et al. \| ApJ \| 907-14 \| 2021 \| 2021ApJ...907...14Q \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...907...14Q 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 Solar Cycle Temporal Variation of the Solar Wind Charge Exchange X-Ray Lines \|Qu, Zhijie, Koutroumpa, Dimitra, et al. \| ApJ \| 930-21 \| 2022 \| 2022ApJ...930...21Q \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...930...21Q Breaking the rules at z \\u2243 0.45: The rebel case of RBS 1055 \|Marinucci, A., Vietri, G., et al. \| A&A \| 666-169 \| 2022 \| 2022A&A...666A.169M \| http://ui.adsabs.harvard.edu/#abs/2022A&A...666A.169M 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	2008-05-15T14:08:21Z/2008-06-11T16:09:57Z
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	2009-07-03T00:00:00Z
Keywords	"rosat bright survey", "qso luminosity function", "XMM", "controversally discussed", "poorly established", "xray luminous qsos", "sample mar", "EPIC", "brightest xray sources", "xray luminosity elimates", "xmm epic spectroscopy", "ROSAT", "ionization fe lines"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mr Mirko Krumpe, 2009, 'The most X-ray luminous QSOs from the ROSAT Bright Survey', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-vrje106